List of exoplanets discovered in 2022

!Name

!data-sort-type="number"|Mass ({{Jupiter mass|link=yes}})

!data-sort-type="number"|Radius ({{Jupiter radius|link=yes}})

!data-sort-type="number"|Period (days)

!data-sort-type="number"|Semi-major axis (AU)

!data-sort-type="number"|Temp. (K)

!Discovery method

!data-sort-type="number"|Distance (ly)

!data-sort-type="number"|Host star mass ({{solar mass|link=yes}})

!data-sort-type="number"|Host star temp. (K)

!Remarks

|13.9{{±|6.1|5.1}}

|

|

|16.9{{±|3.4|1.9}}

|

| style="background:#909090" |astrometry + imaging

|130.9{{±|0.9}}

|2.14{{±|0.15}}

|8790{{±|1513|1292}}

|Host star also known as HIP 99770{{citation|arxiv=2212.00034|year=2023|title=Direct imaging and astrometric detection of a gas giant planet orbiting an accelerating star|last1=Currie |first1=Thayne |last2=Mirek Brandt |first2=G. |last3=Brandt |first3=Timothy D. |last4=Lacy |first4=Brianna |last5=Burrows |first5=Adam |last6=Guyon |first6=Olivier |last7=Tamura |first7=Motohide |last8=Liu |first8=Ranger Y. |last9=Sagynbayeva |first9=Sabina |last10=Tobin |first10=Taylor |last11=Chilcote |first11=Jeffrey |last12=Groff |first12=Tyler |last13=Marois |first13=Christian |last14=Thompson |first14=William |last15=Murphy |first15=Simon |last16=Kuzuhara |first16=Masayuki |last17=Lawson |first17=Kellen |last18=Lozi |first18=Julien |last19=Deo |first19=Vincent |last20=Vievard |first20=Sebastien |last21=Skaf |first21=Nour |last22=Uyama |first22=Taichi |last23=Jovanovic |first23=Nemanja |last24=Martinache |first24=Frantz |last25=Jeremy Kasdin |first25=N. |last26=Kudo |first26=Tomoyuki |last27=McElwain |first27=Michael |last28=Janson |first28=Markus |last29=Wisniewski |first29=John |last30=Hodapp |first30=Klaus |journal=Science |volume=380 |issue=6641 |pages=198–203 |doi=10.1126/science.abo6192 |pmid=37053312 |bibcode=2023Sci...380..198C |s2cid=258108042 |display-authors=1 }}

|1.10{{±|0.37}}

|1.68{{±|0.11}}

|3.22748{{±|0.00008}}

|0.04290{{±|0.00092}}

|1747{{±|62}}

| style="background:#FFFF00" |transit

|3700{{±|200}}

|1.01{{±|0.07|0.06}}

|6390{{±|130}}

|{{citation|arxiv=2207.08742|year=2022|title=Sub-stellar companions of intermediate-mass stars with CoRoT: CoRoT–34b, CoRoT–35b, and CoRoT–36b|doi=10.1093/mnras/stac2131 |last1=Sebastian |first1=D. |last2=Guenther |first2=E. W. |last3=Deleuil |first3=M. |last4=Dorsch |first4=M. |last5=Heber |first5=U. |last6=Heuser |first6=C. |last7=Gandolfi |first7=D. |last8=Grziwa |first8=S. |last9=Deeg |first9=H. J. |last10=Alonso |first10=R. |last11=Bouchy |first11=F. |last12=Csizmadia |first12=Sz |last13=Cusano |first13=F. |last14=Fridlund |first14=M. |last15=Geier |first15=S. |last16=Irrgang |first16=A. |last17=Korth |first17=J. |last18=Nespral |first18=D. |last19=Rauer |first19=H. |last20=Tal-Or |first20=L. |journal=Monthly Notices of the Royal Astronomical Society |volume=516 |pages=636–655 |doi-access=free }}

|0.68{{±|0.47|0.43}}

|1.41{{±|0.14}}

|5.616531{{±|0.000023}}

|0.066{{±|0.007}}

|1567{{±|35}}

| style="background:#FFFF00" |transit

|3110{{±|60}}

|1.32{{±|0.09}}

|6730{{±|140}}

|

|0.0168{{±|0.098}}

|0.186{{±|0.015|0.014}}

|17.51547{{±|0.00228|0.00296}}

|

|570

| style="background:#FFFF00" |transit

|

|0.832{{±|0.253|0.367}}

|4752{{±|138}}

|

|

|0.088{{±|0.004}}

|3.2141±0.0002

|0.0511{{±|0.0021|0.0028}}

|

| style="background:#FFFF00" |transit

|965

|1.018{{±|0.131}}

|5711{{±|105}}

|{{citation|arxiv=2210.10805|year=2023|title=TFAW survey II: Six newly validated planets and 13 planet candidates from K2|doi=10.1093/mnras/stac3087 |last1=Del Ser |first1=D. |last2=Fors |first2=O. |last3=Del Alcázar |first3=M. |last4=Dyachenko |first4=V. |last5=Horch |first5=E. P. |last6=Tokovinin |first6=A. |last7=Ziegler |first7=C. |last8=Van Belle |first8=G. T. |last9=Clark |first9=C. A. |last10=Hartman |first10=Z. D. |journal=Monthly Notices of the Royal Astronomical Society |volume=518 |pages=669–690 |doi-access=free }}

|

|0.068{{±|0.007}}

|0.8094{{±|0.00003}}

|0.0117{{±|0.0009|0.0012}}

|

| style="background:#FFFF00" |transit

|954

|0.808{{±|0.364|0.256}}

|4116{{±|138}}

|

|

|0.110{{±|0.006}}

|5.3301{{±|0.0003}}

|0.0426{{±|0.0016|0.0019}}

|

| style="background:#FFFF00" |transit

|954

|0.808{{±|0.364|0.256}}

|4116{{±|138}}

|

|

|0.172{{±|0.006}}

|6.6690{{±|0.0002}}

|0.0552{{±|0.0017|0.0023}}

|

| style="background:#FFFF00" |transit

|835

|0.814{{±|0.363|0.251}}

|4343{{±|138}}

|

|

|0.109{{±|0.006}}

|4.3696{{±|0.0001}}

|0.0487{{±|0.0027|0.0031}}

|

| style="background:#FFFF00" |transit

|835

|0.814{{±|0.363|0.251}}

|4343{{±|138}}

|

|

|0.189{{±|0.009}}

|5.9382{{±|0.0006|0.0004}}

|0.0586{{±|0.0032|0.0033}}

|

| style="background:#FFFF00" |transit

|2181

|0.893{{±|0.406|0.275}}

|5590{{±|138}}

|

|1.68{{±|0.11}}

|1.229{{±|0.021}}

|3.052524{{±|0.000017}}

|0.04047{{±|0.00094}}

|

| style="background:#FFFF00" |transit

|1201{{±|7}}

|0.949{{±|0.066}}

|5470{{±|110}}

|First confirmed exoplanet discovered by Gaia, along with Gaia-2b{{cite journal |arxiv=2205.10197|doi=10.1051/0004-6361/202243497 |title=The detection of transiting exoplanets by Gaia |year=2022 |last1=Panahi |first1=Aviad |last2=Zucker |first2=Shay |last3=Clementini |first3=Gisella |last4=Audard |first4=Marc |last5=Binnenfeld |first5=Avraham |last6=Cusano |first6=Felice |last7=Evans |first7=Dafydd Wyn |last8=Gomel |first8=Roy |last9=Holl |first9=Berry |last10=Ilyin |first10=Ilya |last11=De Fombelle |first11=Grégory Jevardat |last12=Mazeh |first12=Tsevi |last13=Mowlavi |first13=Nami |last14=Nienartowicz |first14=Krzysztof |last15=Rimoldini |first15=Lorenzo |last16=Shahaf |first16=Sahar |last17=Eyer |first17=Laurent |journal=Astronomy & Astrophysics |volume=663 |pages=A101 |bibcode=2022A&A...663A.101P |s2cid=248965147 }}

|0.817{{±|0.047}}

|1.322{{±|0.013}}

|3.6915224{{±|0.0000039}}

|0.0467{{±|0.0015}}

|

| style="background:#FFFF00" |transit

|676{{±|3}}

|1.000{{±|0.095}}

|5720{{±|84}}

|First confirmed exoplanet discovered by Gaia, along with Gaia-1b

|0.0164{{±|0.0028}}

|

|140.43{{±|0.41}}

|0.422{{±|0.014|0.015}}

|202{{±|11}}

| style="background:#00FF00" |radial vel.

|24.850{{±|0.010}}

|0.510{{±|0.051}}

|3714{{±|51}}

|Planetary orbit partially in habitable zone{{citation|arxiv=2204.06376|year=2022|title=A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514|last1=Damasso |first1=M. |last2=Perger |first2=M. |last3=Almenara |first3=J. M. |last4=Nardiello |first4=D. |last5=Pérez-Torres |first5=M. |last6=Sozzetti |first6=A. |last7=Hara |first7=N. C. |last8=Quirrenbach |first8=A. |last9=Bonfils |first9=X. |last10=Zapatero Osorio |first10=M. R. |last11=Astudillo-Defru |first11=N. |last12=González Hernández |first12=J. I. |last13=Suárez Mascareño |first13=A. |last14=Amado |first14=P. J. |last15=Forveille |first15=T. |last16=Lillo-Box |first16=J. |last17=Alibert |first17=Y. |last18=Caballero |first18=J. A. |last19=Cifuentes |first19=C. |last20=Delfosse |first20=X. |last21=Figueira |first21=P. |last22=Galadí-Enríquez |first22=D. |last23=Hatzes |first23=A. P. |last24=Henning |first24=Th. |last25=Kaminski |first25=A. |last26=Mayor |first26=M. |last27=Murgas |first27=F. |last28=Montes |first28=D. |last29=Pinamonti |first29=M. |last30=Reiners |first30=A. |journal=Astronomy & Astrophysics |volume=666 |pages=A187 |doi=10.1051/0004-6361/202243522 |s2cid=248157318 |display-authors=1 }}

|0.0034{{±|0.0004}}

|

|10.3465{{±|0.027}}

|0.0457{{±|0.0013}}

|230.9{{±|6.7}}

| style="background:#00FF00" |radial vel.

|15.808{{±|0.003}}

|0.120{{±|0.010}}

|3024{{±|52}}

|Planet in habitable zone{{citation|arxiv=2212.07332|year=2022|title=Two temperate Earth-mass planets orbiting the nearby star GJ 1002|doi=10.1051/0004-6361/202244991 |last1=Suárez Mascareño |first1=A. |last2=González-Alvarez |first2=E. |last3=Zapatero Osorio |first3=M. R. |last4=Lillo-Box |first4=J. |last5=Faria |first5=J. P. |last6=Passegger |first6=V. M. |last7=González Hernández |first7=J. I. |last8=Figueira |first8=P. |last9=Sozzetti |first9=S. |last10=Rebolo |first10=R. |last11=Pepe |first11=F. |last12=Santos |first12=N. C. |last13=Cristiani |first13=S. |last14=Lovis |first14=C. |last15=Silva |first15=A. M. |last16=Ribas |first16=I. |last17=Amado |first17=P. J. |last18=Caballero |first18=J. A. |last19=Quirrenbach |first19=A. |last20=Reiners |first20=A. |last21=Zechmeister |first21=M. |last22=Adibekyan |first22=V. |last23=Alibert |first23=Y. |last24=Béjar |first24=V. J. S. |last25=Benatti |first25=S. |last26=D'Odorico |first26=V. |last27=Damasso |first27=M. |last28=Delisle |first28=J. -B. |last29=Dreizler |first29=P. Di Marcantonio S. |last30=Ehrenreich |first30=D. |display-authors=1 |journal=Astronomy & Astrophysics |volume=670 |pages=A5 |s2cid=254353639 }}

|0.0043{{±|0.0005}}

|

|21.202{{±|0.013}}

|0.0738{{±|0.0021}}

|181.7{{±|5.2}}

| style="background:#00FF00" |radial vel.

|15.808{{±|0.003}}

|0.120{{±|0.010}}

|3024{{±|52}}

|Planet in habitable zone

|0.0055{{±|0.0014}}

|0.097{{±|0.004}}

|2.6162745{{±|0.000003}}

|0.0252{{±|0.0005}}

|568{{±|6}}

| style="background:#FFFF00" |transit

|51.64{{±|0.02}}

|0.309{{±|0.014}}

|3369{{±|51}}

|Another planet in system is suspected{{citation|arxiv=2202.00970|year=2022|title=Discovery and mass measurement of the hot, transiting, Earth-sized planet, GJ 3929 B|doi=10.1051/0004-6361/202142653 |last1=Kemmer |first1=J. |last2=Dreizler |first2=S. |last3=Kossakowski |first3=D. |last4=Stock |first4=S. |last5=Quirrenbach |first5=A. |last6=Caballero |first6=J. A. |last7=Amado |first7=P. J. |last8=Collins |first8=K. A. |last9=Espinoza |first9=N. |last10=Herrero |first10=E. |last11=Jenkins |first11=J. M. |last12=Latham |first12=D. W. |last13=Lillo-Box |first13=J. |last14=Narita |first14=N. |last15=Pallé |first15=E. |last16=Reiners |first16=A. |last17=Ribas |first17=I. |last18=Ricker |first18=G. |last19=Rodríguez |first19=E. |last20=Seager |first20=S. |last21=Vanderspek |first21=R. |last22=Wells |first22=R. |last23=Winn |first23=J. |last24=Aceituno |first24=F. J. |last25=Béjar |first25=V. J. S. |last26=Barclay |first26=T. |last27=Bluhm |first27=P. |last28=Chaturvedi |first28=P. |last29=Cifuentes |first29=C. |last30=Collins |first30=K. I. |journal=Astronomy & Astrophysics |volume=659 |pages=A17 |bibcode=2022A&A...659A..17K |s2cid=246473345 |display-authors=1 }}

|0.0180{{±|0.0029}}

|

|15.04{{±|0.03}}

|0.081{{±|0.002}}

|317{{±|3}}

| style="background:#00FF00" |radial vel.

|51.64{{±|0.02}}

|0.309{{±|0.014}}

|3369{{±|51}}

|{{citation|arxiv=2207.10672|year=2022|title=GJ 3929: High-precision Photometric and Doppler Characterization of an Exo-Venus and Its Hot, Mini-Neptune-mass Companion|doi=10.3847/1538-4357/ac8480 |last1=Beard |first1=Corey |last2=Robertson |first2=Paul |last3=Kanodia |first3=Shubham |last4=Lubin |first4=Jack |last5=Cañas |first5=Caleb I. |last6=Gupta |first6=Arvind F. |last7=Holcomb |first7=Rae |last8=Jones |first8=Sinclaire |last9=Libby-Roberts |first9=Jessica E. |last10=Lin |first10=Andrea S. J. |last11=Mahadevan |first11=Suvrath |last12=Stefánsson |first12=Guđmundur |last13=Bender |first13=Chad F. |last14=Blake |first14=Cullen H. |last15=Cochran |first15=William D. |last16=Endl |first16=Michael |last17=Everett |first17=Mark |last18=Ford |first18=Eric B. |last19=Fredrick |first19=Connor |last20=Halverson |first20=Samuel |last21=Hebb |first21=Leslie |last22=Li |first22=Dan |last23=Logsdon |first23=Sarah E. |last24=Luhn |first24=Jacob |last25=McElwain |first25=Michael W. |last26=Metcalf |first26=Andrew J. |last27=Ninan |first27=Joe P. |last28=Rajagopal |first28=Jayadev |last29=Roy |first29=Arpita |last30=Schutte |first30=Maria |journal=The Astrophysical Journal |volume=936 |issue=1 |page=55 |bibcode=2022ApJ...936...55B |s2cid=251018402 |display-authors=1 |doi-access=free }}

|3.6{{±|0.4}}

|

|3448{{±|110|88}}

|3.53{{±|0.07}}

|

| style="background:#00FF00" |radial vel.

|59.91{{±|0.03}}

|0.49{{±|0.02}}

|3540{{±|41}}

|Host star also known as Ross 690[https://iopscience.iop.org/article/10.3847/1538-3881/ac8e05/pdf A Jupiter Analog Orbiting The Nearby M Dwarf GJ 463]{{citation|arxiv=2302.00413|year=2023|title=A dynamical mass for GJ 463 b: A massive super-Jupiter companion beyond the snow line of a nearby M dwarf|doi=10.1051/0004-6361/202245454 |last1=Sozzetti |first1=A. |journal=Astronomy & Astrophysics |volume=670 |pages=L17 |bibcode=2023A&A...670L..17S |s2cid=256253670 }}

|0.0105

|0.19

|2.8531042{{±|0.0000032}}

|0.03165

|696

| style="background:#FFFF00" |transit

|73.21{{±|0.04}}

|0.519{{±|0.013}}

|3556{{±|70}}

|Host star also known as TOI-177{{citation|arxiv=2207.14121|year=2022|title=GJ 3090 b: One of the most favourable mini-Neptune for atmospheric characterisation|doi=10.1051/0004-6361/202243975 |last1=Almenara |first1=J. M. |last2=Bonfils |first2=X. |last3=Otegi |first3=J. F. |last4=Attia |first4=O. |last5=Turbet |first5=M. |last6=Astudillo-Defru |first6=N. |last7=Collins |first7=K. A. |last8=Polanski |first8=A. S. |last9=Bourrier |first9=V. |last10=Hellier |first10=C. |last11=Ziegler |first11=C. |last12=Bouchy |first12=F. |last13=Briceno |first13=C. |last14=Charbonneau |first14=D. |last15=Cointepas |first15=M. |last16=Collins |first16=K. I. |last17=Crossfield |first17=I. |last18=Delfosse |first18=X. |last19=Diaz |first19=R. F. |last20=Dorn |first20=C. |last21=Doty |first21=J. P. |last22=Forveille |first22=T. |last23=Gaisné |first23=G. |last24=Gan |first24=T. |last25=Helled |first25=R. |last26=Hesse |first26=K. |last27=Jenkins |first27=J. M. |last28=Jensen |first28=E. L. N. |last29=Latham |first29=D. W. |last30=Law |first30=N. |journal=Astronomy & Astrophysics |volume=665 |pages=A91 |bibcode=2022A&A...665A..91A |s2cid=252367299 |display-authors=1 }}

|0.0538

|

|12.734{{±|0.033|0.026}}

|0.08575

|421

| style="background:#00FF00" |radial vel.

|73.21{{±|0.04}}

|0.519{{±|0.013}}

|3556{{±|70}}

|Host star also known as TOI-177

|0.0306{{±|0.0037}}

|

|102.09{{±|0.52|0.50}}

|0.4048{{±|0.0077|0.0074}}

|375{{±|7}}

| style="background:#00FF00" |radial vel.

|154.59{{±|0.13}}

|0.852{{±|0.026|0.015}}

|5300{{±|73}}

|{{citation|arxiv=2209.06937|year=2022|title=A CHEOPS-enhanced view of the HD 3167 system|last1=Bourrier |first1=V. |last2=Deline |first2=A. |last3=Krenn |first3=A. |last4=Egger |first4=J. A. |last5=Petit |first5=A. C. |last6=Malavolta |first6=L. |last7=Cretignier |first7=M. |last8=Billot |first8=N. |last9=Broeg |first9=C. |last10=Florén |first10=H. -G. |last11=Queloz |first11=D. |last12=Alibert |first12=Y. |last13=Bonfanti |first13=A. |last14=Bonomo |first14=A. S. |last15=Delisle |first15=J. -B. |last16=Demangeon |first16=O. D. S. |last17=Demory |first17=B. -O. |last18=Dumusque |first18=X. |last19=Ehrenreich |first19=D. |last20=Haywood |first20=R. D. |last21=B Howell |first21=S. |last22=Lendl |first22=M. |last23=Mortier |first23=A. |last24=Nigro |first24=G. |last25=Salmon |first25=S. |last26=Sousa |first26=S. G. |last27=Wilson |first27=T. G. |last28=Adibekyan |first28=V. |last29=Alonso |first29=R. |last30=Anglada |first30=G. |journal=Astronomy & Astrophysics |volume=668 |pages=A31 |doi=10.1051/0004-6361/202243778 |bibcode=2022A&A...668A..31B |s2cid=251861892 |display-authors=1 }}

|0.0758{{±|0.0223|0.0242}}

|0.232{{±|0.012}}

|4.1374354{{±|0.0000036|0.0000037}}

|0.0480{{±|0.0004}}

|935{{±|11}}

| style="background:#FFFF00" |transit

|126.02{{±|0.06}}

|0.863{{±|0.020}}

|5145{{±|50}}

|Host star also known as TOI-179, also red dwarf star in the system{{citation|arxiv=2210.07933|year=2023|title=TOI-179: A young system with a transiting compact Neptune-mass planet and a low-mass companion in outer orbit|last1=Desidera |first1=S. |last2=Damasso |first2=M. |last3=Gratton |first3=R. |last4=Benatti |first4=S. |last5=Nardiello |first5=D. |last6=D'Orazi |first6=V. |last7=Lanza |first7=A. F. |last8=Locci |first8=D. |last9=Marzari |first9=F. |last10=Mesa |first10=D. |last11=Messina |first11=S. |last12=Pillitteri |first12=I. |last13=Sozzetti |first13=A. |last14=Girard |first14=J. |last15=Maggio |first15=A. |last16=Micela |first16=G. |last17=Malavolta |first17=L. |last18=Nascimbeni |first18=V. |last19=Pinamonti |first19=M. |last20=Squicciarini |first20=V. |last21=Alcala |first21=J. |last22=Biazzo |first22=K. |last23=Bohn |first23=A. |last24=Bonavita |first24=M. |last25=Brooks |first25=K. |last26=Chauvin |first26=G. |last27=Covino |first27=E. |last28=Delorme |first28=P. |last29=Hagelberg |first29=J. |last30=Janson |first30=M. |journal=Astronomy & Astrophysics |volume=675 |pages=A158 |doi=10.1051/0004-6361/202244611 |bibcode=2023A&A...675A.158D |s2cid=252907692 |display-authors=1 }}{{citation|arxiv=2210.08179|year=2023|title=A sub-Neptune transiting the young field star HD 18599 at 40 pc|last1=de Leon |first1=Jerome P. |last2=Livingston |first2=John H. |last3=Jenkins |first3=James S. |last4=Vines |first4=Jose I. |last5=Wittenmyer |first5=Robert A. |last6=Clark |first6=Jake T. |last7=Winn |first7=Joshua I. M. |last8=Addison |first8=Brett |last9=Ballard |first9=Sarah |last10=Bayliss |first10=Daniel |last11=Beichman |first11=Charles |last12=Benneke |first12=Björn |author13=David Anthony Berardo |last14=Bowler |first14=Brendan P. |last15=Brown |first15=Tim |last16=Bryant |first16=Edward M. |last17=Christiansen |first17=Jessie |last18=Ciardi |first18=David |last19=Collins |first19=Karen A. |last20=Collins |first20=Kevin I. |last21=Crossfield |first21=Ian |last22=Deming |first22=Drake |last23=Dragomir |first23=Diana |last24=Dressing |first24=Courtney D. |last25=Fukui |first25=Akihiko |last26=Gan |first26=Tianjun |last27=Giacalone |first27=Steven |last28=Gill |first28=Samuel |author29=Erica Gonz\' alez Alvarez |last30=Hesse |first30=Katharine |journal=Monthly Notices of the Royal Astronomical Society |volume=522 |pages=750–766 |doi=10.1093/mnras/stad894 |doi-access=free |display-authors=1 }}{{citation|arxiv=2210.07945|year=2022|title=A dense mini-Neptune orbiting the bright young star HD 18599|doi=10.1093/mnras/stac2845 |last1=Vines |first1=Jose I. |last2=Jenkins |first2=James S. |last3=Berdiñas |first3=Zaira |last4=Soto |first4=Maritza G. |last5=Díaz |first5=Matías R. |last6=Alves |first6=Douglas R. |last7=Tuomi |first7=Mikko |last8=Wittenmyer |first8=Robert A. |last9=De Leon |first9=Jerome Pitogo |last10=Peña |first10=Pablo |last11=Lissauer |first11=Jack J. |last12=Ballard |first12=Sarah |last13=Bedding |first13=Timothy |last14=Bowler |first14=Brendan P. |last15=Horner |first15=Jonathan |last16=Jones |first16=Hugh R A. |last17=Kane |first17=Stephen R. |last18=Kielkopf |first18=John |last19=Plavchan |first19=Peter |last20=Shporer |first20=Avi |last21=Tinney |first21=C. G. |last22=Wright |first22=Hui Zhang Duncan J. |last23=Addison |first23=Brett |last24=Mengel |first24=Matthew W. |last25=Okumura |first25=Jack |last26=Samadi-Ghadim |first26=Anya |journal=Monthly Notices of the Royal Astronomical Society |volume=518 |issue=2 |pages=2627–2639 |doi-access=free }}

|0.0233{{±|0.0034}}

|0.154{{±|0.006}}

|0.926118{{±|0.000050|0.000043}}

|0.0180{{±|0.0003}}

|2141{{±|27}}

| style="background:#FFFF00" |transit

|207.7{{±|0.9}}

|0.90{{±|0.05}}

|5596{{±|50}}

|{{citation|arxiv=2211.02547|year=2022|title=HD 20329b: An ultra-short-period planet around a solar-type star found by TESS|last1=Murgas |first1=F. |last2=Nowak |first2=G. |last3=Masseron |first3=T. |last4=Parviainen |first4=H. |last5=Luque |first5=R. |last6=Pallé |first6=E. |last7=Korth |first7=Judith |last8=Carleo |first8=I. |last9=Csizmadia |first9=Sz. |last10=Esparza-Borges |first10=E. |last11=Alqasim |first11=Ahlam |last12=Cochran |first12=William D. |last13=Dai |first13=Fei |last14=Deeg |first14=Hans J. |last15=Gandolfi |first15=D. |last16=Goffo |first16=Elisa |last17=Kabáth |first17=Petr |last18=Lam |first18=K. W. F. |last19=Livingston |first19=John |last20=Muresan |first20=Alexandra |last21=Osborne |first21=H. L. M. |last22=Persson |first22=Carina M. |last23=Serrano |first23=L. M. |last24=Smith |first24=Alexis M. S. |author25=Vincent Van Eylen |last26=Orell-Miquel |first26=J. |last27=Hinkel |first27=Natalie R. |last28=Galán |first28=D. |last29=Puig-Subirà |first29=M. |last30=Stangret |first30=M. |journal=Astronomy & Astrophysics |volume=668 |pages=A158 |doi=10.1051/0004-6361/202244459 |bibcode=2022A&A...668A.158M |s2cid=253370507 |display-authors=1 }}

|2.12{{±|0.09}}

|

|872.6{{±|2.8}}

|1.900{{±|0.004}}

|

|style="background:#00FF00"|radial vel.

|526{{±|2}}

|1.20{{±|0.05}}

|5067{{±|59|22}}

|Giant host star{{cite journal|last1=Ottoni|first1=G.|last2=Udry|first2=S.|last3=Ségransan|first3=D.|last4=Buldgen|first4=G.|last5=Lovis|first5=C.|last6=Eggenberger|first6=P.|last7=Pezzotti|first7=C.|last8=Adibekyan|first8=V.|last9=Marmier|first9=M.|last10=Mayor|first10=M.|last11=Santos|first11=N.C.|last12=Sousa|first12=S.G.|last13=Lagarde|first13=N.|last14=Charbonnel|first14=C.|display-authors=3|title=CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars|journal=Astronomy & Astrophysics|year=2022|volume=657 |pages=A87 |issn=0004-6361|arxiv=2201.01528|doi=10.1051/0004-6361/202040078|bibcode=2022A&A...657A..87O |doi-access=|s2cid=245440163}}

|

|0.154{{±|0.009}}

|4.040301{{±|0.000023|0.000042}}

|0.0528{{±|0.0030}}

|1378{{±|36}}

| style="background:#FFFF00" |transit

|205.08{{±|0.16}}

|1.158{{±|0.058}}

|6210{{±|173|158}}

|Host star also known as TOI-411, third transiting planet in system is suspected{{citation|arxiv=2209.09597|year=2022|title=TESS discovery of a super-Earth and two sub-Neptunes orbiting the bright, nearby, Sun-like star HD 22946|last1=Cacciapuoti |first1=Luca |last2=Inno |first2=Laura |last3=Covone |first3=Giovanni |last4=Kostov |first4=Veselin B. |last5=Barclay |first5=Thomas |last6=Quintana |first6=Elisa V. |last7=Colon |first7=Knicole D. |last8=Stassun |first8=Keivan G. |last9=Hord |first9=Benjamin |last10=Giacalone |first10=Steven |last11=Kane |first11=Stephen R. |last12=Hoffman |first12=Kelsey |last13=Rowe |first13=Jason |last14=Wang |first14=Gavin |last15=Collins |first15=Kevin I. |last16=Collins |first16=Karen A. |last17=Tan |first17=Thiam-Guan |last18=Gallo |first18=Francesco |last19=Magliano |first19=Christian |last20=Ienco |first20=Riccardo M. |last21=Rabus |first21=Markus |last22=Ciardi |first22=David R. |last23=Furlan |first23=Elise |last24=Howell |first24=Steve B. |last25=Gnilka |first25=Crystal L. |last26=Scott |first26=Nicholas J. |last27=Lester |first27=Kathryn V. |last28=Ziegler |first28=Carl |last29=Briceño |first29=César |last30=Law |first30=Nicholas |journal=Astronomy & Astrophysics |volume=668 |pages=A85 |doi=10.1051/0004-6361/202243565 |bibcode=2022A&A...668A..85C |s2cid=252383725 |display-authors=1 }}

|

|0.245{{±|0.013}}

|9.573096{{±|0.000026|0.000023}}

|0.0939{{±|0.0054}}

|1033{{±|27}}

| style="background:#FFFF00" |transit

|205.08{{±|0.16}}

|1.158{{±|0.058}}

|6210{{±|173|158}}

|Host star also known as TOI-411, third transiting planet in system is suspected

|0.0017{{±|0.0006}}

|0.067{{±|0.005}}

|3.97664{{±|0.000030|0.000044}}

|0.04298{{±|0.00063|0.00065}}

|909{{±|35|32}}

| style="background:#FFFF00" |transit

|127.48{{±|0.06}}

|0.67{{±|0.03}}

|4684{{±|99}}

|{{citation|arxiv=2209.13345|year=2022|title=HD 23472: A multi-planetary system with three super-Earths and two potential super-Mercuries|doi=10.1051/0004-6361/202244293 |last1=Barros |first1=S. C. C. |last2=Demangeon |first2=O. D. S. |last3=Alibert |first3=Y. |last4=Leleu |first4=A. |last5=Adibekyan |first5=V. |last6=Lovis |first6=C. |last7=Bossini |first7=D. |last8=Sousa |first8=S. G. |last9=Hara |first9=N. |last10=Bouchy |first10=F. |last11=Lavie |first11=B. |last12=Rodrigues |first12=J. |last13=Da Silva |first13=J. Gomes |last14=Lillo-Box |first14=J. |last15=Pepe |first15=F. A. |last16=Tabernero |first16=H. M. |last17=Osorio |first17=M. R. Zapatero |last18=Sozzetti |first18=A. |last19=Mascareño |first19=A. Suárez |last20=Micela |first20=G. |last21=Prieto |first21=C. Allende |last22=Cristiani |first22=S. |last23=Damasso |first23=M. |last24=Di Marcantonio |first24=P. |last25=Ehrenreich |first25=D. |last26=Faria |first26=J. |last27=Figueira |first27=P. |last28=Hernández |first28=J. I. González |last29=Jenkins |first29=J. |last30=Lo Curto |first30=G. |journal=Astronomy & Astrophysics |volume=665 |pages=A154 |bibcode=2022A&A...665A.154B |s2cid=251463803 |display-authors=1 }}

|0.0023{{±|0.0009}}

|0.073{{±|0.006}}

|7.90754{{±|0.00011}}

|0.0680{{±|0.0010}}

|723{{±|28|25}}

| style="background:#FFFF00" |transit

|127.48{{±|0.06}}

|0.67{{±|0.03}}

|4684{{±|99}}

|

|0.0024{{±|0.0013}}

|0.102{{±|0.007}}

|12.1621839{{±|0.00012|0.000099}}

|0.0906{{±|0.0014}}

|630{{±|27|23}}

| style="background:#FFFF00" |transit

|127.48{{±|0.06}}

|0.67{{±|0.03}}

|4684{{±|99}}

|

|0.058{{±|0.029|0.024}}

|0.196{{±|0.009}}

|22.89104{{±|0.00035|0.00036}}

|0.1357{{±|0.0034}}

|881.2{{±|7.5}}

| style="background:#FFFF00" |transit

|457.0{{±|0.6}}

|1.26{{±|0.08}}

|6120{{±|50}}

|{{citation|arxiv=2205.09046|year=2022|title=HD 28109 hosts a trio of transiting Neptunian planets including a near-resonant pair, confirmed by ASTEP from Antarctica|last1=Dransfield |first1=Georgina |last2=Triaud |first2=Amaury H. M. J. |last3=Guillot |first3=Tristan |last4=Mekarnia |first4=Djamel |last5=Nesvorný |first5=David |last6=Crouzet |first6=Nicolas |last7=Abe |first7=Lyu |last8=Agabi |first8=Karim |last9=Buttu |first9=Marco |last10=Cabrera |first10=Juan |last11=Gandolfi |first11=Davide |last12=Günther |first12=Maximilian N. |last13=Rodler |first13=Florian |last14=Schmider |first14=François-Xavier |last15=Stee |first15=Philippe |last16=Suarez |first16=Olga |last17=Collins |first17=Karen A. |last18=Dévora-Pajares |first18=Martín |last19=Howell |first19=Steve B. |last20=Matthews |first20=Elisabeth C. |last21=Standing |first21=Matthew R. |last22=Stassun |first22=Keivan G. |last23=Stockdale |first23=Chris |last24=Quinn |first24=Samuel N. |last25=Ziegler |first25=Carl |last26=Crossfield |first26=Ian J. M. |last27=Lissauer |first27=Jack J. |last28=Mann |first28=Andrew W. |last29=Matson |first29=Rachel |last30=Schlieder |first30=Joshua |journal=Monthly Notices of the Royal Astronomical Society |volume=515 |pages=1328–1345 |doi=10.1093/mnras/stac1383 |doi-access=free |display-authors=1 }}

|0.025{{±|0.013|0.010}}

|0.378{{±|0.010}}

|56.00819{{±|0.00194|0.00202}}

|0.308{{±|0.011}}

|585.2{{±|8.7|8.3}}

| style="background:#FFFF00" |transit

|457.0{{±|0.6}}

|1.26{{±|0.08}}

|6120{{±|50}}

|

|0.018{{±|0.009|0.007}}

|0.290{{±|0.010}}

|84.25999{{±|0.00744|0.00662}}

|0.411{{±|0.016}}

|506.5{{±|8.7|8.0}}

| style="background:#FFFF00" |transit

|457.0{{±|0.6}}

|1.26{{±|0.08}}

|6120{{±|50}}

|

|1.57{{±|0.11}}

|

|892.7{{±|5.9}}

|1.913{{±|0.008}}

|

| style="background:#00FF00" |radial vel.

|144.2{{±|0.3}}

|1.15{{±|0.04}}

|4845{{±|52}}

|Giant host star{{cite journal|last1=Pezzotti|first1=C.|last2=Ottoni|first2=G.|last3=Buldgen|first3=G.|last4=Lyttle|first4=A.|last5=Eggenberger|first5=P.|last6=Udry|first6=S.|last7=Ségransan|first7=D.|last8=Mayor|first8=M.|last9=Lovis|first9=C.|last10=Marmier|first10=M.|last11=Miglio|first11=A.|last12=Elsworth|first12=Y.|last13=Davies|first13=G. R.|last14=Ball|first14=W. H.|display-authors=3|title=Coralie radial-velocity search for companions around evolved stars (CASCADES). III. A new Jupiter host-star: in-depth analysis of HD29399 using TESS data|journal=Astronomy & Astrophysics|publisher=EDP Sciences|date=2021-04-22|volume=657 |pages=A89 |issn=0004-6361|arxiv=2201.01553|doi=10.1051/0004-6361/202040080|s2cid=242974999}}

|0.89{{±|0.06|0.05}}

|

|810.2{{±|3.8|4.2}}

|1.955{{±|0.016|0.012}}

|

| style="background:#00FF00" |radial vel.

|394.3{{±|0.9}}

|1.52{{±|0.03}}

|5025.4{{±|23.6|15.5}}

|Giant host star{{citation|arxiv=2206.03899|year=2022|title=A New Third Planet and the Dynamical Architecture of the HD 33142 Planetary System|doi=10.3847/1538-3881/ac7ce0 |last1=Trifonov |first1=Trifon |last2=Wollbold |first2=Anna |last3=Kürster |first3=Martin |last4=Eberhardt |first4=Jan |last5=Stock |first5=Stephan |last6=Henning |first6=Thomas |last7=Reffert |first7=Sabine |last8=Butler |first8=R. Paul |last9=Vogt |first9=Steven S. |last10=Reiners |first10=Ansgar |last11=Lee |first11=Man Hoi |last12=Bitsch |first12=Bertram |last13=Zechmeister |first13=Mathias |last14=Rodler |first14=Florian |last15=Perdelwitz |first15=Volker |last16=Tal-Or |first16=Lev |last17=Rybizki |first17=Jan |last18=Heeren |first18=Paul |last19=Gandolfi |first19=Davide |last20=Barragán |first20=Oscar |last21=Zakhozhay |first21=Olga |last22=Sarkis |first22=Paula |last23=Pinto |first23=Marcelo Tala |last24=Kossakowski |first24=Diana |last25=Wolthoff |first25=Vera |last26=Brems |first26=Stefan S. |last27=Passegger |first27=Vera Maria |journal=The Astronomical Journal |volume=164 |issue=4 |page=156 |bibcode=2022AJ....164..156T |s2cid=249461702 |doi-access=free }}

|0.0944{{±|0.0053}}

|0.331{{±|0.018}}

|29.04992{{±|0.00021}}

|0.229{{±|0.004}}

|1133{{±|30}}

| style="background:#FFFF00" |transit

|873{{±|3}}

|1.89{{±|0.11}}

|8500{{±|150}}

|Host star also known as TOI-1228{{citation|arxiv=2208.06396|year=2022|title=HD 56414 b: A Warm Neptune Transiting an A-type Star|doi=10.3847/2041-8213/ac80f4 |last1=Giacalone |first1=Steven |last2=Dressing |first2=Courtney D. |last3=Muñoz |first3=A. García |last4=Hooton |first4=Matthew J. |last5=Stassun |first5=Keivan G. |last6=Quinn |first6=Samuel N. |last7=Zhou |first7=George |last8=Ziegler |first8=Carl |last9=Vanderspek |first9=Roland |last10=Latham |first10=David W. |last11=Seager |first11=S. |last12=Winn |first12=Joshua N. |last13=Jenkins |first13=Jon M. |last14=Briceño |first14=César |last15=Huang |first15=Chelsea X. |last16=Rodriguez |first16=David R. |last17=Shporer |first17=Avi |last18=Mann |first18=Andrew W. |last19=Watanabe |first19=David |last20=Wohler |first20=Bill |journal=The Astrophysical Journal Letters |volume=935 |issue=1 |pages=L10 |bibcode=2022ApJ...935L..10G |s2cid=251538927 |doi-access=free }}

|2.56{{±|0.19}}

|

|623.0{{±|3.4}}

|1.510{{±|0.006}}

|

|style="background:#00FF00"|radial vel.

|424.1{{±|1.7}}

|1.18{{±|0.05}}

|5066{{±|58|60}}

|Giant host star

|3.04{{±|0.16}}

|

|1193.3{{±|7.0}}

|2.482{{±|0.010}}

|

|style="background:#00FF00"|radial vel.

|245.0{{±|1.3}}

|1.43{{±|0.07}}

|4787{{±|280|51}}

|Giant host star

|1.5{{±|0.5|0.2}}

|

|8241{{±|1019|530}}

|8.0{{±|0.8}}

|

|style="background:#00FF00"|radial vel.

|133.6{{±|0.2}}

|1.00{{±|0.03}}

|5442{{±|17}}

|Eccentric orbit due to hot Jupiter in system{{citation|arxiv=2204.05711|year=2022|title=HD 83443c: A Highly Eccentric Giant Planet on a 22 yr Orbit|doi=10.3847/1538-3881/ac6589 |last1=Errico |first1=Adriana |last2=Wittenmyer |first2=Robert A. |last3=Horner |first3=Jonathan |last4=Li |first4=Zhexing |last5=Brandt |first5=G. Mirek |last6=Kane |first6=Stephen R. |last7=Fetherolf |first7=Tara |last8=Holt |first8=Timothy R. |last9=Carter |first9=Brad |last10=Clark |first10=Jake T. |last11=Butler |first11=R. P. |last12=Tinney |first12=C. G. |last13=Ballard |first13=Sarah |last14=Bowler |first14=Brendan P. |last15=Kielkopf |first15=John |last16=Liu |first16=Huigen |last17=Plavchan |first17=Peter P. |last18=Shporer |first18=Avi |last19=Zhang |first19=Hui |last20=Wright |first20=Duncan J. |last21=Addison |first21=Brett C. |last22=Mengel |first22=Matthew W. |last23=Okumura |first23=Jack |journal=The Astronomical Journal |volume=163 |issue=6 |page=273 |bibcode=2022AJ....163..273E |s2cid=248118529 |doi-access=free }}

|

|0.121{{±|0.004}}

|1.0391353{{±|0.0000049|0.0000045}}

|0.02085{{±|0.00037}}

|2042{{±|27}}

| style="background:#FFFF00" |transit

|268.6{{±|1.3}}

|1.109{{±|0.043}}

|5987{{±|64}}

|Host star also known as TOI-1797{{citation|arxiv=2207.13920|year=2022|title=The HD 93963 a transiting system: A 1.04 d super-Earth and a 3.65 d sub-Neptune discovered by TESS and CHEOPS|last1=Serrano |first1=L. M. |last2=Gandolfi |first2=D. |last3=Hoyer |first3=S. |last4=Brandeker |first4=A. |last5=Hooton |first5=M. J. |last6=Sousa |first6=S. |last7=Murgas |first7=F. |last8=Ciardi |first8=D. R. |last9=Howell |first9=S. B. |last10=Benz |first10=W. |last11=Billot |first11=N. |last12=Florén |first12=H. -G. |last13=Bekkelien |first13=A. |last14=Bonfanti |first14=A. |last15=Krenn |first15=A. |last16=Mustill |first16=A. J. |last17=Wilson |first17=T. G. |last18=Osborn |first18=H. |last19=Parviainen |first19=H. |last20=Heidari |first20=N. |last21=Pallé |first21=E. |last22=Fridlund |first22=M. |last23=Adibekyan |first23=V. |last24=Fossati |first24=L. |last25=Deleuil |first25=M. |last26=Knudstrup |first26=E. |last27=Collins |first27=K. A. |last28=Lam |first28=K. W. F. |last29=Grziwa |first29=S. |last30=Salmon |first30=S. |journal=Astronomy & Astrophysics |volume=667 |pages=A1 |doi=10.1051/0004-6361/202243093 |bibcode=2022A&A...667A...1S |s2cid=250709574 |display-authors=1 }}

|

|0.288{{±|0.005}}

|3.6451398{{±|0.0000106|0.0000142}}

|0.04813{{±|0.00085}}

|1344{{±|18}}

| style="background:#FFFF00" |transit

|268.6{{±|1.3}}

|1.109{{±|0.043}}

|5987{{±|64}}

|Host star also known as TOI-1797

|

|0.258{{±|0.014|0.012}}

|9.188526{{±|0.000026}}

|

|

| style="background:#FFFF00" |transit

|259.5{{±|0.2}}

|1.08{{±|0.05}}

|5881{{±|50}}

|Young host star also known as TOI-1097{{citation|arxiv=2012.03266|year=2022|title=The upper bound of the second Higgs boson mass in minimal gauge mediation with the gravitino warm dark matter|doi=10.1007/JHEP04(2021)024 |last1=Choi |first1=Gong jun |last2=Yanagida |first2=Tsutomu T. |last3=Yokozaki |first3=Norimi |journal=Journal of High Energy Physics |volume=2021 |issue=4 |s2cid=227340010 }}

|

|0.231{{±|0.018|0.016}}

|13.900148{{±|0.000057}}

|

|

| style="background:#FFFF00" |transit

|259.5{{±|0.2}}

|1.08{{±|0.05}}

|5881{{±|50}}

|Young host star also known as TOI-1097

|8.0{{±|1.0}}

|1.00{{±|0.03}}

|109.75{{±|0.40|0.37}}

|0.5109{{±|0.0081|0.0083}}

|

| style="background:#FFFF00" |transit

|310.1{{±|0.7}}

|1.47{{±|0.07}}

|6651{{±|35}}

|Young star, eccentric planetary orbit{{citation|arxiv=2211.08294|year=2022|title=Radial velocity survey for planets around young stars (RVSPY)|last1=Zakhozhay |first1=O. |last2=Launhardt |first2=R. |last3=Trifonov |first3=T. |last4=Kürster |first4=M. |last5=Reffert |first5=S. |last6=Henning |first6=Th. |last7=Brahm |first7=R. |last8=Vinés |first8=J. |last9=Marleau |first9=G. -D. |last10=Patel |first10=J. |journal=Astronomy & Astrophysics |volume=667 |pages=L14 |doi=10.1051/0004-6361/202244747 |s2cid=235028524 }}{{citation|arxiv=2211.11767|year=2023|title=The high-albedo, low polarization disk around HD 114082 that harbors a Jupiter-sized transiting planet|last1=Engler |first1=N. |last2=Milli |first2=J. |last3=Gratton |first3=R. |last4=Ulmer-Moll |first4=S. |last5=Vigan |first5=A. |last6=Lagrange |first6=A. -M. |last7=Kiefer |first7=F. |last8=Rubini |first8=P. |last9=Grandjean |first9=A. |last10=Schmid |first10=H. M. |last11=Messina |first11=S. |last12=Squicciarini |first12=V. |last13=Olofsson |first13=J. |last14=Thébault |first14=P. |last15=van Holstein |first15=R. |last16=Janson |first16=M. |last17=Ménard |first17=F. |last18=Marshall |first18=J. P. |last19=Chauvin |first19=G. |last20=Bhowmik |first20=T. |last21=Boccaletti |first21=A. |last22=Bonnefoy |first22=M. |last23=del Burgo |first23=C. |last24=Choquet |first24=E. |last25=Desidera |first25=S. |last26=Feldt |first26=M. |last27=Fusco |first27=T. |last28=Girard |first28=J. |last29=Gisler |first29=D. |last30=Hagelberg |first30=J. |journal=Astronomy & Astrophysics |volume=672 |pages=A1 |doi=10.1051/0004-6361/202244380 |s2cid=256215468 |display-authors=1 }}

|0.85{{±|0.12|0.11}}

|

|20.6532{{±|0.0032|0.0032}}

|0.1512{{±|0.0058|0.0063}}

|1874

| style="background:#00FF00" |radial vel.

|353.5

|1.08{{±|0.14|0.12}}

|4830

|Host red giant star also known as HR 6840, other planets in system are suspected{{citation|arxiv=2211.06576|year=2022|title=A close-in planet orbiting giant star HD 167768|last1=Teng |first1=Huan-Yu |last2=Sato |first2=Bun'ei |last3=Kunitomo |first3=Masanobu |last4=Takarada |first4=Takuya |last5=Omiya |first5=Masashi |last6=Harakawa |first6=Hiroki |last7=Xiao |first7=Guang-Yao |last8=Liu |first8=Yu-Juan |last9=Izumiura |first9=Hideyuki |last10=Kambe |first10=Eiji |last11=Yoshida |first11=Michitoshi |last12=Itoh |first12=Yoichi |last13=Ando |first13=Hiroyasu |last14=Kokubo |first14=Eiichiro |last15=Shigeru |first15=Ida |journal=Publications of the Astronomical Society of Japan |volume=75 |pages=169–176 |doi=10.1093/pasj/psac097 }}

|0.0425{{±|0.0063}}

|

|284{{±|10|8}}

|0.812{{±|0.028}}

|278{{±|6}}

| style="background:#00FF00" |radial vel.

|174.4{{±|0.1}}

|0.81{{±|0.04}}

|5348{{±|100}}

|Habitable zone planet{{cite journal |arxiv=2211.00667|last1=Orell-Miquel |first1=J. |last2=Nowak |first2=G. |last3=Murgas |first3=F. |last4=Palle |first4=E. |last5=Morello |first5=G. |last6=Luque |first6=R. |last7=Badenas-Agusti |first7=M. |last8=Ribas |first8=I. |last9=Lafarga |first9=M. |last10=Espinoza |first10=N. |last11=Morales |first11=J. C. |last12=Zechmeister |first12=M. |last13=Alqasim |first13=A. |last14=Cochran |first14=W. D. |last15=Gandolfi |first15=D. |last16=Goffo |first16=E. |last17=Kabáth |first17=P. |last18=Korth |first18=J. |last19=Livingston |first19=J. |last20=Lam |first20=K. W. F. |last21=Muresan |first21=A. |last22=Persson |first22=C. M. |last23=Van Eylen |first23=V. |title=HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone |journal=Astronomy & Astrophysics |year=2023 |volume=669 |pages=A40 |doi=10.1051/0004-6361/202244120 |bibcode=2023A&A...669A..40O |s2cid=253197272 }}

|>2.1

|

|>2200

|>3.2

|<125

|

|174.4{{±|0.1}}

|0.81{{±|0.04}}

|5348{{±|100}}

|

|10.070{{±|2.483}}

|

|21000{{±|8000}}

|13.048{{±|3.073}}

|

| style="background:#00FF00" |radial vel.

|66.7{{±|2.4}}

|

|

|Host star also known as GJ 9714

|0.079{{±|0.008}}

|

|9.9

|0.091{{±|0.004}}

|

| style="background:#00FF00" |radial vel.

|227.8{{±|0.4}}

|

|

|Also brown dwarf in the system

|12.3{{±|1.1|1.2}}

|1.46{{±|0.18|0.06}}

|2082

|3.53{{±|0.08|0.07}}

|1181.9{{±|20.6|53.9}}

| style="background:#00FF00" |radial vel.

|125.1{{±|2.6}}

|1.24

|6486

|Some deuterium burning despite its low mass, also another brown dwarf is present in the system{{citation|arxiv=2208.04867|year=2023|title=Direct discovery of the inner exoplanet in the HD 206893 system|last1=Hinkley |first1=S. |last2=Lacour |first2=S. |last3=Marleau |first3=G. D. |last4=Lagrange |first4=A. M. |last5=Wang |first5=J. J. |last6=Kammerer |first6=J. |last7=Cumming |first7=A. |last8=Nowak |first8=M. |last9=Rodet |first9=L. |last10=Stolker |first10=T. |last11=Balmer |first11=W. -O. |last12=Ray |first12=S. |last13=Bonnefoy |first13=M. |last14=Mollière |first14=P. |last15=Lazzoni |first15=C. |last16=Kennedy |first16=G. |last17=Mordasini |first17=C. |last18=Abuter |first18=R. |last19=Aigrain |first19=S. |last20=Amorim |first20=A. |last21=Asensio-Torres |first21=R. |last22=Babusiaux |first22=C. |last23=Benisty |first23=M. |last24=Berger |first24=J. -P. |last25=Beust |first25=H. |last26=Blunt |first26=S. |last27=Boccaletti |first27=A. |last28=Bohn |first28=A. |last29=Bonnet |first29=H. |last30=Bourdarot |first30=G. |journal=Astronomy & Astrophysics |volume=671 |pages=L5 |doi=10.1051/0004-6361/202244727 |bibcode=2023A&A...671L...5H |s2cid=251442869 |display-authors=1 }}

|0.014{{±|0.002}}

|

|2.56

|0.034{{±|0.002}}

|

| style="background:#00FF00" |radial vel.

|120

|

|

|Host star also known as GJ 2030{{citation|arxiv=2208.12720|year=2022|title=3D Selection of 167 Substellar Companions to Nearby Stars|doi=10.3847/1538-4365/ac7e57 |last1=Feng |first1=Fabo |last2=Butler |first2=R. Paul |last3=Vogt |first3=Steven S. |last4=Clement |first4=Matthew S. |last5=Tinney |first5=C. G. |last6=Cui |first6=Kaiming |last7=Aizawa |first7=Masataka |last8=Jones |first8=Hugh R. A. |last9=Bailey |first9=J. |last10=Burt |first10=Jennifer |last11=Carter |first11=B. D. |last12=Crane |first12=Jeffrey D. |last13=Dotti |first13=Francesco Flammini |last14=Holden |first14=Bradford |last15=Ma |first15=Bo |last16=Ogihara |first16=Masahiro |last17=Oppenheimer |first17=Rebecca |last18=o'Toole |first18=S. J. |last19=Shectman |first19=Stephen A. |last20=Wittenmyer |first20=Robert A. |last21=Wang |first21=Sharon X. |last22=Wright |first22=D. J. |last23=Xuan |first23=Yifan |journal=The Astrophysical Journal Supplement Series |volume=262 |issue=1 |page=21 |bibcode=2022ApJS..262...21F |s2cid=251864022 |doi-access=free }}

|12.934{{±|2.361}}

|

|25600{{±|2500}}

|16.752{{±|1.312}}

|

| style="background:#00FF00" |radial vel.

|120

|

|

|Host star also known as GJ 2030

|0.038{{±|0.010}}

|

|10.6

|0.091{{±|0.004}}

|

| style="background:#00FF00" |radial vel.

|57.7

|

|

|Host star also known as GJ 3222, planet on extremely eccentric orbit, also brown dwarf in the system

|0.0067{{±|0.0011}}

|0.111{{±|0.002}}

|2.76953{{±|0.00003}}

|0.02933{{±|0.00024}}

|709{{±|4}}

| style="background:#FFFF00" |transit

|32.63{{±|0.07}}

|0.439{{±|0.011}}

|3803{{±|10}}

|Host star also known as TOI-4599{{citation|arxiv=2204.10261|year=2022|title=The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc|last1=Luque |first1=R. |last2=Fulton |first2=B. J. |last3=Kunimoto |first3=M. |last4=Amado |first4=P. J. |last5=Gorrini |first5=P. |last6=Dreizler |first6=S. |last7=Hellier |first7=C. |last8=Henry |first8=G. W. |last9=Molaverdikhani |first9=K. |last10=Morello |first10=G. |last11=Peña-Moñino |first11=L. |last12=Pérez-Torres |first12=M. |last13=Pozuelos |first13=F. J. |last14=Shan |first14=Y. |last15=Anglada-Escudé |first15=G. |last16=Béjar |first16=V. J. S. |last17=Bergond |first17=G. |last18=Boyle |first18=A. W. |last19=Caballero |first19=J. A. |last20=Charbonneau |first20=D. |last21=Ciardi |first21=D. R. |last22=Dufoer |first22=S. |last23=Espinoza |first23=N. |last24=Everett |first24=M. |last25=Fischer |first25=D. |last26=Hatzes |first26=A. P. |last27=Henning |first27=Th. |last28=Hesse |first28=K. |last29=Howard |first29=A. |last30=Howell |first30=S. B. |journal=Astronomy & Astrophysics |volume=664 |pages=A199 |doi=10.1051/0004-6361/202243834 |bibcode=2022A&A...664A.199L |s2cid=248300168 |display-authors=1 }}

|0.0097{{±|0.0015}}

|0.137{{±|0.004}}

|5.70588{{±|0.00007}}

|0.04749{{±|0.00039}}

|557{{±|3}}

| style="background:#FFFF00" |transit

|32.63{{±|0.07}}

|0.439{{±|0.011}}

|3803{{±|10}}

|Host star also known as TOI-4599

|0.0052{{±|0.0007}}

|0.103{{±|0.005}}

|0.548177{{±|0.000019}}

|0.01188{{±|0.00040}}

|1617{{±|41}}

| style="background:#FFFF00" |transit

|154.81{{±|0.15}}

|0.740{{±|0.017}}

|4440{{±|100}}

|Host star also known as TOI-500{{citation|arxiv=2204.13573|year=2022|title=A low-eccentricity migration pathway for a 13-h-period Earth analogue in a four-planet system|doi=10.1038/s41550-022-01641-y |last1=Serrano |first1=Luisa Maria |last2=Gandolfi |first2=Davide |last3=Mustill |first3=Alexander J. |last4=Barragán |first4=Oscar |last5=Korth |first5=Judith |last6=Dai |first6=Fei |last7=Redfield |first7=Seth |last8=Fridlund |first8=Malcolm |last9=Lam |first9=Kristine W. F. |last10=Díaz |first10=Matías R. |last11=Grziwa |first11=Sascha |last12=Collins |first12=Karen A. |last13=Livingston |first13=John H. |last14=Cochran |first14=William D. |last15=Hellier |first15=Coel |last16=Bellomo |first16=Salvatore E. |last17=Trifonov |first17=Trifon |last18=Rodler |first18=Florian |last19=Alarcon |first19=Javier |last20=Jenkins |first20=Jon M. |last21=Latham |first21=David W. |last22=Ricker |first22=George |last23=Seager |first23=Sara |last24=Vanderspeck |first24=Roland |last25=Winn |first25=Joshua N. |last26=Albrecht |first26=Simon |last27=Collins |first27=Kevin I. |last28=Csizmadia |first28=Szilárd |last29=Daylan |first29=Tansu |last30=Deeg |first30=Hans J. |journal=Nature Astronomy |volume=6 |issue=6 |pages=736–750 |bibcode=2022NatAs...6..736S |s2cid=248426734 |display-authors=1 }}

|0.0146{{±|0.0016}}

|

|6.6356{{±|0.0040}}

|

|

| style="background:#00FF00" |radial vel.

|154.81{{±|0.15}}

|0.740{{±|0.017}}

|4440{{±|100}}

|Host star also known as TOI-500

|0.1055{{±|0.0033}}

|

|26.233{{±|0.020}}

|

|

| style="background:#00FF00" |radial vel.

|154.81{{±|0.15}}

|0.740{{±|0.017}}

|4440{{±|100}}

|Host star also known as TOI-500

|0.0376{{±|0.0042}}

|

|61.30{{±|0.28}}

|

|

| style="background:#00FF00" |radial vel.

|154.81{{±|0.15}}

|0.740{{±|0.017}}

|4440{{±|100}}

|Host star also known as TOI-500

|

|0.268{{±|0.027}}

|7.713057{{±|0.000021}}

|0.07870{{±|0.00056|0.00017}}

|1060{{±|50}}

| style="background:#FFFF00" |transit

|191.2{{±|0.4}}

|1.094{{±|0.024|0.007}}

|5991{{±|50}}

|Host star also known as TOI-4399, shares system with a red dwarf{{citation|arxiv=2204.11975|year=2022|title=A Mini-Neptune from TESS and CHEOPS Around the 120 Myr Old AB Dor Member HIP 94235|last1=Zhou |first1=George |last2=Wirth |first2=Christopher P. |last3=Huang |first3=Chelsea X. |last4=Venner |first4=Alexander |last5=Franson |first5=Kyle |last6=Quinn |first6=Samuel N. |last7=Bouma |first7=L. G. |last8=Kraus |first8=Adam L. |last9=Mann |first9=Andrew W. |last10=Newton |first10=Elisabeth. R. |last11=Dragomir |first11=Diana |last12=Heitzmann |first12=Alexis |last13=Lowson |first13=Nataliea |last14=Douglas |first14=Stephanie T. |last15=Battley |first15=Matthew |last16=Gillen |first16=Edward |last17=Triaud |first17=Amaury |last18=Latham |first18=David W. |last19=Howell |first19=Steve B. |last20=Hartman |first20=J. D. |last21=Tofflemire |first21=Benjamin M. |last22=Wittenmyer |first22=Robert A. |last23=Bowler |first23=Brendan P. |last24=Horner |first24=Jonathan |last25=Kane |first25=Stephen R. |last26=Kielkopf |first26=John |last27=Plavchan |first27=Peter |last28=Wright |first28=Duncan J. |last29=Addison |first29=Brett C. |last30=Mengel |first30=Matthew W. |journal=The Astronomical Journal |volume=163 |issue=6 |page=289 |doi=10.3847/1538-3881/ac69e3 |bibcode=2022AJ....163..289Z |s2cid=248392044 |display-authors=1 |doi-access=free }}

|0.30{{±|0.07}}

|

|285.1{{±|1.2|1.5}}

|0.937{{±|0.003}}

|

| style="background:#00FF00" |radial vel.

|200.2

|1.35{{±|0.19|0.21}}

|4971

|Red giant host star also known as HD 184010{{citation|arxiv=2209.09426|year=2022|title=A trio of giant planets orbiting evolved star HD 184010|doi=10.1093/pasj/psac070 |last1=Teng |first1=Huan-Yu |last2=Sato |first2=Bun'ei |last3=Takarada |first3=Takuya |last4=Omiya |first4=Masashi |last5=Harakawa |first5=Hiroki |last6=Nagasawa |first6=Makiko |last7=Hasegawa |first7=Ryo |last8=Izumiura |first8=Hideyuki |last9=Kambe |first9=Eiji |last10=Yoshida |first10=Michitoshi |last11=Itoh |first11=Yoichi |last12=Ando |first12=Hiroyasu |last13=Kokubo |first13=Eiichiro |last14=Ida |first14=Shigeru |journal=Publications of the Astronomical Society of Japan |volume=74 |issue=6 |pages=1309–1328 }}

|0.28{{±|0.08|0.10}}

|

|483.3{{±|3.2|4.0}}

|1.332{{±|0.006|0.007}}

|

| style="background:#00FF00" |radial vel.

|200.2

|1.35{{±|0.19|0.21}}

|4971

|Red giant host star also known as HD 184010

|0.46{{±|0.08}}

|

|837.7{{±|6.4|5.5}}

|1.922{{±|0.010|0.008}}

|

| style="background:#00FF00" |radial vel.

|200.2

|1.35{{±|0.19|0.21}}

|4971

|Red giant host star also known as HD 184010

|0.0272{{±|0.0172}}

|0.259{{±|0.017|0.015}}

|23.448172{{±|0.00076|0.00099}}

|

|710

| style="background:#FFFF00" |transit

|

|0.823{{±|0.369|0.25}}

|5561{{±|138 }}

|{{citation|arxiv=2203.02087|year=2022|title=Scaling K2. V. Statistical Validation of 60 New Exoplanets from K2 Campaigns 2–18|doi=10.3847/1538-3881/ac5c4c |last1=Christiansen |first1=Jessie L. |last2=Bhure |first2=Sakhee |last3=Zink |first3=Jon K. |last4=Hardegree-Ullman |first4=Kevin K. |last5=Adkins |first5=Britt Duffy |last6=Hedges |first6=Christina |last7=Morton |first7=Timothy D. |last8=Bieryla |first8=Allyson |last9=Ciardi |first9=David R. |last10=Cochran |first10=William D. |last11=Dressing |first11=Courtney D. |last12=Everett |first12=Mark E. |last13=Isaacson |first13=Howard |last14=Livingston |first14=John H. |last15=Ziegler |first15=Carl |last16=Berlind |first16=Perry |last17=Calkins |first17=Michael L. |last18=Esquerdo |first18=Gilbert A. |last19=Latham |first19=David W. |last20=Endl |first20=Michael |last21=MacQueen |first21=Phillip J. |last22=Fulton |first22=Benjamin J. |last23=Hirsch |first23=Lea A. |last24=Howard |first24=Andrew W. |last25=Weiss |first25=Lauren M. |last26=Allen |first26=Bridgette E. |last27=Berberyann |first27=Arthur |last28=Ciardi |first28=Krys N. |last29=Dunlavy |first29=Ava |last30=Glassford |first30=Sofia H. |journal=The Astronomical Journal |volume=163 |issue=6 |page=244 |bibcode=2022AJ....163..244C |s2cid=247244871 |display-authors=1 |doi-access=free }}

|0.0199{{±|0.0115}}

|0.210{{±|0.016|0.014}}

|15.93703{{±|0.00079|0.00114}}

|

|770

| style="background:#FFFF00" |transit

|

|0.825{{±|0.366|0.255}}

|5601{{±|138}}

|

|0.0203{{±|0.0126}}

|0.215{{±|0.020|0.017}}

|20.64509{{±|0.00099|0.00137}}

|

|450

| style="background:#FFFF00" |transit

|

|0.756{{±|0.231|0.347}}

|4348{{±|128}}

|

|0.0073{{±|0.0042}}

|0.118{{±|0.009|0.008}}

|5.02559{{±|0.00028|0.00034}}

|

|800

| style="background:#FFFF00" |transit

|

|0.746{{±|0.334|0.232}}

|4663{{±|138}}

|

|0.0078{{±|0.0041}}

|0.121{{±|0.010|0.009}}

|9.66018{{±|0.00116}}

|

|650

| style="background:#FFFF00" |transit

|

|0.746{{±|0.334|0.232}}

|4663{{±|138}}

|

|0.0146{{±|0.0085}}

|0.173{{±|0.013|0.012}}

|20.20108{{±|0.00235|0.00273}}

|

|500

| style="background:#FFFF00" |transit

|

|0.746{{±|0.334|0.232}}

|4663{{±|138}}

|

|0.0069{{±|0.0040}}

|0.117{{±|0.009|0.008}}

|5.76161{{±|0.00084|0.00071}}

|

|1080

| style="background:#FFFF00" |transit

|

|0.735{{±|0.334|0.224}}

|5682{{±|138}}

|

|0.0327{{±|0.0207}}

|0.286{{±|0.020|0.048}}

|2.14084{{±|0.00003|0.00004}}

|

|1420

| style="background:#FFFF00" |transit

|

|0.984{{±|0.428|0.303}}

|5377{{±|138}}

|

|4.7{{±|2.2}}

|1.162{{±|0.082|0.077}}

|3.11490{{±|0.00001}}

|

|1000

| style="background:#FFFF00" |transit

|

|0.958{{±|0.44|0.298}}

|4925{{±|138}}

|

|0.0289{{±|0.0168}}

|0.262{{±|0.006}}

|9.84407{{±|0.00056|0.00057}}

|

|870

| style="background:#FFFF00" |transit

|

|0.847{{±|0.101|0.088}}

|5479{{±|27}}

|

|0.0162{{±|0.0089}}

|0.184{{±|0.013|0.012}}

|11.02066{{±|0.00143|0.00136}}

|

|1130

| style="background:#FFFF00" |transit

|

|1.158{{±|0.499|0.349}}

|6138{{±|138}}

|

|0.0113{{±|0.0058}}

|0.142{{±|0.005}}

|4.52195{{±|0.00032|0.00040}}

|

|1210

| style="background:#FFFF00" |transit

|

|0.731{{±|0.067|0.061}}

|5789{{±|21}}

|

|0.0179{{±|0.0109}}

|0.197{{±|0.008|0.007}}

|16.43445{{±|0.00237|0.00270}}

|

|790

| style="background:#FFFF00" |transit

|

|0.731{{±|0.067|0.061}}

|5789{{±|21}}

|

|0.0183{{±|0.0106}}

|0.200{{±|0.016|0.015}}

|14.45389{{±|0.00477|0.00417}}

|

|1000

| style="background:#FFFF00" |transit

|

|1.119{{±|0.492|0.344}}

|5822{{±|138}}

|

|0.0129{{±|0.0074}}

|0.155{{±|0.011|0.010}}

|5.77647{{±|0.00026|0.00023}}

|

|1240

| style="background:#FFFF00" |transit

|

|0.908{{±|0.394|0.281}}

|5937{{±|138}}

|

|0.0123{{±|0.0073}}

|0.151{{±|0.013|0.011}}

|12.83223{{±|0.00155|0.00161}}

|

|530

| style="background:#FFFF00" |transit

|

|0.821{{±|0.371|0.258}}

|4200{{±|138}}

|

|0.0283{{±|0.0173}}

|0.257{{±|0.024|0.020}}

|2.06043{{±|0.00011|0.00007}}

|

|1130

| style="background:#FFFF00" |transit

|

|0.923{{±|0.425|0.291}}

|4823{{±|138}}

|

|0.0175{{±|0.0104}}

|0.194{{±|0.032|0.017}}

|8.77724{{±|0.00062|0.00061}}

|

|680

| style="background:#FFFF00" |transit

|

|0.856{{±|0.375|0.265}}

|4603{{±|138}}

|

|0.0250{{±|0.0144}}

|0.243{{±|0.016|0.015}}

|9.40131{{±|0.00046|0.00050}}

|

|1110

| style="background:#FFFF00" |transit

|

|0.993{{±|0.416|0.302}}

|5911{{±|138}}

|

|0.0040{{±|0.0026}}

|0.095{{±|0.012|0.009}}

|7.93893{{±|0.00059}}

|

|670

| style="background:#FFFF00" |transit

|

|0.754{{±|0.337|0.239}}

|4473{{±|138}}

|

|0.0158{{±|0.0094}}

|0.178{{±|0.016|0.013}}

|16.03465{{±|0.00184|0.00157}}

|

|530

| style="background:#FFFF00" |transit

|

|0.754{{±|0.337|0.239}}

|4473{{±|138}}

|

|0.0121{{±|0.0070}}

|0.150{{±|0.016|0.012}}

|26.80302{{±|0.00277|0.00304}}

|

|440

| style="background:#FFFF00" |transit

|

|0.754{{±|0.337|0.239}}

|4473{{±|138}}

|

|0.0162{{±|0.0101}}

|0.185{{±|0.013|0.011}}

|21.70015{{±|0.00202|0.00191}}

|

|610

| style="background:#FFFF00" |transit

|

|0.922{{±|0.401|0.284}}

|5452{{±|138}}

|

|0.0102{{±|0.0052}}

|0.139{{±|0.010|0.009}}

|1.86596{{±|0.00001}}

|

|1270

| style="background:#FFFF00" |transit

|

|1.061{{±|0.459|0.327}}

|5129{{±|138}}

|

|0.0040{{±|0.0026}}

|0.096{{±|0.020|0.005}}

|2.23152{{±|0.0019|0.00032}}

|

|600

| style="background:#FFFF00" |transit

|

|0.330{{±|0.009}}

|3623{{±|138}}

|

|0.0054{{±|0.0027}}

|0.106{{±|0.004|0.006}}

|4.19476{{±|0.00030|0.00018}}

|

|480

| style="background:#FFFF00" |transit

|

|0.330{{±|0.009}}

|3623{{±|138}}

|

|0.0085{{±|0.0044}}

|0.124{{±|0.010|0.006}}

|6.67958{{±|0.00071|0.00049}}

|

|410

| style="background:#FFFF00" |transit

|

|0.330{{±|0.009}}

|3623{{±|138}}

|

|0.0075{{±|0.0042}}

|0.120{{±|0.012|0.007}}

|9.71504{{±|0.00100|0.00073}}

|

|370

| style="background:#FFFF00" |transit

|

|0.330{{±|0.009}}

|3623{{±|138}}

|

|0.0179{{±|0.0104}}

|0.198{{±|0.008|0.007}}

|13.62749{{±|0.00034|0.00057}}

|

|330

| style="background:#FFFF00" |transit

|

|0.330{{±|0.009}}

|3623{{±|138}}

|

|0.0100{{±|0.0056}}

|0.137{{±|0.012|0.011}}

|2.38086{{±|0.00016|0.00021}}

|

|1100

| style="background:#FFFF00" |transit

|1370{{±|20}}

|0.9270{{±|0.4120|0.2860}}

|4844{{±|138}}

|

|0.0195{{±|0.0115}}

|0.207{{±|0.006|0.005}}

|7.47322{{±|0.00037|0.00031}}

|

|1010

| style="background:#FFFF00" |transit

|1400{{±|30}}

|0.911{{±|0.088|0.083}}

|5749{{±|22}}

|

|0.1430{{±|0.0996}}

|0.653{{±|0.023}}

|28.73532{{±|0.00099}}

|

|340

| style="background:#FFFF00" |transit

|870{{±|12}}

|0.570{{±|0.051|0.048}}

|3572{{±|138}}

|

|0.0412{{±|0.0263}}

|0.326{{±|0.029|0.020}}

|6.33906{{±|0.00022|0.00018}}

|

|970

| style="background:#FFFF00" |transit

|948{{±|13}}

|0.8420{{±|0.3760|0.2590}}

|5367{{±|138}}

|

|0.0177{{±|0.0103}}

|0.195{{±|0.010}}

|8.58404{{±|0.00088|0.00202}}

|

|1050

| style="background:#FFFF00" |transit

|846{{±|9}}

|0.8020{{±|0.3570|0.2460}}

|5782{{±|138}}

|

|0.0165{{±|0.0085}}

|0.182{{±|0.013|0.012}}

|20.85133{{±|0.00280|0.00298}}

|

|780

| style="background:#FFFF00" |transit

|846{{±|9}}

|0.8020{{±|0.3570|0.2460}}

|5782{{±|138}}

|

|0.0636{{±|0.0390}}

|0.416{{±|0.027|0.030}}

|3.31279{{±|0.00010}}

|

|1310

| style="background:#FFFF00" |transit

|1490{{±|18}}

|0.7890{{±|0.3510|0.2390}}

|5558{{±|138}}

|

|0.0078{{±|0.0053}}

|0.122{{±|0.025|0.016}}

|4.62265{{±|0.00022|0.00025}}

|

|900

| style="background:#FFFF00" |transit

|1660{{±|50}}

|0.7570{{±|0.3410|0.2400}}

|5543{{±|138}}

|

|0.0140{{±|0.0079}}

|0.165{{±|0.014|0.013}}

|15.39872{{±|0.00242|0.00193}}

|

|840

| style="background:#FFFF00" |transit

|1330{{±|30}}

|0.8410{{±|0.3700|0.2580}}

|5726{{±|138}}

|

|0.0199{{±|0.0127}}

|0.210{{±|0.015|0.014}}

|10.41318{{±|0.00093|0.00069}}

|

|950

| style="background:#FFFF00" |transit

|867{{±|9}}

|0.8810{{±|0.3810|0.2690}}

|5678{{±|138}}

|

|0.0123{{±|0.0063}}

|0.151{{±|0.012|0.011}}

|5.09571{{±|0.00011}}

|

|890

| style="background:#FFFF00" |transit

|319.7{{±|1.5}}

|0.478{{±|0.214|0.147}}

|4938{{±|138}}

|

|0.0240{{±|0.0141}}

|0.231{{±|0.017|0.015}}

|4.80335{{±|0.00035|0.00046}}

|

|910

| style="background:#FFFF00" |transit

|935{{±|10}}

|0.9520{{±|0.4210|0.2930}}

|5007{{±|138}}

|

|0.0371{{±|0.0220}}

|0.303{{±|0.025|0.022}}

|8.49128{{±|0.00033|0.00030}}

|

|750

| style="background:#FFFF00" |transit

|935{{±|10}}

|0.9520{{±|0.4210|0.2930}}

|5007{{±|138}}

|

|0.0106{{±|0.0061}}

|0.140{{±|0.010|0.009}}

|0.6736{{±|0.00001}}

|

|1990

| style="background:#FFFF00" |transit

|897{{±|9}}

|0.9540{{±|0.4290|0.2930}}

|5236{{±|138}}

|

|0.0314{{±|0.0189}}

|0.278{{±|0.015|0.010}}

|25.76051{{±|0.00199|0.00188}}

|

|590

| style="background:#FFFF00" |transit

|897{{±|9}}

|0.9540{{±|0.4290|0.2930}}

|5236{{±|138}}

|

|0.0212{{±|0.0127}}

|0.216{{±|0.016}}

|3.57232{{±|0.00018|0.00015}}

|

|1210

| style="background:#FFFF00" |transit

|650{{±|5}}

|0.9370{{±|0.4060|0.2850}}

|5387{{±|138}}

|

|0.0191{{±|0.0112}}

|0.203{{±|0.010|0.009}}

|6.39302{{±|0.00113|0.00075}}

|

|1240

| style="background:#FFFF00" |transit

|1980{{±|40}}

|0.9450{{±|0.0900|0.0830}}

|5946{{±|20}}

|

|0.0736{{±|0.0412}}

|0.455{{±|0.013}}

|18.78783{{±|0.00087|0.00099}}

|

|870

| style="background:#FFFF00" |transit

|1980{{±|40}}

|0.9450{{±|0.0900|0.0830}}

|5946{{±|20}}

|

|0.0051{{±|0.0025}}

|0.103{{±|0.004}}

|3.86505{{±|0.00018}}

|

|570

| style="background:#FFFF00" |transit

|203.5{{±|0.8}}

|0.374{{±|0.009}}

|3578{{±|138}}

|

|0.0183{{±|0.0117}}

|0.201{{±|0.018|0.017}}

|6.29309{{±|0.00057|0.00070}}

|

|660

| style="background:#FFFF00" |transit

|655{{±|5}}

|0.8700{{±|0.3950|0.2690}}

|4213{{±|138}}

|

|0.0245{{±|0.0149}}

|0.239{{±|0.019|0.017}}

|17.27474{{±|0.00259|0.00317}}

|

|870

| style="background:#FFFF00" |transit

|1710{{±|60}}

|0.9440{{±|0.4190|0.2900}}

|5716{{±|138}}

|

|0.0783{{±|0.0515}}

|0.476{{±|0.031|0.034}}

|33.58977{{±|0.00076}}

|

|580

| style="background:#FFFF00" |transit

|804{{±|8}}

|0.7840{{±|0.3400|0.2410}}

|5511{{±|138}}

|

|0.0230{{±|0.0127}}

|0.225{{±|0.007}}

|13.11536{{±|0.00044|0.00060}}

|

|450

| style="background:#FFFF00" |transit

|397{{±|2}}

|0.552{{±|0.015}}

|3748{{±|138}}

|

|0.0586{{±|0.0342}}

|0.407{{±|0.007|0.010}}

|3.43547{{±|0.00003}}

|

|980

| style="background:#FFFF00" |transit

|643{{±|7}}

|1.034{{±|0.459|0.314}}

|4927{{±|138}}

|

|0.063{{±|0.039}}

|0.410{{±|0.027|0.026}}

|22.5494{{±|0.00137|0.00143}}

|

|720

| style="background:#FFFF00" |transit

|278{{±|2}}

|0.7980{{±|0.3390|0.2450}}

|5784{{±|138}}

|

|0.0066{{±|0.0035}}

|0.114{{±|0.008|0.007}}

|4.9419{{±|0.00066|0.00069}}

|

|1110

| style="background:#FFFF00" |transit

|

|

|

|

|0.0078{{±|0.0044}}

|0.121{{±|0.008|0.007}}

|9.22453{{±|0.00132|0.00091}}

|

|900

| style="background:#FFFF00" |transit

|

|

|

|

|0.0122{{±|0.0062}}

|0.149{{±|0.010|0.009}}

|20.97895{{±|0.00130|0.00124}}

|

|610

| style="background:#FFFF00" |transit

|

|

|

|

|0.0212{{±|0.0127}}

|0.221{{±|0.015|0.014}}

|1.90808{{±|0.00004|0.00005}}

|

|1800

| style="background:#FFFF00" |transit

|

|

|

|

|1.1{{±|0.1}}

|

|

|4.4{{±|1.9|0.4}}

|4700{{±|3300|700}}

| style="background:#0099FF" |microlensing

|17000{{±|700}}

|0.58{{±|0.03}}

|

|

|1.61{{±|0.14}}

|

|1460{{±|90}}

|2.1{{±|0.2}}

|

| style="background:#FF7519" |timing

|1340{{±|20}}

|0.48+0.12

|

|{{citation|arxiv=2202.02118|year=2022|title=Detection of two additional circumbinary planets around Kepler-451|author1=Ekrem Murat Esmer |last2=Baştürk |first2=Özgür |author3=Selim Osman Selam |last4=Aliş |first4=Sinan |journal=Monthly Notices of the Royal Astronomical Society |volume=511 |issue=4 |pages=5207–5216 |doi=10.1093/mnras/stac357 |doi-access=free |bibcode=2022MNRAS.511.5207E }}

|1.76{{±|0.18}}

|

|43.0{{±|0.1}}

|0.20{{±|0.03}}

|

| style="background:#FF7519" |timing

|1340{{±|20}}

|0.48+0.12

|

|

|0.40{{±|0.09}}

|

|1919{{±|27|24}}

|3.053{{±|0.049}}

|

| style="background:#00FF00" |radial vel.

|

|1.03{{±|0.04}}

|

|{{citation|arxiv=2204.00019|year=2022|title=Kepler-1656b's Extreme Eccentricity: Signature of a Gentle Giant|doi=10.3847/1538-3881/ac6094 |last1=Angelo |first1=Isabel |last2=Naoz |first2=Smadar |last3=Petigura |first3=Erik |last4=MacDougall |first4=Mason |last5=Stephan |first5=Alexander P. |last6=Isaacson |first6=Howard |last7=Howard |first7=Andrew W. |journal=The Astronomical Journal |volume=163 |issue=5 |page=227 |bibcode=2022AJ....163..227A |s2cid=247922620 |doi-access=free }}

| <4.6

| 0.8886{{±|0.0535|0.0526}}

| 737.11310{{±|0.00146|0.00770}}

| 1.64{{±|0.10}}

|

| style="background:#FFFF00" |transit

| 5436{{±|334|298}}

| 1.088{{±|0.072}}

| 6157{{±|231|202}}

| Possible exomoon host{{cite journal |last1=Kipping |first1=David |last2=Bryson |first2=Steve |display-authors=etal |date=13 January 2022 |title=An exomoon survey of 70 cool giant exoplanets and the new candidate Kepler-1708 b-i |journal=Nature |volume= 6|issue= 3|pages= 367–380|doi= 10.1038/s41550-021-01539-1|pmid=35399159 |pmc=8938273 |arxiv=2201.04643 |bibcode=2022NatAs...6..367K }}{{cite web |title=Kepler-1708 |url=https://exoplanetarchive.ipac.caltech.edu/overview/Kepler-1708 |website=NASA Exoplanet Archive |accessdate=13 January 2022}}

|0.0064{{±|0.0019}}

|0.072{{±|0.004}}

|7.54425{{±|0.00054}}

|

|

| style="background:#FFFF00" |transit

|923{{±|3}}

|1.12{{±|0.03}}

|5818{{±|27}}

|Very dense planets, additional planet in system suspected{{citation|arxiv=2201.11459|year=2022|title=Alleviating the transit timing variation bias in transit surveys|last1=Leleu |first1=A. |last2=Delisle |first2=J. -B. |last3=Mardling |first3=R. |last4=Udry |first4=S. |last5=Chatel |first5=G. |last6=Alibert |first6=Y. |last7=Eggenberger |first7=P. |journal=Astronomy & Astrophysics |volume=661 |pages=A141 |doi=10.1051/0004-6361/202142822 |s2cid=246294682 }}

|0.0066{{±|0.0020}}

|0.078{{±|0.005}}

|11.3295{{±|0.0011}}

|

|

| style="background:#FFFF00" |transit

|923{{±|3}}

|1.12{{±|0.03}}

|5818{{±|27}}

|Very dense planets, additional planet in system suspected

|0.007{{±|0.023|0.005}}

|

|

|2.44{{±|0.88|0.75}}

|

| style="background:#0099FF" |microlensing

|17000{{±|7000}}

|0.41{{±|0.25|0.21}}

|

|

|0.018{{±|0.011|0.009}}

|

|

|1.81{{±|0.55|0.59}}

|

| style="background:#0099FF" |microlensing

|18000{{±|6000|8000}}

|0.34{{±|0.22|0.17}}

|

|

|3.67{{±|2.17|2.07}}

|

|

|2.34{{±|0.56|0.74}}

|

| style="background:#0099FF" |microlensing

|17000{{±|4000|5000}}

|0.63{{±|0.37|0.35}}

|

|{{citation|arxiv=2209.00112|year=2022|title=KMT-2017-BLG-0673Lb and KMT-2019-BLG-0414Lb: Two microlensing planets detected in peripheral fields of KMTNet survey|last1=Han |first1=Cheongho |last2=Lee |first2=Chung-Uk |last3=Gould |first3=Andrew |author4=Youn Kil Jung |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Hwang |first7=Kyu-Ha |last8=Kim |first8=Doeon |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yang |first12=Hongjing |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |last16=Kim |first16=Dong-Jin |last17=Kim |first17=Seung-Lee |last18=Lee |first18=Dong-Joo |last19=Lee |first19=Yongseok |last20=Park |first20=Byeong-Gon |last21=Pogge |first21=Richard W. |journal=Astronomy & Astrophysics |volume=666 |pages=A132 |doi=10.1051/0004-6361/202244438 |bibcode=2022A&A...666A.132H |s2cid=251979813 }}

|0.016{{±|0.017|0.009}}

|

|

|1.38{{±|0.39|0.32}}

|

| style="background:#0099FF" |microlensing

|23000{{±|2000}}

|0.32{{±|0.31|0.17}}

|

|

|0.011{{±|0.006}}

|

|

|1.78{{±|0.45|0.46}}

|

| style="background:#0099FF" |microlensing

|14000{{±|6000}}

|0.41{{±|0.23|0.19}}

|

|{{citation|arxiv=2210.12344|year=2023|title=Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10−4 Planets from the First 4 yr Survey|last1=Zang |first1=Weicheng |author2=Youn Kil Jung |last3=Yang |first3=Hongjing |last4=Zhang |first4=Xiangyu |last5=Udalski |first5=Andrzej |last6=Yee |first6=Jennifer C. |last7=Gould |first7=Andrew |last8=Mao |first8=Shude |last9=Albrow |first9=Michael D. |last10=Chung |first10=Sun-Ju |last11=Han |first11=Cheongho |last12=Hwang |first12=Kyu-Ha |last13=Ryu |first13=Yoon-Hyun |last14=Shin |first14=In-Gu |last15=Shvartzvald |first15=Yossi |last16=Cha |first16=Sang-Mok |last17=Kim |first17=Dong-Jin |last18=Kim |first18=Hyoun-Woo |last19=Kim |first19=Seung-Lee |last20=Lee |first20=Chung-Uk |last21=Lee |first21=Dong-Joo |last22=Lee |first22=Yongseok |last23=Park |first23=Byeong-Gon |last24=Pogge |first24=Richard W. |last25=Mróz |first25=Przemek |last26=Skowron |first26=Jan |last27=Poleski |first27=Radoslaw |last28=Szymański |first28=Michał K. |last29=Soszyński |first29=Igor |last30=Pietrukowicz |first30=Paweł |journal=The Astronomical Journal |volume=165 |issue=3 |page=103 |doi=10.3847/1538-3881/acb34b |bibcode=2023AJ....165..103Z |s2cid=253098604 |display-authors=1 |doi-access=free }}

|1.45{{±|1.23|0.88}}

|

|

|4.39{{±|2.18|2.40}}

|

| style="background:#0099FF" |microlensing

|21000{{±|4000|6000}}

|0.51{{±|0.43|0.31}}

|

|{{citation|arxiv=2206.11409|year=2022|title=Systematic KMTNet Planetary Anomaly Search. VI. Complete Sample of 2018 Sub-prime-field Planets|author1=Youn Kil Jung |last2=Zang |first2=Weicheng |last3=Han |first3=Cheongho |last4=Gould |first4=Andrew |last5=Udalski |first5=Andrzej |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Hwang |first8=Kyu-Ha |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yang |first12=Hongjing |last13=Yee |first13=Jennifer C. |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |last16=Kim |first16=Seung-Lee |last17=Lee |first17=Chung-Uk |last18=Lee |first18=Dong-Joo |last19=Lee |first19=Yongseok |last20=Park |first20=Byeong-Gon |last21=Pogge |first21=Richard W. |last22=Mróz |first22=Przemek |last23=Szymański |first23=Michał K. |last24=Skowron |first24=Jan |last25=Poleski |first25=Radek |last26=Soszyński |first26=Igor |last27=Pietrukowicz |first27=Paweł |last28=Kozłowski |first28=Szymon |last29=Ulaczyk |first29=Krzysztof |last30=Rybicki |first30=Krzysztof A. |journal=The Astronomical Journal |volume=164 |issue=6 |page=262 |doi=10.3847/1538-3881/ac9c5c |bibcode=2022AJ....164..262J |s2cid=249953591 |display-authors=1 |doi-access=free }}

|0.23{{±|0.32|0.12}}

|

|

|0.87{{±|0.24|0.25}}

|

| style="background:#0099FF" |microlensing

|23000{{±|3000|4000}}

|0.10{{±|0.14|0.05}}

|

|

|2.11{{±|2.09|1.04}}

|

|

|2.46{{±|0.51|0.58}}

|

| style="background:#0099FF" |microlensing

|22000{{±|3000|4000}}

|0.29{{±|0.28|0.14}}

|

|

|0.27{{±|\0.12}}

|

|

|4.62{{±|0.80|1.10}}

|

| style="background:#0099FF" |microlensing

|23000{{±|3000|4000}}

|0.69{{±|0.32|0.31}}

|

|

|1.15{{±|0.73|0.63}}

|

|

|3.81{{±|2.96|2.32}}

|

| style="background:#0099FF" |microlensing

|14000{{±|6000}}

|0.66{{±|0.42|0.36}}

|

|

|16.0{{±|11.7|8.0}}

|

|

|4.86{{±|2.97|2.55}}

|

| style="background:#0099FF" |microlensing

|15000{{±|10000|7000}}

|0.82{{±|0.57|0.39}}

|

|

|4.57{{±|3.74|2.06}}

|

|

|1.16{{±|0.47|0.51}}

|

| style="background:#0099FF" |microlensing

|14000{{±|5000|6000}}

|0.74{{±|0.43|0.38}}

|

|

|0.19{{±|0.21|0.11}}

|

|

|1.7{{±|0.5}}

|

| style="background:#0099FF" |microlensing

|22000{{±|3000|5000}}

|0.30{{±|0.34|0.18}}

|

|{{citation|arxiv=2204.02017|year=2022|title=Systematic KMTNet planetary anomaly search. IV. Complete sample of 2019 prime-field|last1=Zang |first1=Weicheng |last2=Yang |first2=Hongjing |last3=Han |first3=Cheongho |last4=Lee |first4=Chung-Uk |last5=Udalski |first5=Andrzej |last6=Gould |first6=Andrew |last7=Mao |first7=Shude |last8=Zhang |first8=Xiangyu |last9=Zhu |first9=Wei |last10=Albrow |first10=Michael D. |last11=Chung |first11=Sun-Ju |last12=Hwang |first12=Kyu-Ha |author13=Youn Kil Jung |last14=Ryu |first14=Yoon-Hyun |last15=Shin |first15=In-Gu |last16=Shvartzvald |first16=Yossi |last17=Yee |first17=Jennifer C. |last18=Cha |first18=Sang-Mok |last19=Kim |first19=Dong-Jin |last20=Kim |first20=Hyoun-Woo |last21=Kim |first21=Seung-Lee |last22=Lee |first22=Dong-Joo |last23=Lee |first23=Yongseok |last24=Park |first24=Byeong-Gon |last25=Mróz |first25=Przemek |last26=Skowron |first26=Jan |last27=Poleski |first27=Radoslaw |last28=Szymański |first28=Michał K. |last29=Soszyński |first29=Igor |last30=Pietrukowicz |first30=Paweł |journal=Monthly Notices of the Royal Astronomical Society |volume=515 |pages=928–939 |doi=10.1093/mnras/stac1883 |doi-access=free |display-authors=1 }}

|0.013{{±|0.008|0.007}}

|

|

|1.70{{±|0.50|0.56}}

|

| style="background:#0099FF" |microlensing

|15000{{±|8000|7000}}

|0.25{{±|0.16|0.13}}

|

|

|4.05{{±|1.73|1.85}}

|

|

|2.6{{±|0.6|0.8}}

|

| style="background:#0099FF" |microlensing

|15000{{±|6000|5000}}

|0.79{{±|0.33|0.36}}

|

|

|0.015{{±|0.005}}

|

|

|3.02{{±|0.70|0.73}}

|

| style="background:#0099FF" |microlensing

|22000{{±|2000|7000}}

|0.74{{±|0.25}}

|

|

|0.28{{±|0.29|0.18}}

|

|

|2.0{{±|0.8|0.7}}

|

| style="background:#0099FF" |microlensing

|20000{{±|5000|7000}}

|0.47{{±|0.41|0.28}}

|

|

|0.0352{{±|0.0173|0.0142}}

|

|

|3.5{{±|1.3|1.0}}

|

| style="background:#0099FF" |microlensing

|15000{{±|5000|4000}}

|0.78{{±|0.29|0.26}}

|

|{{citation|arxiv=2205.12584|year=2022|title=KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: Two microlensing planets in the KMTNet high-cadence fields with followup observations|last1=Yang |first1=Hongjing |last2=Zang |first2=Weicheng |last3=Gould |first3=Andrew |last4=Yee |first4=Jennifer C. |last5=Hwang |first5=Kyu-Ha |last6=Christie |first6=Grant |last7=Sumi |first7=Takahiro |last8=Zhang |first8=Jiyuan |last9=Mao |first9=Shude |last10=Albrow |first10=Michael D. |last11=Chung |first11=Sun-Ju |last12=Han |first12=Cheongho |author13=Youn Kil Jung |last14=Ryu |first14=Yoon-Hyun |last15=Shin |first15=In-Gu |last16=Shvartzvald |first16=Yossi |last17=Cha |first17=Sang-Mok |last18=Kim |first18=Dong-Jin |last19=Kim |first19=Hyoun-Woo |last20=Kim |first20=Seung-Lee |last21=Lee |first21=Chung-Uk |last22=Lee |first22=Dong-Joo |last23=Lee |first23=Yongseok |last24=Park |first24=Byeong-Gon |last25=Pogge |first25=Richard W. |last26=Drummond |first26=John |last27=Maoz |first27=Dan |last28=McCormick |first28=Jennie |last29=Natusch |first29=Tim |last30=Penny |first30=Matthew T. |journal=Monthly Notices of the Royal Astronomical Society |volume=516 |issue=2 |pages=1894–1909 |doi=10.1093/mnras/stac2023 |doi-access=free |display-authors=1 }}

|0.40{{±|0.07|0.08}}

|

|

|2.5{{±|2.8|1.9}}

|

| style="background:#0099FF" |microlensing

|23000{{±|3000|5000}}

|0.47{{±|0.33|0.24}}

|

|Multiple solutions for orbital separation{{citation|arxiv=2204.11383|year=2022|title=KMT-2021-BLG-0240: Microlensing event with a deformed planetary signal|last1=Han |first1=Cheongho |last2=Kim |first2=Doeon |last3=Yang |first3=Hongjing |last4=Gould |first4=Andrew |author5=Youn Kil Jung |last6=Albrow |first6=Michael D. |last7=Chung |first7=Sun-Ju |last8=Hwang |first8=Kyu-Ha |last9=Lee |first9=Chung-Uk |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yee |first13=Jennifer C. |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |last16=Kim |first16=Dong-Jin |last17=Kim |first17=Seung-Lee |last18=Lee |first18=Dong-Joo |last19=Lee |first19=Yongseok |last20=Park |first20=Byeong-Gon |last21=Pogge |first21=Richard W. |journal=Astronomy & Astrophysics |volume=664 |pages=A114 |doi=10.1051/0004-6361/202243161 |bibcode=2022A&A...664A.114H |s2cid=248377479 }}

|0.64{{±|0.25|0.24}}

|

|

|1.0{{±|1.1|0.8}}

|

| style="background:#0099FF" |microlensing

|23000{{±|3000|5000}}

|0.47{{±|0.33|0.24}}

|

|Multiple solutions for orbital separation

|0.10{{±|0.13|0.07}}

|

|

|1.54{{±|0.24|0.30}}

|

| style="background:#0099FF" |microlensing

|23000{{±|3000|4000}}

|0.32{{±|0.39|0.21}}

|

|

|0.45{{±|0.40|0.25}}

|

|

|2.43{{±|0.67}}

|

| style="background:#0099FF" |microlensing

|20000{{±|3000|4000}}

|0.36{{±|0.32|0.20}}

|

|

|5.97{{±|2.94|2.60}}

|

|

|3.23{{±|0.76|0.80}}

|

| style="background:#0099FF" |microlensing

|11000{{±|6000|4000}}

|0.69{{±|0.34|0.30}}

|

|Multiple orbital solutions{{citation|arxiv=2209.03886|year=2023|title=Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets|last1=Shin |first1=In-Gu |last2=Yee |first2=Jennifer C. |last3=Gould |first3=Andrew |last4=Hwang |first4=Kyu-Ha |last5=Yang |first5=Hongjing |last6=Bond |first6=Ian A. |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Han |first9=Cheongho |author10=Youn Kil Jung |last11=Ryu |first11=Yoon-Hyun |last12=Shvartzvald |first12=Yossi |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |last16=Kim |first16=Seung-Lee |last17=Lee |first17=Chung-Uk |last18=Lee |first18=Dong-Joo |last19=Lee |first19=Yongseok |last20=Park |first20=Byeong-Gon |last21=Pogge |first21=Richard W. |last22=Abe |first22=Fumio |last23=Barry |first23=Richard |last24=Bennett |first24=David P. |last25=Bhattacharya |first25=Aparna |last26=Fujii |first26=Hirosane |last27=Fukui |first27=Akihiko |last28=Hirao |first28=Yuki |author29=Stela Ishitani Silva |last30=Itow |first30=Yoshitaka |journal=The Astronomical Journal |volume=165 |issue=1 |page=8 |doi=10.3847/1538-3881/ac9d93 |bibcode=2023AJ....165....8S |s2cid=254407196 |display-authors=1 |doi-access=free }}

|0.19{{±|0.09|0.10}}

|

|

|2.07{{±|0.35|0.47}}

|

| style="background:#0099FF" |microlensing

|22000{{±|3000|5000}}

|0.55{{±|0.26|0.28}}

|

|Multiple orbital solutions

|0.12{{±|0.06|0.04}}

|

|

|2.22{{±|0.66|0.48}}

|

| style="background:#0099FF" |microlensing

|10000{{±|3000|2000}}

|0.22{{±|0.12|0.07}}

|

|{{citation|arxiv=2207.07295|title=Mass Production of 2021 KMTNet Microlensing Planets II|last1=Ryu |first1=Yoon-Hyun |last2=Shin |first2=In-Gu |last3=Yang |first3=Hongjing |last4=Gould |first4=Andrew |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Han |first7=Cheongho |last8=Hwang |first8=Kyu-Ha |author9=Youn Kil Jung |last10=Shvartzvald |first10=Yossi |last11=Yee |first11=Jennifer C. |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=%Hyoun-Woo |last16=Kim |first16=Seung-Lee |last17=Lee |first17=Chung-Uk |last18=Lee |first18=Dong-Joo |last19=Lee |first19=Yongseok |last20=Park |first20=Byeong-Gon |last21=Pogge |first21=Richard W. |journal=The Astronomical Journal |year=2023 |volume=165 |issue=3 |page=83 |doi=10.3847/1538-3881/acab6b |bibcode=2023AJ....165...83R |s2cid=256544515 |doi-access=free }}

|1.26{{±|1.01|0.66}}

|

|

|1.75{{±|0.42}}

|

| style="background:#0099FF" |microlensing

|21000{{±|3000|5000}}

|0.38{{±|0.30|0.20}}

|

|

|0.22{{±|0.31|0.12}}

|

|

|1.26{{±|1.41|1.08}}

|

| style="background:#0099FF" |microlensing

|27000{{±|3000}}

|0.14{{±|0.19|0.07}}

|

|{{citation|arxiv=2203.16734|year=2022|title=KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensing|last1=Han |first1=Cheongho |last2=Gould |first2=Andrew |last3=Bond |first3=Ian A. |author4=Youn Kil Jung |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Hwang |first7=Kyu-Ha |last8=Ryu |first8=Yoon-Hyun |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Yee |first11=Jennifer C. |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Seung-Lee |last16=Lee |first16=Chung-Uk |last17=Lee |first17=Dong-Joo |last18=Lee |first18=Yongseok |last19=Park |first19=Byeong-Gon |last20=Pogge |first20=Richard W. |last21=Kim |first21=Doeon |last22=Abe |first22=Fumio |last23=Barry |first23=Richard K. |last24=Bennett |first24=David P. |last25=Bhattacharya |first25=Aparna |last26=Fujii |first26=Hirosane |last27=Fukui |first27=Akihiko |last28=Hirao |first28=Yuki |last29=Itow |first29=Yoshitaka |last30=Kirikawa |first30=Rintaro |journal=Astronomy & Astrophysics |volume=662 |pages=A70 |doi=10.1051/0004-6361/202243550 |bibcode=2022A&A...662A..70H |s2cid=247839227 |display-authors=1 }}

|0.25{{±|0.35|0.13}}

|

|

|0.93{{±|1.05|0.80}}

|

| style="background:#0099FF" |microlensing

|27000{{±|3000}}

|0.14{{±|0.19|0.07}}

|

|

|1.30{{±|0.68}}

|

|

|3.54{{±|1.06}}

|

| style="background:#0099FF" |microlensing

|15000{{±|5000}}

|0.63{{±|0.33}}

|

|

|0.0599{{±|0.0643|0.0319}}

|

|

|1.52{{±|0.57|0.41}}

|

| style="background:#0099FF" |microlensing

|22000{{±|3000|4000}}

|0.24{{±|0.26|0.13}}

|

|

|0.38{{±|0.22|0.20}}

|

|

|2.89{{±|0.44|0.66}}

|

| style="background:#0099FF" |microlensing

|20000{{±|3000|5000}}

|0.57{{±|0.32|0.29}}

|

|Host star also known as MOA-2021-BLG-182

|0.1928{{±|0.1129}}

|

|

|2.37{{±|0.77}}

|

| style="background:#0099FF" |microlensing

|19000{{±|5000|8000}}

|0.42{{±|0.25}}

|

|

|0.0143{{±|0.0073}}

|

|

|2.29{{±|0.56|0.71}}

|

| style="background:#0099FF" |microlensing

|19000{{±|3000|5000}}

|0.37{{±|0.19}}

|

|{{citation|arxiv=2202.03022|year=2022|title=Mass Production of 2021 KMTNet Microlensing Planets I|last1=Ryu |first1=Yoon-Hyun |author2=Youn Kil Jung |last3=Yang |first3=Hongjing |last4=Gould |first4=Andrew |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Han |first7=Cheongho |last8=Hwang |first8=Kyu-Ha |last9=Shin |first9=In-Gu |last10=Shvartzvald |first10=Yossi |last11=Yee |first11=Jennifer C. |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=%Hyoun-Woo |last16=Kim |first16=Seung-Lee |last17=Lee |first17=Chung-Uk |last18=Lee |first18=Dong-Joo |last19=Lee |first19=Yongseok |last20=Park |first20=Byeong-Gon |last21=Pogge |first21=Richard |journal=The Astronomical Journal |volume=164 |issue=5 |page=180 |doi=10.3847/1538-3881/ac8d6c |bibcode=2022AJ....164..180R |s2cid=246634000 |doi-access=free }}

|0.12{{±|0.20|0.07}}

|

|

|0.72{{±|0.13|0.14}}

|

| style="background:#0099FF" |microlensing

|25000{{±|3000|4000}}

|0.08{{±|0.13|0.04}}

|

|

|0.145{{±|0.094|0.072}}

|

|

|2.5{{±|0.8|06}}

|

| style="background:#0099FF" |microlensing

|23000{{±|2000|4000}}

|0.58{{±|0.33|0.27}}

|

|

|0.73{{±|0.50|0.40}}

|

|

|1.9{{±|0.3|0.5}}

|

| style="background:#0099FF" |microlensing

|23000{{±|3000|4000}}

|0.48{{±|0.33|0.26}}

|

|Possibly a binary star system{{citation|arxiv=2204.11378|year=2022|title=KMT-2021-BLG-1898: Planetary microlensing event involved with binary source stars|last1=Han |first1=Cheongho |last2=Gould |first2=Andrew |last3=Kim |first3=Doeon |author4=Youn Kil Jung |last5=Albrow |first5=Michael D. |last6=Chung |first6=Sun-Ju |last7=Hwang |first7=Kyu-Ha |last8=Lee |first8=Chung-Uk |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Yee |first12=Jennifer C. |last13=Zang |first13=Weicheng |last14=Cha |first14=Sang-Mok |last15=Kim |first15=Dong-Jin |last16=Kim |first16=Seung-Lee |last17=Lee |first17=Dong-Joo |last18=Lee |first18=Yongseok |last19=Park |first19=Byeong-Gon |last20=Pogge |first20=Richard W. |journal=Astronomy & Astrophysics |volume=663 |pages=A145 |doi=10.1051/0004-6361/202243102 |bibcode=2022A&A...663A.145H |s2cid=248377122 }}

|0.07{{±|0.10|0.03}}

|

|

|0.94{{±|0.16}}

|

| style="background:#0099FF" |microlensing

|22000{{±|3000}}

|0.11{{±|0.17|0.06}}

|

|Multiple orbital solutions

|0.80{{±|0.56|0.35}}

|

|

|1.38{{±|0.26}}

|

| style="background:#0099FF" |microlensing

|8000{{±|4000|3000}}

|0.12{{±|0.09|0.06}}

|

|

|0.0147{{±|0.0014}}

|

|8.781{{±|0.007}}

|0.048{{±|0.006}}

|330

| style="background:#00FF00" |radial vel.

|33.31

|0.21

|3129

|Host star also known as Gliese 3049{{citation|arxiv=2210.12710|year=2023|title=L 363-38 b: A planet newly discovered with ESPRESSO orbiting a nearby M dwarf star|last1=Sartori |first1=Lia F. |last2=Lovis |first2=Christophe |last3=Delisle |first3=Jean-Baptiste |last4=Lendl |first4=Monika |last5=Cugno |first5=Gabriele |last6=Boehle |first6=Anna |last7=Dannert |first7=Felix |last8=Krenn |first8=Andrea |last9=Gubler |first9=Jonas L. |last10=Quanz |first10=Sascha P. |journal=Astronomy & Astrophysics |volume=670 |pages=A42 |doi=10.1051/0004-6361/202244347 |bibcode=2023A&A...670A..42S |s2cid=253098575 }}

|30

|

|

|

|

| style="background:#0099FF" |microlensing

|8000{{±|2000}}

|0.8

|

|{{citation|arxiv=2205.07522|year=2022|title=MOA-2019-BLG-008Lb: A New Microlensing Detection of an Object at the Planet/Brown Dwarf Boundary|doi=10.3847/1538-3881/ac78ed |last1=Bachelet |first1=E. |last2=Tsapras |first2=Y. |last3=Gould |first3=Andrew |last4=Street |first4=R. A. |last5=Bennett |first5=David P. |last6=Hundertmark |first6=M. P. G. |last7=Bozza |first7=V. |last8=Bramich |first8=D. M. |last9=Cassan |first9=A. |last10=Dominik |first10=M. |last11=Horne |first11=K. |last12=Mao |first12=S. |last13=Saha |first13=A. |last14=Wambsganss |first14=J. |last15=Zang |first15=Weicheng |last16=Abe |first16=Fumio |last17=Barry |first17=Richard |last18=Bennett |first18=David P. |last19=Bhattacharya |first19=Aparna |last20=Bond |first20=Ian A. |last21=Fukui |first21=Akihiko |last22=Fujii |first22=Hirosane |last23=Hirao |first23=Yuki |last24=Itow |first24=Yoshitaka |last25=Kirikawa |first25=Rintaro |last26=Kondo |first26=Iona |last27=Koshimoto |first27=Naoki |last28=Matsubara |first28=Yutaka |last29=Matsumoto |first29=Sho |last30=Miyazaki |first30=Shota |journal=The Astronomical Journal |volume=164 |issue=3 |page=75 |bibcode=2022AJ....164...75B |s2cid=248810881 |display-authors=1 |doi-access=free }}

|0.036{{±|0.060|0.021}}

|

|

|1.11{{±|0.23|0.20}}

|

| style="background:#0099FF" |microlensing

|26000{{±|3000}}

|0.23{{±|0.39|0.14}}

|

|{{citation|arxiv=2204.03672|year=2022|title=MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis|author1=Stela Ishitani Silva |last2=Ranc |first2=Clément |last3=Bennett |first3=David P. |last4=Bond |first4=Ian A. |last5=Zang |first5=Weicheng |last6=Abe |first6=Fumio |last7=Barry |first7=Richard K. |last8=Bhattacharya |first8=Aparna |last9=Fujii |first9=Hirosane |last10=Fukui |first10=Akihiko |last11=Hirao |first11=Yuki |last12=Itow |first12=Yoshitaka |last13=Kirikawa |first13=Rintaro |last14=Kondo |first14=Iona |last15=Koshimoto |first15=Naoki |last16=Matsubara |first16=Yutaka |last17=Matsumoto |first17=Sho |last18=Miyazaki |first18=Shota |last19=Muraki |first19=Yasushi |last20=Olmschenk |first20=Greg |last21=Okamura |first21=Arisa |last22=Rattenbury |first22=Nicholas J. |last23=Satoh |first23=Yuki |last24=Sumi |first24=Takahiro |last25=Suzuki |first25=Daisuke |last26=Toda |first26=Taiga |last27=Tristram |first27=Paul . J. |last28=Vandorou |first28=Aikaterini |last29=Yama |first29=Hibiki |last30=Petric |first30=Andreea |journal=The Astronomical Journal |volume=164 |issue=3 |page=118 |doi=10.3847/1538-3881/ac82b8 |bibcode=2022AJ....164..118I |s2cid=248069150 |display-authors=1 |doi-access=free }}

|0.217{{±|0.116|0.106}}

|

|

|2.88{{±|0.40|0.41}}

|

| style="background:#0099FF" |microlensing

|25000{{±|3000}}

|0.656{{±|0.346|0.322}}

|

|{{citation|arxiv=2210.02436|year=2023|title=MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert|last1=Olmschenk |first1=Greg |last2=Bennett |first2=David P. |last3=Bond |first3=Ian A. |last4=Zang |first4=Weicheng |author5=Youn Kil Jung |last6=Yee |first6=Jennifer C. |last7=Bachelet |first7=Etienne |last8=Abe |first8=Fumio |last9=Barry |first9=Richard K. |last10=Bhattacharya |first10=Aparna |last11=Fujii |first11=Hirosane |last12=Fukui |first12=Akihiko |last13=Hirao |first13=Yuki |author14=Stela Ishitani Silva |last15=Itow |first15=Yoshitaka |last16=Kirikawa |first16=Rintaro |last17=Kondo |first17=Iona |last18=Koshimoto |first18=Naoki |last19=Matsubara |first19=Yutaka |last20=Matsumoto |first20=Sho |last21=Miyazaki |first21=Shota |last22=Munford |first22=Brandon |last23=Muraki |first23=Yasushi |last24=Okamura |first24=Arisa |last25=Ranc |first25=Clément |last26=Rattenbury |first26=Nicholas J. |last27=Satoh |first27=Yuki |last28=Sumi |first28=Takahiro |last29=Suzuki |first29=Daisuke |last30=Toda |first30=Taiga |journal=The Astronomical Journal |volume=165 |issue=4 |page=175 |doi=10.3847/1538-3881/acbcc8 |bibcode=2023AJ....165..175O |s2cid=252715812 |display-authors=1 |doi-access=free }}

|14.4

|

|

|290

|

| style="background:#FF6CDA" |imaging

|474

|9.1

|21900

|{{citation|arxiv=2205.02279|year=2022|title=A scaled-up planetary system around a supernova progenitor|last1=Squicciarini |first1=V. |last2=Gratton |first2=R. |last3=Janson |first3=M. |last4=Mamajek |first4=E. E. |last5=Chauvin |first5=G. |last6=Delorme |first6=P. |last7=Langlois |first7=M. |last8=Vigan |first8=A. |last9=Ringqvist |first9=S. C. |last10=Meeus |first10=G. |last11=Reffert |first11=S. |last12=Kenworthy |first12=M. |last13=Meyer |first13=M. R. |last14=Bonnefoy |first14=M. |last15=Bonavita |first15=M. |last16=Mesa |first16=D. |last17=Samland |first17=M. |last18=Desidera |first18=S. |last19=D'Orazi |first19=V. |last20=Engler |first20=N. |last21=Alecian |first21=E. |last22=Miglio |first22=A. |last23=Henning |first23=T. |last24=Quanz |first24=S. P. |last25=Mayer |first25=L. |last26=Flasseur |first26=O. |last27=Marleau |first27=G. D. |journal=Astronomy & Astrophysics |volume=664 |pages=A9 |doi=10.1051/0004-6361/202243675 |bibcode=2022A&A...664A...9S |s2cid=248524983 }}

|18.5

|

|

|21

|

| style="background:#FF6CDA" |imaging

|474

|9.1

|21900

|

|2.98{{±|0.16|0.15}}

|1.07{{±|0.04}}

|54.18915{{±|0.00015}}

|0.313{{±|0.013}}

|688{{±|14|13}}

| style="background:#FFFF00" |transit

|1195{{±|8}}

|1.47{{±|0.09}}

|5980{{±|80}}

|Planet on eccentric orbit, host star also known as TOI-5152{{citation|arxiv=2207.03911|year=2022|title=Two long-period transiting exoplanets on eccentric orbits: NGTS-20 b (TOI-5152 b) and TOI-5153 B|doi=10.1051/0004-6361/202243583 |last1=Ulmer-Moll |first1=S. |last2=Lendl |first2=M. |last3=Gill |first3=S. |last4=Villanueva |first4=S. |last5=Hobson |first5=M. J. |last6=Bouchy |first6=F. |last7=Brahm |first7=R. |last8=Dragomir |first8=D. |last9=Grieves |first9=N. |last10=Mordasini |first10=C. |last11=Anderson |first11=D. R. |last12=Acton |first12=J. S. |last13=Bayliss |first13=D. |last14=Bieryla |first14=A. |last15=Burleigh |first15=M. R. |last16=Casewell |first16=S. L. |last17=Chaverot |first17=G. |last18=Eigmüller |first18=P. |last19=Feliz |first19=D. |last20=Gaudi |first20=B. S. |last21=Gillen |first21=E. |last22=Goad |first22=M. R. |last23=Gupta |first23=A. F. |last24=Günther |first24=M. N. |last25=Henderson |first25=B. A. |last26=Henning |first26=T. |last27=Jenkins |first27=J. S. |last28=Jones |first28=M. |last29=Jordán |first29=A. |last30=Kendall |first30=A. |journal=Astronomy & Astrophysics |volume=666 |pages=A46 |bibcode=2022A&A...666A..46U |s2cid=250408027 |display-authors=1 }}

|2.36{{±|0.21}}

|1.33{{±|0.03}}

|1.5433897{{±|0.0000016}}

|0.0236{{±|0.0005}}

|1357{{±|15}}

| style="background:#FFFF00" |transit

|2090{{±|90|80}}

|0.72{{±|0.04}}

|4660{{±|41}}

|{{citation|arxiv=2210.01027|year=2022|title=NGTS-21b: An Inflated Super-Jupiter Orbiting a Metal-poor K dwarf|doi=10.1093/mnras/stac2884 |last1=Alves |first1=Douglas R. |last2=Jenkins |first2=James S. |last3=Vines |first3=Jose I. |last4=Nielsen |first4=Louise D. |last5=Gill |first5=Samuel |last6=Acton |first6=Jack S. |last7=Anderson |first7=D. R. |last8=Bayliss |first8=Daniel |last9=Bouchy |first9=François |last10=Breytenbach |first10=Hannes |last11=Bryant |first11=Edward M. |last12=Burleigh |first12=Matthew R. |last13=Casewell |first13=Sarah L. |last14=Eigmüller |first14=Philipp |last15=Gillen |first15=Edward |last16=Goad |first16=Michael R. |last17=Günther |first17=Maximilian N. |last18=Henderson |first18=Beth A. |last19=Kendall |first19=Alicia |last20=Lendl |first20=Monika |last21=Moyano |first21=Maximiliano |last22=Sefako |first22=Ramotholo R. |last23=Smith |first23=Alexis M S. |last24=Costes |first24=Jean C. |last25=Tilbrook |first25=Rosanne H. |last26=Thomas |first26=Jessymol K. |last27=Udry |first27=Stéphane |last28=Watson |first28=Christopher A. |last29=West |first29=Richard G. |last30=Wheatley |first30=Peter J. |journal=Monthly Notices of the Royal Astronomical Society |volume=517 |issue=3 |pages=4447–4457 |doi-access=free |display-authors=1 }}

|0.613{{±|0.097}}

|1.267{{±|0.030}}

|4.0764326{{±|0.0000041}}

|0.0504{{±|0.012}}

|1327{{±|17|16}}

| style="background:#FFFF00" |transit

|3230{{±|70}}

|1.01{{±|0.06|0.07}}

|6057{{±|64}}

|{{citation|arxiv=2211.01044|year=2022|title=The discovery of three hot Jupiters, NGTS-23b, 24b and 25b, and updated parameters for HATS-54b from the Next Generation Transit Survey|doi=10.1093/mnras/stac3192 |last1=Jackson |first1=David G. |last2=Watson |first2=Christopher A. |last3=De Mooij |first3=Ernst J W. |last4=Acton |first4=Jack S. |last5=Alves |first5=Douglas R. |last6=Anderson |first6=David R. |last7=Armstrong |first7=David J. |last8=Bayliss |first8=Daniel |last9=Belardi |first9=Claudia |last10=Bouchy |first10=François |last11=Bryant |first11=Edward M. |last12=Burleigh |first12=Matthew R. |last13=Casewell |first13=Sarah L. |last14=Costes |first14=Jean C. |last15=Eigmüller |first15=Phillip |last16=Goad |first16=Michael R. |last17=Gill |first17=Samuel |last18=Gillen |first18=Edward |last19=Günther |first19=Maximilian N. |last20=Hawthorn |first20=Faith |last21=Henderson |first21=Beth A. |last22=Jackman |first22=James A G. |last23=Jenkins |first23=James S. |last24=Lendl |first24=Monika |last25=Kendall |first25=Alicia |last26=McCormac |first26=James |last27=Moyano |first27=Maximiliano |last28=Nielsen |first28=Louise D. |last29=Osborn |first29=Ares |last30=Sefako |first30=Ramotholo R. |journal=Monthly Notices of the Royal Astronomical Society |volume=518 |issue=4 |pages=4845–4860 |doi-access=free |display-authors=1 }}

|0.52{{±|0.12|0.11}}

|1.214{{±|0.058|0.062}}

|3.4678796{{±|0.0000070}}

|0.0479{{±|0.0028|0.0030}}

|1499{{±|41|36}}

| style="background:#FFFF00" |transit

|2360{{±|80}}

|1.26{{±|0.05|0.21}}

|5820{{±|93|8}}

|

|0.639{{±|0.058|0.052}}

|1.023{{±|0.035|0.052}}

|2.8230930{{±|0.0000033}}

|0.0388{{±|0.0014|0.002}}

|1101{{±|15|14}}

| style="background:#FFFF00" |transit

|2350{{±|30}}

|0.91{{±|0.03|0.04}}

|5321{{±|58}}

|

|0.71{{±|0.12}}

|

|

|2.13{{±|0.33}}

|

| style="background:#0099FF" |microlensing

|26000{{±|2000}}

|0.46{{±|0.08}}

|

|{{citation|arxiv=2201.04312|year=2022|title=OGLE-2016-BLG-1093Lb: A Sub-Jupiter-mass Spitzer Planet Located in the Galactic Bulge|doi=10.3847/1538-3881/ac6513 |last1=Shin |first1=In-Gu |last2=Yee |first2=Jennifer C. |last3=Hwang |first3=Kyu-Ha |last4=Gould |first4=Andrew |last5=Udalski |first5=Andrzej |last6=Bond |first6=Ian A. |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Han |first9=Cheongho |last10=Kil Jung |first10=Youn |last11=Woo Kim |first11=Hyoun |last12=Ryu |first12=Yoon-Hyun |last13=Shvartzvald |first13=Yossi |last14=Zang |first14=Weicheng |last15=Cha |first15=Sang-Mok |last16=Kim |first16=Dong-Jin |last17=Kim |first17=Seung-Lee |last18=Lee |first18=Chung-Uk |last19=Lee |first19=Dong-Joo |last20=Lee |first20=Yongseok |last21=Park |first21=Byeong-Gon |last22=Pogge |first22=Richard W. |last23=Mróz |first23=Przemek |last24=Szymański |first24=Michał K. |last25=Skowron |first25=Jan |last26=Poleski |first26=Radek |last27=Soszyński |first27=Igor |last28=Pietrukowicz |first28=Paweł |last29=Kozłowski |first29=Szymon |last30=Ulaczyk |first30=Krzysztof |journal=The Astronomical Journal |volume=163 |issue=6 |page=254 |bibcode=2022AJ....163..254S |s2cid=245877628 |display-authors=1 |doi-access=free }}

|0.046{{±|0.037|0.025}}

|

|

|2.41{{±|0.34|0.44}}

|

| style="background:#0099FF" |microlensing

|24000{{±|3000|4000}}

|0.45{{±|0.36|0.25}}

|

|Host star also known as KMT-2017-BLG-0752{{citation|arxiv=2205.10510|year=2022|title=Four sub-Jovian-mass planets detected by high-cadence microlensing surveys|last1=Han |first1=Cheongho |last2=Kim |first2=Doeon |last3=Gould |first3=Andrew |last4=Udalski |first4=Andrzej |last5=Bond |first5=Ian A. |last6=Bozza |first6=Valerio |author7=Youn Kil Jung |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |last10=Hwang |first10=Kyu-Ha |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Zang |first15=Weicheng |last16=Cha |first16=Sang-Mok |last17=Kim |first17=Dong-Jin |last18=Kim |first18=Seung-Lee |last19=Lee |first19=Chung-Uk |last20=Lee |first20=Dong-Joo |last21=Lee |first21=Yongseok |last22=Park |first22=Byeong-Gon |last23=Pogge |first23=Richard W. |last24=Mróz |first24=Przemek |last25=Szymański |first25=Michał K. |last26=Skowron |first26=Jan |last27=Poleski |first27=Radosław |last28=Soszyński |first28=Igor |last29=Pietrukowicz |first29=Paweł |last30=Kozłowski |first30=Szymon |journal=Astronomy & Astrophysics |volume=664 |pages=A33 |doi=10.1051/0004-6361/202243484 |bibcode=2022A&A...664A..33H |s2cid=248986310 |display-authors=1 }}

|0.017{{±|0.015|0.009}}

|

|

|1.75{{±|0.46|0.47}}

|

| style="background:#0099FF" |microlensing

|21000{{±|3000|5000}}

|0.38{{±|0.34|0.20}}

|

|

|0.14{{±|0.07|0.06}}

|

|

|2.86{{±|0.73|0.80}}

|

| style="background:#0099FF" |microlensing

|21000{{±|3000|4000}}

|0.69{{±|0.34|0.30}}

|

|

|0.89{{±|0.36|0.31}}

|

|

|1.75{{±|0.24|0.23}}

|

| style="background:#0099FF" |microlensing

|22000{{±|3000}}

|0.72{{±|0.29|0.25}}

|

|

|0.91{{±|0.66|0.52}}

|

|

|4.06{{±|2.14|2.58}}

|

| style="background:#0099FF" |microlensing

|19000{{±|5000|8000}}

|0.48{{±|0.35|0.28}}

|

|

|0.056{{±|0.033|0.031}}

|

|

|3.23{{±|1.29|1.71}}

|

| style="background:#0099FF" |microlensing

|19000{{±|6000|8000}}

|0.69{{±|0.41|0.38}}

|

|{{citation|arxiv=2204.04354|year=2022|title=Systematic KMTNet planetary anomaly search|last1=Gould |first1=Andrew |last2=Han |first2=Cheongho |last3=Zang |first3=Weicheng |last4=Yang |first4=Hongjing |last5=Hwang |first5=Kyu-Ha |last6=Udalski |first6=Andrzej |last7=Bond |first7=Ian A. |last8=Albrow |first8=Michael D. |last9=Chung |first9=Sun-Ju |author10=Youn Kil Jung |last11=Ryu |first11=Yoon-Hyun |last12=Shin |first12=In-Gu |last13=Shvartzvald |first13=Yossi |last14=Yee |first14=Jennifer C. |last15=Cha |first15=Sang-Mok |last16=Kim |first16=Dong-Jin |last17=Kim |first17=Hyoun-Woo |last18=Kim |first18=Seung-Lee |last19=Lee |first19=Chung-Uk |last20=Lee |first20=Dong-Joo |last21=Lee |first21=Yongseok |last22=Park |first22=Byeong-Gon |last23=Pogge |first23=Richard W. |last24=Mróz |first24=Przemek |last25=Szymański |first25=Michał K. |last26=Skowron |first26=Jan |last27=Poleski |first27=Radek |last28=Soszyński |first28=Igor |last29=Pietrukowicz |first29=Paweł |last30=Kozłowski |first30=Szymon |journal=Astronomy & Astrophysics |volume=664 |pages=A13 |doi=10.1051/0004-6361/202243744 |s2cid=248085003 |display-authors=1 }}

|0.20{{±|0.16|0.13}}

|

|

|1.68{{±|1.47|0.63}}

|

| style="background:#0099FF" |microlensing

|5100{{±|4100|1800}}

|0.16{{±|0.12|0.10}}

|

|

|0.95{{±|0.75|0.44}}

|

|

|3.63{{±|1.02|0.96}}

|

| style="background:#0099FF" |microlensing

|

|0.28{{±|0.22|0.13}}

|

|Multiple solutions for frojected separation

|11.2{{±|6.3|5.9}}

|

|

|6.21{{±|1.32|2.10}}

|

| style="background:#0099FF" |microlensing

|21000{{±|4000|7000}}

|0.62{{±|0.38|0.36}}

|

|Multiple solutions for frojected separation

|0.97{{±|1.78|0.56}}

|

|

|1.36{{±|0.20|0.17}}

|

| style="background:#0099FF" |microlensing

|26000{{±|4000|3000}}

|0.092{{±|0.170|0.053}}

|

|

|3.26{{±|0.83|0.58}}

|

|

|2.18{{±|0.58|0.72}}

|

| style="background:#0099FF" |microlensing

|19000{{±|2000}}

|0.42{{±|0.34|0.23}}

|

|Multiple solutions for planetary parameters{{citation|arxiv=2208.04230|year=2022|title=OGLE-2019-BLG-0362Lb: A SUPER-JOVIAN-MASS PLANET AROUND a LOW-MASS STAR|volume=55 |issue=4 |doi=10.5303/JKAS.2022.55.4.123 |last1=Chung |first1=Sun-Ju |last2=Yee |first2=Jennifer C. |last3=Udalski |first3=Andrej |last4=Gould |first4=Andrew |last5=Albrow |first5=Michael D. |last6=Jung |first6=Youn Kil |last7=Hwang |first7=Kyu-Ha |last8=Han |first8=Cheongho |last9=Ryu |first9=Yoon-Hyun |last10=Shin |first10=In-Gu |last11=Shvartzvald |first11=Yossi |last12=Zang |first12=Weicheng |last13=Cha |first13=Sang-Mok |last14=Kim |first14=Dong-Jin |last15=Kim |first15=Seung-Lee |last16=Lee |first16=Chung-Uk |last17=Lee |first17=Dong-Joo |last18=Lee |first18=Yongseok |last19=Park |first19=Byeong-Gon |last20=Pogge |first20=Richard W. |last21=Poleski |first21=Radek |last22=Mroz |first22=Przemek |last23=Pietrukowicz |first23=Pawel |last24=Skowron |first24=Jan |last25=Szymanski |first25=Michal K. |last26=Soszynski |first26=Igor |last27=Kozlowski |first27=Szymon |last28=Rybicki |first28=Krzysztof A. |last29=Iwanek |first29=Patryk |last30=Wrona |first30=Marcin |journal=Journal of the Korean Astronomical Society |page=123 |bibcode=2022JKAS...55..123C |s2cid=251402706 |display-authors=1 }}

|2.2{{±|1.8|1.3}}

|

|

|3.1{{±|1.2|1.1}}

|

| style="background:#0099FF" |microlensing

|20000{{±|4000}}

|0.55+0.17

|

|Circumbinary planet{{citation|arxiv=2204.05606|year=2022|title=OGLE-2019-BLG-1470LABc: Another microlensing giant planet in a binary system?|last1=Kuang |first1=Renkun |last2=Zang |first2=Weicheng |author3=Youn Kil Jung |last4=Udalski |first4=Andrzej |last5=Yang |first5=Hongjing |last6=Mao |first6=Shude |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Han |first10=Cheongho |last11=Hwang |first11=Kyu-Ha |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yee |first15=Jennifer C. |last16=Cha |first16=Sang-Mok |last17=Kim |first17=Dong-Jin |last18=Kim |first18=Hyoun-Woo |author19=Seung- Lee Kim |last20=Lee |first20=Chung-Uk |last21=Lee |first21=Dong-Joo |last22=Lee |first22=Yongseok |last23=Park |first23=Byeong-Gon |last24=Pogge |first24=Richard W. |last25=Mróz |first25=Przemek |last26=Skowron |first26=Jan |last27=Poleski |first27=Radoslaw |last28=Szymański |first28=Michał K. |last29=Soszyński |first29=Igor |last30=Pietrukowicz |first30=Paweł |journal=Monthly Notices of the Royal Astronomical Society |volume=516 |issue=2 |pages=1704–1720 |doi=10.1093/mnras/stac2315 |doi-access=free |display-authors=1 }}

|0.0421{{±|0.0042}}

|

|124.64{{±|0.48|0.52}}

|

|

| style="background:#00FF00" |radial vel.

|59.62{{±|0.07}}

|1.11{{±|0.01}}

|6013{{±|18}}

|{{citation|arxiv=2203.01018|year=2022|title=A Radial Velocity Study of the Planetary System of π Mensae: Improved Planet Parameters for π Mensae c and a Third Planet on a 125 Day Orbit|doi=10.3847/1538-3881/ac5dcb |last1=Hatzes |first1=Artie P. |last2=Gandolfi |first2=Davide |last3=Korth |first3=Judith |last4=Rodler |first4=Florian |last5=Sabotta |first5=Silvia |last6=Esposito |first6=Massimiliano |last7=Barragán |first7=Oscar |last8=Van Eylen |first8=Vincent |last9=Livingston |first9=John H. |last10=Serrano |first10=Luisa Maria |last11=Luque |first11=Rafael |last12=Smith |first12=Alexis M. S. |last13=Redfield |first13=Seth |last14=Persson |first14=Carina M. |last15=Pätzold |first15=Martin |last16=Palle |first16=Enric |last17=Nowak |first17=Grzegorz |last18=Osborne |first18=Hannah L. M. |last19=Narita |first19=Norio |last20=Mathur |first20=Savita |last21=Lam |first21=Kristine W. F. |last22=Kabáth |first22=Petr |last23=Johnson |first23=Marshall C. |last24=Guenther |first24=Eike W. |last25=Grziwa |first25=Sascha |last26=Goffo |first26=Elisa |last27=Fridlund |first27=Malcolm |last28=Endl |first28=Michael |last29=Deeg |first29=Hans J. |last30=Csizmadia |first30=Szilard |journal=The Astronomical Journal |volume=163 |issue=5 |page=223 |bibcode=2022AJ....163..223H |s2cid=247218413 |display-authors=1 |doi-access=free }}

|0.0008{{±|0.0002}}

|

|5.122{{±|0.002|0.0036}}

|0.02885{{±|0.00019|0.00022}}

|360

| style="background:#00FF00" |radial vel.

|4.2465{{±|0.0003}}

|0.1221{{±|0.0022}}

|2900{{±|100}}

|{{citation|arxiv=2202.05188|year=2022|title=A candidate short-period sub-Earth orbiting Proxima Centauri|doi=10.1051/0004-6361/202142337 |last1=Faria |first1=J. P. |last2=Suárez Mascareño |first2=A. |last3=Figueira |first3=P. |last4=Silva |first4=A. M. |last5=Damasso |first5=M. |last6=Demangeon |first6=O. |last7=Pepe |first7=F. |last8=Santos |first8=N. C. |last9=Rebolo |first9=R. |last10=Cristiani |first10=S. |last11=Adibekyan |first11=V. |last12=Alibert |first12=Y. |last13=Allart |first13=R. |last14=Barros |first14=S. C. C. |last15=Cabral |first15=A. |last16=d'Odorico |first16=V. |last17=Di Marcantonio |first17=P. |last18=Dumusque |first18=X. |last19=Ehrenreich |first19=D. |last20=González Hernández |first20=J. I. |last21=Hara |first21=N. |last22=Lillo-Box |first22=J. |last23=Lo Curto |first23=G. |last24=Lovis |first24=C. |last25=Martins |first25=C. J. A. P. |last26=Mégevand |first26=D. |last27=Mehner |first27=A. |last28=Micela |first28=G. |last29=Molaro |first29=P. |last30=Nunes |first30=N. J. |journal=Astronomy & Astrophysics |volume=658 |pages=A115 |bibcode=2022A&A...658A.115F |s2cid=246706321 |display-authors=1 }}

|0.0072{{±|0.0009}}

|

|723{{±|8}}

|

|

| style="background:#FF7519" |timing

|22000

|

|

|Pulsar planet, another planet in the system is suspected.{{citation|arxiv=2203.01136|year=2022|title=A search for planetary companions around 800 pulsars from the Jodrell Bank pulsar timing programme|doi=10.1093/mnras/stac593 |last1=Niţu |first1=Iuliana C. |last2=Keith |first2=Michael J. |last3=Stappers |first3=Ben W. |last4=Lyne |first4=Andrew G. |last5=Mickaliger |first5=Mitchell B. |journal=Monthly Notices of the Royal Astronomical Society |volume=512 |issue=2 |pages=2446–2459 |doi-access=free }}

|0.0126{{±|0.0019}}

|

|10.76{{±|0.01|0.02}}

|0.05353{{±|0.00047|0.00051}}

|

| style="background:#00FF00" |radial vel.

|36.594{{±|0.011}}

|0.1774{{±|0.0045}}

|3071{{±|34|22}}

|Host star also known as Gliese 585, planet close to habitable zone.{{citation|arxiv=2205.11986|year=2022|title=A super-Earth orbiting near the inner edge of the habitable zone around the M4.5 dwarf Ross 508|last1=Harakawa |first1=Hiroki |last2=Takarada |first2=Takuya |last3=Kasagi |first3=Yui |last4=Hirano |first4=Teruyuki |last5=Kotani |first5=Takayuki |last6=Kuzuhara |first6=Masayuki |last7=Omiya |first7=Masashi |last8=Kawahara |first8=Hajime |last9=Fukui |first9=Akihiko |last10=Hori |first10=Yasunori |author11=Hiroyuki Tako Ishikawa |last12=Ogihara |first12=Masahiro |last13=Livingston |first13=John |last14=Brandt |first14=Timothy D. |last15=Currie |first15=Thayne |last16=Aoki |first16=Wako |last17=Beichman |first17=Charles A. |last18=Henning |first18=Thomas |last19=Hodapp |first19=Klaus |last20=Ishizuka |first20=Masato |last21=Izumiura |first21=Hideyuki |last22=Jacobson |first22=Shane |last23=Janson |first23=Markus |last24=Kambe |first24=Eiji |last25=Kodama |first25=Takanori |last26=Kokubo |first26=Eiichiro |last27=Konishi |first27=Mihoko |last28=Krishnamurthy |first28=Vigneshwaran |last29=Kudo |first29=Tomoyuki |last30=Kurokawa |first30=Takashi |journal=Publications of the Astronomical Society of Japan |volume=74 |issue=4 |pages=904–922 |doi=10.1093/pasj/psac044 |display-authors=1 }}

|0.127891{{±|0.013510|0.025081}}

|0.631521{{±|0.007554|0.009811}}

|4.532058{{±|0.000002|0.000002}}

|0.055780{{±|0.005563|0.003893}}

|878{{±|32|41}}

| style="background:#FFFF00" |transit

|314{{±|2}}

|0.781{{±|0.042}}

|4994{{±|50}}

|{{citation|arxiv=2211.07957|year=2023|title=VaTEST I: Validation of sub-Saturn exoplanet TOI-181b in narrow orbit from its host star|last1=Mistry |first1=Priyashkumar |last2=Pathak |first2=Kamlesh |last3=Lekkas |first3=Georgios |last4=Prasad |first4=Aniket |last5=Bhattarai |first5=Surendra |last6=Maity |first6=Mousam |last7=Beichman |first7=Charles A. |last8=Ciardi |first8=David R. |last9=Evans |first9=Phil |last10=Lucero |first10=Jennifer P. |journal=Monthly Notices of the Royal Astronomical Society |volume=521 |pages=1066–1078 |doi=10.1093/mnras/stad543 |doi-access=free }}

|

|0.116{{±|0.004}}

|0.7363104{{±|0.0000003}}

|0.0112{{±|0.0001}}

|910{{±|36}}

| style="background:#FFFF00" |transit

|155.9

|0.35{{±|0.01}}

|3383{{±|157}}

|{{citation|arxiv=2201.12661|year=2022|title=Validation of 13 Hot and Potentially Terrestrial TESS Planets|doi=10.3847/1538-3881/ac4334 |last1=Giacalone |first1=Steven |last2=Dressing |first2=Courtney D. |last3=Hedges |first3=Christina |last4=Kostov |first4=Veselin B. |last5=Collins |first5=Karen A. |last6=Jensen |first6=Eric L. N. |last7=Yahalomi |first7=Daniel A. |last8=Bieryla |first8=Allyson |last9=Ciardi |first9=David R. |last10=Howell |first10=Steve B. |last11=Lillo-Box |first11=Jorge |last12=Barkaoui |first12=Khalid |last13=Winters |first13=Jennifer G. |last14=Matthews |first14=Elisabeth |last15=Livingston |first15=John H. |last16=Quinn |first16=Samuel N. |last17=Safonov |first17=Boris S. |last18=Cadieux |first18=Charles |last19=Furlan |first19=E. |last20=Crossfield |first20=Ian J. M. |last21=Mandell |first21=Avi M. |last22=Gilbert |first22=Emily A. |last23=Kruse |first23=Ethan |last24=Quintana |first24=Elisa V. |last25=Ricker |first25=George R. |last26=Seager |first26=S. |last27=Winn |first27=Joshua N. |last28=Jenkins |first28=Jon M. |last29=Duffy Adkins |first29=Britt |last30=Baker |first30=David |journal=The Astronomical Journal |volume=163 |issue=2 |page=99 |bibcode=2022AJ....163...99G |s2cid=246386453 |display-authors=1 |doi-access=free }}

|0.0239{{±|0.0179|0.0098}}

|0.237{{±|0.016}}

|3.9940{{±|0.0004}}

|0.0269{{±|0.0011}}

|

| style="background:#FFFF00" |transit

|212.6{{±|0.6|0.3}}

|0.16{{±|0.01}}

|4031{{±|21|23}}

|{{citation|arxiv=2211.08490|year=2022|title=A systematic validation of hot Neptunes in TESS data|last1=Magliano |first1=Christian |last2=Covone |first2=Giovanni |last3=Dobal |first3=Richa |last4=Cacciapuoti |first4=Luca |last5=Tonietti |first5=Luca |last6=Giacalone |first6=Steven |last7=Vines |first7=Jose I. |last8=Inno |first8=Laura |last9=Jenkins |first9=James S. |last10=Lissauer |first10=Jack J. |last11=Bieryla |first11=Allyson |last12=Oliva |first12=Fabrizio |last13=Pagano |first13=Isabella |last14=Kostov |first14=Veselin |last15=Ziegler |first15=Carl |last16=Ciardi |first16=David R. |last17=Gonzales |first17=Erica J. |last18=Dressing |first18=Courtney D. |last19=Buchhave |first19=Lars A. |last20=Howell |first20=Steve B. |last21=Matson |first21=Rachel A. |last22=Matthews |first22=Elisabeth |last23=Rotundi |first23=Alessandra |last24=Alves |first24=Douglas |last25=Fiscale |first25=Stefano |last26=Ienco |first26=Riccardo M. |last27=Pena |first27=Pablo |last28=Gallo |first28=Francesco |last29=Muscari Tomajoli |first29=Maria T. |journal=Monthly Notices of the Royal Astronomical Society |volume=519 |pages=1562–1577 |doi=10.1093/mnras/stac3404 |doi-access=free }}

|

|0.104{{±|0.010}}

|0.5481579{{±|0.0000006}}

|0.0128{{±|0.0011}}

|1693{{±|105}}

| style="background:#FFFF00" |transit

|154.8

|0.88{{±|0.25}}

|4621{{±|50}}

|

|

|0.181{{±|0.009}}

|1.5483510{{±|0.0000015}}

|0.0251 ± 0.0019

|1082{{±|47}}

| style="background:#FFFF00" |transit

|132.7

|0.85{{±|0.20}}

|4369{{±|100}}

|

|

|

|5.0988179{{±|0.0000045|0.0000046}}

|0.04825{{±|0.00065|0.00066}}

|603.6{{±|5.5|5.3}}

| style="background:#FFFF00" |transit

|107.81{{±|0.19}}

|0.577{{±|0.024|0.023}}

|3708{{±|57|56}}

|{{citation|arxiv=2204.03108|year=2022|title=A Close-in Puffy Neptune with Hidden Friends: The Enigma of TOI 620|doi=10.3847/1538-3881/ac658b |last1=Reefe |first1=Michael A. |last2=Luque |first2=Rafael |last3=Gaidos |first3=Eric |last4=Beard |first4=Corey |last5=Plavchan |first5=Peter P. |last6=Cointepas |first6=Marion |last7=Cale |first7=Bryson L. |last8=Palle |first8=Enric |last9=Parviainen |first9=Hannu |last10=Feliz |first10=Dax L. |last11=Eastman |first11=Jason |last12=Stassun |first12=Keivan |last13=Gagné |first13=Jonathan |last14=Jenkins |first14=Jon M. |last15=Boyd |first15=Patricia T. |last16=Kidwell |first16=Richard C. |last17=McDermott |first17=Scott |last18=Collins |first18=Karen A. |last19=Fong |first19=William |last20=Guerrero |first20=Natalia |last21=Almenara-Villa |first21=Jose-Manuel |last22=Bean |first22=Jacob |last23=Beichman |first23=Charles A. |last24=Berberian |first24=John |last25=Bieryla |first25=Allyson |last26=Bonfils |first26=Xavier |last27=Bouchy |first27=François |last28=Brady |first28=Madison |last29=Bryant |first29=Edward M. |last30=Cacciapuoti |first30=Luca |journal=The Astronomical Journal |volume=163 |issue=6 |page=269 |bibcode=2022AJ....163..269R |s2cid=248006000 |display-authors=1 |doi-access=free }}

|2.76{{±|0.24}}

|1.375{{±|0.045}}

|4.633611{{±|0.000001}}

|0.060{{±|0.003}}

|1561{{±|33|32}}

| style="background:#FFFF00" |transit

|530{{±|4}}

|1.428{{±|0.094}}

|6715{{±|128}}

|{{citation|arxiv=2212.08242|year=2023|title=Spinning up a Daze: TESS Uncovers a Hot Jupiter Orbiting the Rapid Rotator TOI-778|last1=Clark |first1=Jake |last2=Addison |first2=Brett |last3=Okumura |first3=Jack |last4=Vach |first4=Sydney |last5=Heitzmann |first5=Alexis |last6=Rodriguez |first6=Joseph |last7=Wright |first7=Duncan |last8=Clerte |first8=Mathieu |last9=Brown |first9=Carolyn |last10=Fetherolf |first10=Tara |last11=Wittenmyer |first11=Robert |last12=Plavchan |first12=Peter |last13=Kane |first13=Stephen |last14=Horner |first14=Jonathan |last15=Kielkopf |first15=John |last16=Shporer |first16=Avi |last17=Tinney |first17=C. |last18=Hui-Gen |first18=Liu |last19=Ballard |first19=Sarah |last20=Bowler |first20=Brendan |last21=Mengel |first21=Matthew |last22=Zhou |first22=George |last23=Lee |first23=Annette |last24=David |first24=Avelyn |last25=Heim |first25=Jessica |last26=Lee |first26=Michele |last27=Sevilla |first27=Veronica |last28=Zafar |first28=Naqsh |last29=Hinkel |first29=Natalie |last30=Allen |first30=Bridgette |journal=The Astronomical Journal |volume=165 |issue=5 |page=207 |doi=10.3847/1538-3881/acc3a0 |bibcode=2023AJ....165..207C |s2cid=254823145 |display-authors=1 |doi-access=free }}

|

|0.113{{±|0.006}}

|1.0418777{{±|0.0000324}}

|0.0171{{±|0.0003}}

|1118{{±|49}}

| style="background:#FFFF00" |transit

|136.3

|0.61{{±|0.03}}

|3920{{±|160}}

|

|0.0286{{±|0.0031}}

|0.247{{±|0.033}}

|1.8237305{{±|0.0000020|0.0000021}}

|0.02636{{±|0.00017}}

|941{{±|31}}

| style="background:#FFFF00" |transit

|253.8{{±|0.5}}

|0.730{{±|0.037}}

|4550{{±|75}}

|{{citation|arxiv=2210.08996|year=2023|title=TOI-969: A late-K dwarf with a hot mini-Neptune in the desert and an eccentric cold Jupiter|last1=Lillo-Box |first1=J. |last2=Gandolfi |first2=D. |last3=Armstrong |first3=D. J. |last4=Collins |first4=K. A. |last5=Nielsen |first5=L. D. |last6=Luque |first6=R. |last7=Korth |first7=J. |last8=Sousa |first8=S. G. |last9=Quinn |first9=S. N. |last10=Acuña |first10=L. |last11=Howell |first11=S. B. |last12=Morello |first12=G. |last13=Hellier |first13=C. |last14=Giacalone |first14=S. |last15=Hoyer |first15=S. |last16=Stassun |first16=K. |last17=Palle |first17=E. |last18=Aguichine |first18=A. |last19=Mousis |first19=O. |last20=Adibekyan |first20=V. |last21=Azevedo Silva |first21=T. |last22=Barrado |first22=D. |last23=Deleuil |first23=M. |last24=Eastman |first24=J. D. |last25=Hawthorn |first25=F. |last26=Irwin |first26=J. M. |last27=Jenkins |first27=J. M. |last28=Latham |first28=D. W. |last29=Muresan |first29=A. |last30=Persson |first30=C. M. |journal=Astronomy & Astrophysics |volume=669 |pages=A109 |doi=10.1051/0004-6361/202243879 |bibcode=2023A&A...669A.109L |s2cid=252917906 |display-authors=1 }}

|11.3{{±|1.1|0.9}}

|

|1700{{±|290|280}}

|2.52{{±|0.27|0.29}}

|96.4{{±|6.8|5.8}}

| style="background:#00FF00" |radial vel.

|253.8{{±|0.5}}

|0.730{{±|0.037}}

|4550{{±|75}}

|Eccentric orbit

|0.0425{{±|0.0055}}

|0.231{{±|0.004}}

|6.443868{{±|0.000025}}

|0.06152{{±|0.00086|0.00089}}

|784{{±|13}}

| style="background:#FFFF00" |transit

|224.5{{±|0.2}}

|0.748{{±|0.032}}

|4734{{±|67}}

|{{citation|arxiv=2201.03570|year=2022|title=A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS|doi=10.1093/mnras/stab3799 |last1=Wilson |first1=Thomas G. |last2=Goffo |first2=Elisa |last3=Alibert |first3=Yann |last4=Gandolfi |first4=Davide |last5=Bonfanti |first5=Andrea |last6=Persson |first6=Carina M. |last7=Collier Cameron |first7=Andrew |last8=Fridlund |first8=Malcolm |last9=Fossati |first9=Luca |last10=Korth |first10=Judith |last11=Benz |first11=Willy |last12=Deline |first12=Adrien |last13=Florén |first13=Hans-Gustav |last14=Guterman |first14=Pascal |last15=Adibekyan |first15=Vardan |last16=Hooton |first16=Matthew J. |last17=Hoyer |first17=Sergio |last18=Leleu |first18=Adrien |last19=Mustill |first19=Alexander James |last20=Salmon |first20=Sébastien |last21=Sousa |first21=Sérgio G. |last22=Suarez |first22=Olga |last23=Abe |first23=Lyu |last24=Agabi |first24=Abdelkrim |last25=Alonso |first25=Roi |last26=Anglada |first26=Guillem |last27=Asquier |first27=Joel |last28=Bárczy |first28=Tamas |last29=Barrado Navascues |first29=David |last30=Barros |first30=Susana C C. |journal=Monthly Notices of the Royal Astronomical Society |volume=511 |pages=1043–1071 |doi-access=free |display-authors=1 }}

|0.0079{{±|0.0057|0.0063}}

|0.237{{±|0.004}}

|12.226574{{±|0.000046|0.000043}}

|0.09429{{±|0.00132|0.00136}}

|634{{±|10}}

| style="background:#FFFF00" |transit

|224.5{{±|0.2}}

|0.748{{±|0.032}}

|4734{{±|67}}

|

|

|0.154{{±|0.007}}

|0.6047328{{±|0.0000032}}

|0.0118{{±|0.0001}}

|1336{{±|56}}

| style="background:#FFFF00" |transit

|200.9

|0.60{{±|0.02}}

|3921{{±|157}}

|

|0.0313{{±|0.0042}}

|0.160{{±|0.010|0.007}}

|0.6047328{{±|0.0000032}}

|0.01159{{±|0.00023|0.00020}}

|1323{{±|44}}

| style="background:#FFFF00" |transit

|200.4{{±|0.6|2.2}}

|0.604{{±|0.030}}

|3875{{±|75}}

|{{citation|arxiv=2210.14901|year=2023|title=TOI-1075 b: A Dense, Massive, Ultra-short-period Hot Super-Earth Straddling the Radius Gap|last1=Essack |first1=Zahra |last2=Shporer |first2=Avi |last3=Burt |first3=Jennifer A. |last4=Seager |first4=Sara |last5=Cambioni |first5=Saverio |last6=Lin |first6=Zifan |last7=Collins |first7=Karen A. |last8=Mamajek |first8=Eric E. |last9=Stassun |first9=Keivan G. |last10=Ricker |first10=George R. |last11=Vanderspek |first11=Roland |last12=Latham |first12=David W. |last13=Winn |first13=Joshua N. |last14=Jenkins |first14=Jon M. |last15=Paul Butler |first15=R. |last16=Charbonneau |first16=David |last17=Collins |first17=Kevin I. |last18=Crane |first18=Jeffrey D. |last19=Gan |first19=Tianjun |last20=Hellier |first20=Coel |last21=Howell |first21=Steve B. |last22=Irwin |first22=Jonathan |last23=Mann |first23=Andrew W. |last24=Ramadhan |first24=Ali |last25=Shectman |first25=Stephen A. |last26=Teske |first26=Johanna K. |last27=Yee |first27=Samuel W. |last28=Mireles |first28=Ismael |last29=Quintana |first29=Elisa V. |last30=Tenenbaum |first30=Peter |journal=The Astronomical Journal |volume=165 |issue=2 |page=47 |doi=10.3847/1538-3881/ac9c5b |bibcode=2023AJ....165...47E |s2cid=253117166 |display-authors=1 |doi-access=free }}

|3.35{{±|0.18}}

|1.30{{±|0.05}}

|4.0782387{{±|0.0000024|0.0000025}}

|0.0561{{±|0.0024|0.0025}}

|1728{{±|27}}

| style="background:#FFFF00" |transit

|925{{±|7}}

|1.35{{±|0.08}}

|6311{{±|98}}

|{{citation|arxiv=2205.10854|year=2022|title=Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type stars|doi=10.1051/0004-6361/202243454 |last1=Psaridi |first1=A. |last2=Bouchy |first2=F. |last3=Lendl |first3=M. |last4=Grieves |first4=N. |last5=Stassun |first5=K.G. |last6=Carmichael |first6=T. |last7=S |first7=Gill |last8=A |first8=Peña Rojas P. |last9=T |first9=Gan |last10=A |first10=Shporer |last11=A |first11=Bieryla |last12=L |first12=Christiansen J. |last13=M |first13=Crossfield I. J. |last14=M |first14=Galland F. Hooton M. J. Jenkins J. |last15=S |first15=Jenkins J. |last16=W |first16=Latham D. |last17=B |first17=Lund M. |last18=E |first18=Rodriguez J. |last19=B |first19=Ting E. |last20=A |first20=Udry S. Ulmer-Moll S. Wittenmyer R. |author21=Yanzhe Zhang Y |last22=G |first22=Zhou |last23=B |first23=Addison |last24=M |first24=Cointepas |last25=A |first25=Collins K. |last26=I |first26=Collins K. |last27=A |first27=Deline |last28=D |first28=Dressing C. |last29=P |first29=Evans |last30=S |first30=Giacalone |display-authors=1 |journal=Astronomy & Astrophysics |volume=664 |pages=A94 |bibcode=2022A&A...664A..94P |s2cid=248872705 }}

|0.0095{{±|0.0022|0.0028}}

|0.170{{±|0.019|0.013}}

|4.1728{{±|0.0002}}

|

|

| style="background:#FFFF00" |transit

|275.8{{±|0.5}}

|1.022{{±|0.027}}

|5770{{±|50}}

|{{citation|arxiv=2210.09283|year=2023|title=TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain|last1=Dai |first1=Fei |last2=Masuda |first2=Kento |last3=Beard |first3=Corey |last4=Robertson |first4=Paul |last5=Goldberg |first5=Max |last6=Batygin |first6=Konstantin |last7=Bouma |first7=Luke |last8=Lissauer |first8=Jack J. |last9=Knudstrup |first9=Emil |last10=Albrecht |first10=Simon |last11=Howard |first11=Andrew W. |last12=Knutson |first12=Heather A. |last13=Petigura |first13=Erik A. |last14=Weiss |first14=Lauren M. |last15=Isaacson |first15=Howard |author16=Martti Holst Kristiansen |last17=Osborn |first17=Hugh |last18=Wang |first18=Songhu |last19=Wang |first19=Xian-Yu |last20=Behmard |first20=Aida |last21=Greklek-McKeon |first21=Michael |last22=Vissapragada |first22=Shreyas |last23=Batalha |first23=Natalie M. |last24=Brinkman |first24=Casey L. |last25=Chontos |first25=Ashley |last26=Crossfield |first26=Ian |last27=Dressing |first27=Courtney |last28=Fetherolf |first28=Tara |last29=Fulton |first29=Benjamin |last30=Hill |first30=Michelle L. |journal=The Astronomical Journal |volume=165 |issue=2 |page=33 |doi=10.3847/1538-3881/aca327 |bibcode=2023AJ....165...33D |s2cid=252918416 |display-authors=1 |doi-access=free }}

|0.0189{{±|0.0041|0.0053}}

|0.257{{±|0.005}}

|6.2573{{±|0.0002}}

|

|

| style="background:#FFFF00" |transit

|275.8{{±|0.5}}

|1.022{{±|0.027}}

|5770{{±|50}}

|

|0.0252{{±|0.0076|0.0060}}

|0.413{{±|0.007}}

|12.5194{{±|0.0004}}

|

|

| style="background:#FFFF00" |transit

|275.8{{±|0.5}}

|1.022{{±|0.027}}

|5770{{±|50}}

|

|0.0170{{±|0.0031}}

|0.236{{±|0.006|0.008}}

|18.7992{{±|0.0017|0.0015}}

|

|

| style="background:#FFFF00" |transit

|275.8{{±|0.5}}

|1.022{{±|0.027}}

|5770{{±|50}}

|

|0.0261{{±|0.0088|0.0113}}

|0.346{{±|0.010}}

|26.3162{{±|0.0017|0.0013}}

|

|

| style="background:#FFFF00" |transit

|275.8{{±|0.5}}

|1.022{{±|0.027}}

|5770{{±|50}}

|

|0.0151{{±|0.0148|0.0104}}

|0.226{{±|0.010}}

|39.5387{{±|0.0036|0.0030}}

|

|

| style="background:#FFFF00" |transit

|275.8{{±|0.5}}

|1.022{{±|0.027}}

|5770{{±|50}}

|

|1.18{{±|0.14}}

|1.30{{±|0.08}}

|2.103195{{±|0.000012|0.000011}}

|

|2162

| style="background:#FFFF00" |transit

|1013{{±|3}}

|1.38{{±|0.086|0.082}}

|6260{{±|100}}

|Subgiant host star{{citation|arxiv=2205.01860|year=2022|title=TOI-2046b, TOI-1181b and TOI-1516b, three new hot Jupiters from TESS: Planets orbiting a young star, a subgiant and a normal star|last1=Kabáth |first1=Petr |last2=Chaturvedi |first2=Priyanka |last3=MacQueen |first3=Phillip J. |last4=Skarka |first4=Marek |last5=Šubjak |first5=Ján |last6=Esposito |first6=Massimilliano |last7=Cochran |first7=William D. |last8=Bellomo |first8=Salvatore E. |last9=Karjalainen |first9=Raine |last10=Guenther |first10=Eike W. |last11=Endl |first11=Michael |last12=Csizmadia |first12=Szilárd |last13=Karjalainen |first13=Marie |last14=Hatzes |first14=Artie |last15=Žák |first15=Jiří |last16=Gandolfi |first16=Davide |last17=Boffin |first17=Henri M. J. |last18=Vines |first18=Jose I. |last19=Livingston |first19=John H. |last20=García |first20=Rafael A. |last21=Mathur |first21=Savita |last22=González-Cuesta |first22=Lucía |last23=Blažek |first23=Martin |last24=Caldwell |first24=Douglas A. |last25=Colón |first25=Knicole D. |last26=Deeg |first26=Hans |last27=Erikson |first27=Anders |author28=Vincent Van Eylen |last29=Fong |first29=William |last30=Fridlund |first30=Malcolm |journal=Monthly Notices of the Royal Astronomical Society |volume=513 |issue=4 |pages=5955–5972 |doi=10.1093/mnras/stac1254 |doi-access=free |display-authors=1 }}

|

|0.259{{±|0.011}}

|91.68278{{±|0.00032|0.00041}}

|0.404{{±|0.026|0.023}}

|400

| style="background:#FFFF00" |transit

|447.1{{±|0.7}}

|1.03{{±|0.06}}

|5592{{±|50}}

|{{citation|arxiv=2209.13651|year=2023|title=Validation of TOI-1221 b: A Warm Sub-Neptune Exhibiting Transit Timing Variations around a Sun-like Star|last1=Mann |first1=Christopher R. |last2=Lafrenière |first2=David |last3=Dragomir |first3=Diana |last4=Quinn |first4=Samuel N. |last5=Tan |first5=Thiam-Guan |last6=Collins |first6=Karen A. |last7=Howell |first7=Steve B. |last8=Ziegler |first8=Carl |last9=Mann |first9=Andrew W. |last10=Stassun |first10=Keivan G. |last11=Kristiansen |first11=Martti H. |last12=Osborn |first12=Hugh |last13=Boyajian |first13=Tabetha |last14=Eisner |first14=Nora |last15=Hellier |first15=Coel |last16=Ricker |first16=George R. |last17=Vanderspek |first17=Roland |last18=Latham |first18=David W. |last19=Seager |first19=S. |last20=Winn |first20=Joshua N. |last21=Jenkins |first21=Jon M. |last22=McLean |first22=Brian |last23=Rowden |first23=Pamela |last24=Torres |first24=Guillermo |last25=Caldwell |first25=Douglas A. |last26=Collins |first26=Kevin I. |last27=Schwarz |first27=Richard P. |journal=The Astronomical Journal |volume=165 |issue=5 |page=217 |doi=10.3847/1538-3881/acc8d4 |bibcode=2023AJ....165..217M |s2cid=252568279 |doi-access=free }}

|0.0255{{±|0.0035}}

|0.269{{±|0.005}}

|4.30744{{±|0.00002}}

|0.049{{±|0.002}}

|955

| style="background:#FFFF00" |transit

|557.9{{±|1.0}}

|1.12{{±|0.16}}

|5217{{±|50}}

|{{citation|arxiv=2204.11895|year=2022|title=The TESS-Keck Survey. XI. Mass Measurements for Four Transiting Sub-Neptunes Orbiting K Dwarf TOI–1246|last1=Turtelboom |first1=Emma V. |last2=Weiss |first2=Lauren M. |last3=Dressing |first3=Courtney D. |last4=Nowak |first4=Grzegorz |last5=Pallé |first5=Enric |last6=Beard |first6=Corey |last7=Blunt |first7=Sarah |last8=Brinkman |first8=Casey |last9=Chontos |first9=Ashley |last10=Claytor |first10=Zachary R. |last11=Dai |first11=Fei |last12=Dalba |first12=Paul A. |last13=Giacalone |first13=Steven |last14=Gonzales |first14=Erica |last15=Harada |first15=Caleb K. |last16=Hill |first16=Michelle L. |last17=Holcomb |first17=Rae |last18=Korth |first18=Judith |last19=Lubin |first19=Jack |last20=Masseron |first20=Thomas |last21=MacDougall |first21=Mason |last22=Mayo |first22=Andrew W. |last23=Močnik |first23=Teo |last24=Akana Murphy |first24=Joseph M. |last25=Polanski |first25=Alex S. |last26=Rice |first26=Malena |last27=Rubenzahl |first27=Ryan A. |last28=Scarsdale |first28=Nicholas |last29=Stassun |first29=Keivan G. |last30=Tyler |first30=Dakotah B. |journal=The Astronomical Journal |volume=163 |issue=6 |page=293 |doi=10.3847/1538-3881/ac69e5 |bibcode=2022AJ....163..293T |s2cid=248392257 |display-authors=1 |doi-access=free }}

|0.0277{{±|0.0038}}

|0.224{{±|0.007}}

|5.904144{{±|0.000083}}

|0.061{{±|0.002}}

|860

| style="background:#FFFF00" |transit

|557.9{{±|1.0}}

|1.12{{±|0.16}}

|5217{{±|50}}

|

|0.0167{{±|0.0053}}

|0.313{{±|0.008}}

|18.65590{{±|0.00048}}

|0.131{{±|0.004}}

|586

| style="background:#FFFF00" |transit

|557.9{{±|1.0}}

|1.12{{±|0.16}}

|5217{{±|50}}

|

|0.0466{{±|0.0072}}

|0.338{{±|0.014}}

|37.9216{{±|0.0010}}

|0.211{{±|0.007}}

|462

| style="background:#FFFF00" |transit

|557.9{{±|1.0}}

|1.12{{±|0.16}}

|5217{{±|50}}

|

|0.0373{{±|0.0245}}

|0.276{{±|0.008}}

|16.608164{{±|0.000083}}

|0.1116{{±|0.0033}}

|499{{±|4}}

| style="background:#FFFF00" |transit

|239.5{{±|0.3}}

|0.66{{±|0.01}}

|4227{{±|85}}

|{{citation|arxiv=2212.04307|year=2022|title=Discovery of TOI-1260d and the characterisation of the multi-planet system|doi=10.1093/mnras/stac3639 |last1=Lam |first1=Kristine W F. |last2=Cabrera |first2=J. |last3=Hooton |first3=M. J. |last4=Alibert |first4=Y. |last5=Bonfanti |first5=A. |last6=Beck |first6=M. |last7=Deline |first7=A. |last8=Florén |first8=H-G |last9=Simon |first9=A. E. |last10=Fossati |first10=L. |last11=Persson |first11=C. M. |last12=Fridlund |first12=M. |last13=Salmon |first13=S. |last14=Hoyer |first14=S. |last15=Osborn |first15=H. P. |last16=Wilson |first16=T. G. |last17=Georgieva |first17=I. Y. |last18=Nowak |first18=Gr |last19=Luque |first19=R. |last20=Egger |first20=J. A. |last21=Abidekyan |first21=V. |last22=Alonso |first22=R. |last23=Escudé |first23=G Anglada |last24=Bárczy |first24=T. |last25=Barrado |first25=D. |last26=Barros |first26=S C C. |last27=Baumjohann |first27=W. |last28=Beck |first28=T. |last29=Bekkelien |first29=A. |last30=Benz |first30=W. |journal=Monthly Notices of the Royal Astronomical Society |volume=519 |pages=1437–1451 |doi-access=free |display-authors=1 }}

|0.303{{±|0.026}}

|0.81{{±|0.05}}

|8.1577080{{±|0.0000044}}

|0.072{{±|0.009|0.010}}

|919

| style="background:#FFFF00" |transit

|359.1{{±|0.4}}

|0.92{{±|0.03}}

|5290{{±|117}}

|{{citation|arxiv=2201.13341|year=2022|title=TOI-1268b: The youngest hot Saturn-mass transiting exoplanet|last1=Šubjak |first1=J. |last2=Endl |first2=M. |last3=Chaturvedi |first3=P. |last4=Karjalainen |first4=R. |last5=Cochran |first5=W. D. |last6=Esposito |first6=M. |last7=Gandolfi |first7=D. |last8=Lam |first8=K. W. F. |last9=Stassun |first9=K. |last10=Žák |first10=J. |last11=Lodieu |first11=N. |last12=Boffin |first12=H. M. J. |last13=MacQueen |first13=P. J. |last14=Hatzes |first14=A. |last15=Guenther |first15=E. W. |last16=Georgieva |first16=I. |last17=Grziwa |first17=S. |last18=Schmerling |first18=H. |last19=Skarka |first19=M. |last20=Blažek |first20=M. |last21=Karjalainen |first21=M. |last22=Špoková |first22=M. |last23=Isaacson |first23=H. |last24=Howard |first24=A. W. |last25=Burke |first25=C. J. |last26=Van Eylen |first26=V. |last27=Falk |first27=B. |last28=Fridlund |first28=M. |last29=Goffo |first29=E. |last30=Jenkins |first30=J. M. |journal=Astronomy & Astrophysics |volume=662 |pages=A107 |doi=10.1051/0004-6361/202142883 |bibcode=2022A&A...662A.107S |s2cid=246430777 |display-authors=1 }}

|0.0774{{±|0.0072}}

|0.370{{±|0.019}}

|3.31599{{±|0.00002}}

|0.0412{{±|0.0008}}

|961{{±|32}}

| style="background:#FFFF00" |transit

|450.6{{±|1.3}}

|0.851{{±|0.049}}

|4985{{±|121}}

|{{citation|arxiv=2206.14327|year=2022|title=The TESS–Keck Survey. XIII. An Eccentric Hot Neptune with a Similar-mass Outer Companion around TOI-1272|doi=10.3847/1538-3881/ac7ce1 |last1=MacDougall |first1=Mason G. |last2=Petigura |first2=Erik A. |last3=Fetherolf |first3=Tara |last4=Beard |first4=Corey |last5=Lubin |first5=Jack |last6=Angelo |first6=Isabel |last7=Batalha |first7=Natalie M. |last8=Behmard |first8=Aida |last9=Blunt |first9=Sarah |last10=Brinkman |first10=Casey |last11=Chontos |first11=Ashley |last12=Crossfield |first12=Ian J. M. |last13=Dai |first13=Fei |last14=Dalba |first14=Paul A. |last15=Dressing |first15=Courtney |last16=Fulton |first16=Benjamin |last17=Giacalone |first17=Steven |last18=Hill |first18=Michelle L. |last19=Howard |first19=Andrew W. |last20=Huber |first20=Daniel |last21=Isaacson |first21=Howard |last22=Kane |first22=Stephen R. |last23=Kosiarek |first23=Molly |last24=Mayo |first24=Andrew |last25=Močnik |first25=Teo |last26=Akana Murphy |first26=Joseph M. |last27=Pidhorodetska |first27=Daria |last28=Polanski |first28=Alex |last29=Rice |first29=Malena |last30=Robertson |first30=Paul |journal=The Astronomical Journal |volume=164 |issue=3 |page=97 |bibcode=2022AJ....164...97M |s2cid=250113765 |display-authors=1 |doi-access=free }}

|0.0840{{±|0.0098}}

|

|8.689{{±|0.008}}

|0.0783{{±|0.0014}}

|697{{±|23}}

| style="background:#00FF00" |radial vel.

|450.6{{±|1.3}}

|0.851{{±|0.049}}

|4985{{±|121}}

|

|0.0712{{±|0.0574|0.0304}}

|0.454{{±|0.010}}

|2.69998{{±|0.00015}}

|0.0429{{±|0.0006}}

|

| style="background:#FFFF00" |transit

|375.3{{±|1.3|0.5}}

|1.46{{±|0.06}}

|5307{{±|18|16}}

|

|0.2643{{±|0.0220}}

|

|443{{±|11|13}}

|

|

| style="background:#00FF00" |radial vel.

|375.3{{±|1.3|0.5}}

|1.46{{±|0.06}}

|5307{{±|18|16}}

|{{citation|arxiv=2211.17035|year=2022|title=Radial velocity confirmation of a hot super-Neptune discovered by TESS with a warm Saturn-mass companion|last1=Knudstrup |first1=E. |last2=Gandolfi |first2=D. |last3=Nowak |first3=G. |last4=Persson |first4=C. M. |last5=Furlan |first5=E. |last6=Livingston |first6=J. |last7=Matthews |first7=E. |last8=Lundkvist |first8=M. S. |last9=Winther |first9=M. L. |last10=Rørsted |first10=J. L. |last11=Albrecht |first11=S. H. |last12=Goffo |first12=E. |last13=Carleo |first13=I. |last14=Deeg |first14=H. J. |last15=Collins |first15=K. A. |last16=Narita |first16=N. |last17=Isaacson |first17=H. |last18=Redfield |first18=S. |last19=Dai |first19=F. |last20=Hirano |first20=T. |last21=Akana Murphy |first21=J. M. |last22=Beard |first22=C. |last23=Buchhave |first23=L. A. |last24=Cary |first24=S. |last25=Chontos |first25=A. |last26=Crossfield |first26=I. |last27=Cochran |first27=W. D. |last28=Conti |first28=D. |last29=Dalba |first29=P. A. |last30=Esposito |first30=M. |journal=Monthly Notices of the Royal Astronomical Society |volume=519 |issue=4 |pages=5637–5655 |doi=10.1093/mnras/stac3684 |doi-access=free |display-authors=1 }}

|

|0.121{{±|0.013}}

|1.4520358{{±|0.0000098}}

|0.0230{{±|0.0026}}

|1136{{±|59}}

| style="background:#FFFF00" |transit

|106.0

|0.59{{±|0.23}}

|4266{{±|100}}

|

|0.0283{{±|0.0072|0.0063}}

|0.354{{±|0.012|0.010}}

|12.9972{{±|0.0006}}

|0.108{{±|0.003}}

|867{{±|17}}

| style="background:#FFFF00" |transit

|504.17{{±|0.12|0.09}}

|0.981{{±|0.062|0.065}}

|5840{{±|62}}

|Another planet in the system is suspected.{{citation|arxiv=2207.03293|year=2022|title=The GAPS programme at TNG. XL. A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422|doi=10.1051/0004-6361/202244079 |last1=Naponiello |first1=L. |last2=Mancini |first2=L. |last3=Damasso |first3=M. |last4=Bonomo |first4=A. |last5=Sozzetti |first5=A. |last6=Nardiello |first6=D. |last7=Biazzo |first7=K. |last8=Stognone |first8=R. |last9=Lillo-Box |first9=J. |last10=Lanza |first10=A. |last11=Poretti |first11=E. |last12=Lissauer |first12=J. |last13=Zeng |first13=L. |last14=Bieryla |first14=A. |last15=Hébrard |first15=G. |last16=Basilicata |first16=M. |last17=Benatti |first17=S. |last18=Bignamini |first18=A. |last19=Borsa |first19=F. |last20=Claudi |first20=R. |last21=Cosentino |first21=R. |last22=Covino |first22=E. |last23=de Gurtubai |first23=A. |last24=Delfosse |first24=X. |last25=Desidera |first25=S. |last26=Dragomir |first26=D. |last27=Eastman |first27=J. D. |last28=Essack |first28=Z. |last29=Fiorenzano |first29=A. F. M. |last30=Giacobbe |first30=P. |display-authors=1 |journal=Astronomy & Astrophysics |volume=A8 |page=667 |bibcode=2022A&A...667A...8N |s2cid=250334523 }}

|

|0.104{{±|0.005}}

|0.4090677{{±|0.0000003}}

|0.0071{{±|0.0002}}

|1072{{±|54}}

| style="background:#FFFF00" |transit

|134.5

|0.29{{±|0.02}}

|3330{{±|160}}

|

|0.0152{{±|0.0041}}

|0.149{{±|0.006}}

|11.06201{{±|0.00002}}

|0.061{{±|0.003}}

|326{{±|7}}

| style="background:#FFFF00" |transit

|99.51{{±|0.04}}

|0.249{{±|0.008}}

|3185{{±|50}}

|Also a red dwarf on a 97AU separation in the system{{cite journal|last1=Cadieux|first1=Charles|last2=Doyon|first2=René|last3=Plotnykov|first3=Mykhaylo|last4=Hébrard|first4=Guillaume|last5=Jahandar|first5=Farbod|last6=Artigau|first6=Étienne|last7=Valencia|first7=Diana|last8=Cook|first8=Neil J.|last9=Martioli|first9=Eder|last10=Vandal|first10=Thomas|last11=Donati|first11=Jean-François|last12=Cloutier|first12=Ryan|last13=Narita|first13=Norio|last14=Fukui|first14=Akihiko|last15=Hirano|first15=Teruyuki|last16=Bouchy|first16=François|last17=Cowan|first17=Nicolas B.|last18=Gonzales|first18=Erica J.|last19=Ciardi|first19=David R.|last20=Stassun|first20=Keivan G.|last21=Arnold|first21=Luc|last22=Benneke|first22=Björn|last23=Boisse|first23=Isabelle|last24=Bonfils|first24=Xavier|last25=Carmona|first25=Andrés|last26=Cortés-Zuleta|first26=Pía|last27=Delfosse|first27=Xavier|last28=Forveille|first28=Thierry|last29=Fouqué|first29=Pascal|last30=da Silva|first30=João Gomes|last31=Jenkins|first31=Jon M.|last32=Kiefer|first32=Flavien|last33=Kóspál|first33=Ágnes|last34=Lafrenière|first34=David|last35=Martins|first35=Jorge H. C.|last36=Moutou|first36=Claire|last37=do Nascimento|first37=J.-D.|last38=Ould-Elhkim|first38=Merwan|last39=Pelletier|first39=Stefan|last40=Twicken|first40=Joseph D.|last41=Bouma|first41=Luke G.|last42=Cartwright|first42=Scott|last43=Darveau-Bernier|first43=Antoine|last44=Grankin|first44=Konstantin|last45=Ikoma|first45=Masahiro|last46=Kagetani|first46=Taiki|last47=Kawauchi|first47=Kiyoe|last48=Kodama|first48=Takanori|last49=Kotani|first49=Takayuki|last50=Latham|first50=David W.|last51=Menou|first51=Kristen|last52=Ricker|first52=George|last53=Seager|first53=Sara|last54=Tamura|first54=Motohide|last55=Vanderspek|first55=Roland|last56=Watanabe|display-authors=2|first56=Noriharu|title=TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf|journal=The Astronomical Journal|volume=164:96|issue=3|date=27 June 2022 |publication-date=12 August 2022|arxiv=2208.06333|doi=10.3847/1538-3881/ac7cea|bibcode=2022AJ....164...96C|doi-access=free|pages=28pp}}

|0.0101{{±|0.0008}}

|0.114{{±|0.003}}

|1.8805136{{±|0.0000024|0.0000026}}

|

|682.2{{±|7.4|6.9}}

| style="background:#FFFF00" |transit

|80.64{{±|0.07}}

|0.339{{±|0.011}}

|3496{{±|25}}

|{{citation|arxiv=2208.10351|year=2022|title=TOI-1468: A system of two transiting planets, a super-Earth and a mini-Neptune, on opposite sides of the radius valley|last1=Chaturvedi |first1=P. |last2=Bluhm |first2=P. |last3=Nagel |first3=E. |last4=Hatzes |first4=A. P. |last5=Morello |first5=G. |last6=Brady |first6=M. |last7=Korth |first7=J. |last8=Molaverdikhani |first8=K. |last9=Kossakowski |first9=D. |last10=Caballero |first10=J. A. |last11=Guenther |first11=E. W. |last12=Pallé |first12=E. |last13=Espinoza |first13=N. |last14=Seifahrt |first14=A. |last15=Lodieu |first15=N. |last16=Cifuentes |first16=C. |last17=Furlan |first17=E. |last18=Amado |first18=P. J. |last19=Barclay |first19=T. |last20=Bean |first20=J. |last21=Béjar |first21=V. J. S. |last22=Bergond |first22=G. |last23=Boyle |first23=A. W. |last24=Ciardi |first24=D. |last25=Collins |first25=K. A. |last26=Collins |first26=K. I. |last27=Esparza-Borges |first27=E. |last28=Fukui |first28=A. |last29=Gnilka |first29=C. L. |last30=Goeke |first30=R. |journal=Astronomy & Astrophysics |volume=666 |pages=A155 |doi=10.1051/0004-6361/202244056 |bibcode=2022A&A...666A.155C |s2cid=251718760 |display-authors=1 }}

|0.0209{{±|0.0021}}

|0.184{{±|0.004}}

|15.532482{{±|0.000034|0.000033}}

|

|337.5{{±|3.7|3.4}}

| style="background:#FFFF00" |transit

|80.64{{±|0.07}}

|0.339{{±|0.011}}

|3496{{±|25}}

|

|3.16{{±|0.12}}

|1.36{{±|0.03}}

|2.056014{{±|0.000002}}

|

|1820

| style="background:#FFFF00" |transit

|804.6{{±|1.9}}

|1.085{{±|0.061|0.066}}

|6420{{±|100}}

|

|0.0132{{±|0.0085}}

|0.214{{±|0.016}}

|2.7

|

|

| style="background:#FFFF00" |transit

|364.6

|1.00{{±|0.05}}

|5542.3{{±|100.0}}

|{{citation|arxiv=2209.06958|year=2023|title=TESS-Keck Survey. XIV. Two Giant Exoplanets from the Distant Giants Survey|last1=Van Zandt |first1=Judah E. |last2=Petigura |first2=Erik A. |last3=MacDougall |first3=Mason |last4=Gilbert |first4=Gregory J. |last5=Lubin |first5=Jack |last6=Batalha |first6=Natalie M. |last7=Crossfield |first7=Ian J. M. |last8=Dressing |first8=Courtney |last9=Fulton |first9=Benjamin |last10=Howard |first10=Andrew W. |last11=Huber |first11=Daniel |last12=Isaacson |first12=Howard |last13=Kane |first13=Stephen R. |last14=Robertson |first14=Paul |last15=Roy |first15=Arpita |last16=Weiss |first16=Lauren M. |last17=Behmard |first17=Aida |last18=Beard |first18=Corey |last19=Chontos |first19=Ashley |last20=Dai |first20=Fei |last21=Dalba |first21=Paul A. |last22=Fetherolf |first22=Tara |last23=Giacalone |first23=Steven |last24=Hill |first24=Michelle L. |last25=Hirsch |first25=Lea A. |last26=Holcomb |first26=Rae |last27=Howell |first27=Steve B. |last28=Mayo |first28=Andrew |last29=Mocnik |first29=Teo |last30=Akana Murphy |first30=Joseph M. |journal=The Astronomical Journal |volume=165 |issue=2 |page=60 |doi=10.3847/1538-3881/aca6ef |bibcode=2023AJ....165...60V |s2cid=252280288 |display-authors=1 |doi-access=free }} Host star also known as BD+82 71, planet suspected since 2020{{citation|arxiv=2002.00691|year=2020|title=Vetting of 384 TESS Objects of Interest with TRICERATOPS and Statistical Validation of 12 Planet Candidates|doi=10.3847/1538-3881/abc6af |last1=Giacalone |first1=Steven |last2=Dressing |first2=Courtney D. |last3=Jensen |first3=Eric L. N. |last4=Collins |first4=Karen A. |last5=Ricker |first5=George R. |last6=Vanderspek |first6=Roland |last7=Seager |first7=S. |last8=Winn |first8=Joshua N. |last9=Jenkins |first9=Jon M. |last10=Barclay |first10=Thomas |last11=Barkaoui |first11=Khalid |last12=Cadieux |first12=Charles |last13=Charbonneau |first13=David |last14=Collins |first14=Kevin I. |last15=Conti |first15=Dennis M. |last16=Doyon |first16=René |last17=Evans |first17=Phil |last18=Ghachoui |first18=Mourad |last19=Gillon |first19=Michaël |last20=Guerrero |first20=Natalia M. |last21=Hart |first21=Rhodes |last22=Jehin |first22=Emmanuël |last23=Kielkopf |first23=John F. |last24=McLean |first24=Brian |last25=Murgas |first25=Felipe |last26=Palle |first26=Enric |last27=Parviainen |first27=Hannu |last28=Pozuelos |first28=Francisco J. |last29=Relles |first29=Howard M. |last30=Shporer |first30=Avi |journal=The Astronomical Journal |volume=161 |page=24 |s2cid=227141512 |display-authors=1 |doi-access=free }}

|0.602{{±|0.078}}

|

|501{{±|16}}

|

|

| style="background:#00FF00" |radial vel.

|364.6

|1.00{{±|0.05}}

|5542.3{{±|100.0}}

| Host star also known as BD+82 71, additional long-period companion is suspected.

|0.0979{{±|0.0066}}

|0.461{{±|0.016}}

|3.8

|

|

| style="background:#FFFF00" |transit

|405.7

|0.84{{±|0.03}}

|5066{{±|100}}

| Host star also known as TYC 4108-1434-1, planet suspected since 2020

|0.929{{±|0.037}}

|

|393.2{{±|4.3}}

|

|

| style="background:#00FF00" |radial vel.

|405.7

|0.84{{±|0.03}}

|5066{{±|100}}

| Host star also known as TYC 4108-1434-1

|0.04{{±|0.03}}

|0.184{{±|0.017|0.013}}

|10.98462{{±|0.00046|0.00051}}

|0.103{{±|0.002}}

|1062{{±|14|13}}

| style="background:#FFFF00" |transit

|540.6{{±|1.0|1.2}}

|1.21{{±|0.02}}

|6170{{±|61}}

|{{citation|arxiv=2203.04334|year=2022|title=TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration|doi=10.3847/1538-3881/ac5c4f |last1=Tran |first1=Quang H. |last2=Bowler |first2=Brendan P. |last3=Endl |first3=Michael |last4=Cochran |first4=William D. |last5=MacQueen |first5=Phillip J. |last6=Gandolfi |first6=Davide |last7=Persson |first7=Carina M. |last8=Fridlund |first8=Malcolm |last9=Palle |first9=Enric |last10=Nowak |first10=Grzegorz |last11=Deeg |first11=Hans J. |last12=Luque |first12=Rafael |last13=Livingston |first13=John H. |last14=Kabáth |first14=Petr |last15=Skarka |first15=Marek |last16=Šubjak |first16=Ján |last17=Howell |first17=Steve B. |last18=Albrecht |first18=Simon H. |last19=Collins |first19=Karen A. |last20=Esposito |first20=Massimiliano |last21=Van Eylen |first21=Vincent |last22=Grziwa |first22=Sascha |last23=Goffo |first23=Elisa |last24=Huang |first24=Chelsea X. |last25=Jenkins |first25=Jon M. |last26=Karjalainen |first26=Marie |last27=Karjalainen |first27=Raine |last28=Knudstrup |first28=Emil |last29=Korth |first29=Judith |last30=Lam |first30=Kristine W. F. |journal=The Astronomical Journal |volume=163 |issue=5 |page=225 |bibcode=2022AJ....163..225T |s2cid=247318919 |display-authors=1 |doi-access=free }}

|0.63{{±|0.09|0.08}}

|0.987{{±|0.025}}

|40.74976{{±|0.000022|0.00021}}

|0.249{{±|0.005}}

|684{{±|9}}

| style="background:#FFFF00" |transit

|540.6{{±|1.0|1.2}}

|1.21{{±|0.02}}

|6170{{±|61}}

|

|

|0.126{{±|0.009}}

|1.7666957{{±|0.0000054}}

|0.0226{{±|0.0004}}

|764{{±|19}}

| style="background:#FFFF00" |transit

|100.6

|0.49{{±|0.03}}

|3499{{±|70}}

|

|0.0173{{±|0.0031}}

|0.181{{±|0.016}}

|3.1342790{{±|0.0000072}}

|0.033548{{±|0.000260|0.000268}}

|590{{±|90}}

| style="background:#FFFF00" |transit

|147.2{{±|0.2}}

|0.51{{±|0.02}}

|3627{{±|31}}

|{{citation|arxiv=2211.06205|year=2023|title=A sub-Neptune planet around TOI-1695 discovered and characterized with SPIRou and TESS|last1=Kiefer |first1=F. |last2=Hébrard |first2=G. |last3=Martioli |first3=E. |last4=Artigau |first4=E. |last5=Doyon |first5=R. |last6=Donati |first6=J. -F. |last7=Cadieux |first7=C. |last8=Carmona |first8=A. |last9=Ciardi |first9=D. R. |last10=Cristofari |first10=P. I. |last11=de Almeida |first11=L. |last12=Figueira |first12=P. |last13=Gaidos |first13=E. |last14=Gonzales |first14=E. |last15=Lecavelier |first15=A. |last16=Stassun |first16=K. G. |last17=Arnold |first17=L. |last18=Benneke |first18=B. |last19=Boisse |first19=I. |last20=Bonfils |first20=X. |last21=Cook |first21=N. J. |last22=Cortés-Zuleta |first22=P. |last23=Delfosse |first23=X. |last24=Dias do Nascimento |first24=J. |last25=Fausnaugh |first25=M. |last26=Fong |first26=W. |last27=Fouqué |first27=P. |last28=Forveille |first28=T. |last29=Gomes da Silva |first29=J. |last30=Hesse |first30=K. |journal=Astronomy & Astrophysics |volume=670 |pages=A136 |doi=10.1051/0004-6361/202245129 |bibcode=2023A&A...670A.136K |s2cid=253498974 |display-authors=1 }}{{citation|arxiv=2211.06445|year=2023|title=TOI-1695 b: A Water World Orbiting an Early-M Dwarf in the Planet Radius Valley|last1=Cherubim |first1=Collin |last2=Cloutier |first2=Ryan |last3=Charbonneau |first3=David |last4=Stockdale |first4=Chris |last5=Stassun |first5=Keivan G. |last6=Schwarz |first6=Richard P. |last7=Safonov |first7=Boris |last8=Mortier |first8=Annelies |last9=Latham |first9=David W. |last10=Horne |first10=Keith |last11=Haywood |first11=Raphaëlle D. |last12=Gonzales |first12=Erica |last13=Goliguzova |first13=Maria V. |last14=Collins |first14=Karen A. |last15=Ciardi |first15=David R. |last16=Bieryla |first16=Allyson |last17=Belinski |first17=Alexander A. |last18=Watson |first18=Christopher A. |last19=Vanderspek |first19=Rolands |last20=Udry |first20=Stéphane |last21=Sozzetti |first21=Alessandro |last22=Ségransan |first22=Damien |last23=Sasselov |first23=Dimitar |last24=Ricker |first24=George R. |last25=Rice |first25=Ken |last26=Poretti |first26=Ennio |last27=Piotto |first27=Giampaolo |last28=Pepe |first28=Francesco |last29=Molinari |first29=Emilio |last30=Micela |first30=Giuseppina |journal=The Astronomical Journal |volume=165 |issue=4 |page=167 |doi=10.3847/1538-3881/acbdfd |bibcode=2023AJ....165..167C |s2cid=256627151 |display-authors=1 |doi-access=free }}

|0.1781

|0.276{{±|0.010}}

|2.500311{{±|0.000004}}

|0.0229{{±|0.0002}}

|489{{±|13}}

| style="background:#FFFF00" |transit

|210.8{{±|0.5}}

|0.255{{±|0.0066}}

|3185{{±|76}}

|{{citation|arxiv=2203.02694|year=2022|title=TOI-1696: A Nearby M4 Dwarf with a 3 R ⊕ Planet in the Neptunian Desert|last1=Mori |first1=Mayuko |last2=Livingston |first2=John H. |author3=Jerome de Leon |last4=Narita |first4=Norio |last5=Hirano |first5=Teruyuki |last6=Fukui |first6=Akihiko |last7=Collins |first7=Karen A. |last8=Fujita |first8=Naho |last9=Hori |first9=Yasunori |author10=Hiroyuki Tako Ishikawa |last11=Kawauchi |first11=Kiyoe |last12=Stassun |first12=Keivan G. |last13=Watanabe |first13=Noriharu |last14=Giacalone |first14=Steven |last15=Gore |first15=Rebecca |last16=Schroeder |first16=Ashley |last17=Dressing |first17=Courtney D. |last18=Bieryla |first18=Allyson |last19=Jensen |first19=Eric L. N. |last20=Massey |first20=Bob |last21=Shporer |first21=Avi |last22=Kuzuhara |first22=Masayuki |last23=Charbonneau |first23=David |last24=Ciardi |first24=David R. |last25=Doty |first25=John P. |last26=Esparza-Borges |first26=Emma |last27=Harakawa |first27=Hiroki |last28=Hodapp |first28=Klaus |last29=Ikoma |first29=Masahiro |last30=Ikuta |first30=Kai |journal=The Astronomical Journal |volume=163 |issue=6 |page=298 |doi=10.3847/1538-3881/ac6bf8 |bibcode=2022AJ....163..298M |s2cid=247291913 |display-authors=1 |doi-access=free }}{{citation|arxiv=2204.09063|year=2022|title=TOI-1696 and TOI-2136: Constraining the Masses of Two Mini-Neptunes with the Habitable-Zone Planet Finder|last1=Beard |first1=Corey |last2=Robertson |first2=Paul |last3=Kanodia |first3=Shubham |last4=Libby-Roberts |first4=Jessica |last5=Canas |first5=Caleb I. |last6=Gupta |first6=Arvind F. |last7=Holcomb |first7=Rae |last8=Jones |first8=Sinclaire |last9=Kobulnicky |first9=Henry A. |last10=Lin |first10=Andrea S. J. |last11=Lubin |first11=Jack |last12=Maney |first12=Marissa |last13=Parker |first13=Brock A. |last14=Stefansson |first14=Gudmundur |last15=Cochran |first15=William D. |last16=Endl |first16=Michael |last17=Hebb |first17=Leslie |last18=Mahadevan |first18=Suvrath |last19=Wisniewski |first19=John |last20=Bender |first20=Chad F. |last21=Diddams |first21=Scott A. |last22=Everett |first22=Mark |last23=Fredrick |first23=Connor |last24=Halverson |first24=Samuel |last25=Hearty |first25=Fred |last26=Metcalf |first26=Andrew J. |last27=Monson |first27=Andrew |last28=Ninan |first28=Joe P. |last29=Roy |first29=Arpita |last30=Schutte |first30=Maria |journal=The Astronomical Journal |volume=163 |issue=6 |page=286 |doi=10.3847/1538-3881/ac69ec |bibcode=2022AJ....163..286B |s2cid=248266475 |display-authors=1 |doi-access=free }}

|0.0890{{±|0.0148}}

|0.477{{±|0.010}}

|24.283429{{±|0.00043}}

|0.16{{±|0.04}}

|687{{±|50}}

| style="background:#FFFF00" |transit

|264.7{{±|0.2}}

|0.984{{±|0.050|0.059}}

|5665{{±|55}}

|{{citation|arxiv=2204.08984|year=2022|title=A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N|last1=König |first1=P. -C. |last2=Damasso |first2=M. |last3=Hébrard |first3=G. |last4=Naponiello |first4=L. |last5=Cortés-Zuleta |first5=P. |last6=Biazzo |first6=K. |last7=Santos |first7=N. C. |last8=Bonomo |first8=A. S. |last9=Lecavelier des Étangs |first9=A. |last10=Zeng |first10=L. |last11=Hoyer |first11=S. |last12=Sozzetti |first12=A. |last13=Affer |first13=L. |last14=Almenara |first14=J. M. |last15=Benatti |first15=S. |last16=Bieryla |first16=A. |last17=Boisse |first17=I. |last18=Bonfils |first18=X. |last19=Boschin |first19=W. |last20=Carmona |first20=A. |last21=Claudi |first21=R. |last22=Collins |first22=K. A. |last23=Dalal |first23=S. |last24=Deleuil |first24=M. |last25=Delfosse |first25=X. |last26=Demangeon |first26=O. D. S. |last27=Desidera |first27=S. |last28=Díaz |first28=R. F. |last29=Forveille |first29=T. |last30=Heidari |first30=N. |journal=Astronomy & Astrophysics |volume=666 |pages=A183 |doi=10.1051/0004-6361/202143002 |bibcode=2022A&A...666A.183K |s2cid=248239823 |display-authors=1 }}

|0.021{{±|0.06}}

|0.279{{±|0.02}}

|18.849975{{±|0.000006}}

|0.1176{{±|0.0013}}

|433{{±|14}}

| style="background:#FFFF00" |transit

|130.85{{±|0.05}}

|0.606{{±|0.020}}

|4065{{±|51}}

|{{citation|arxiv=2202.01240|year=2022|title=A Transiting, Temperate Mini-Neptune Orbiting the M Dwarf TOI-1759 Unveiled by TESS|doi=10.3847/1538-3881/ac4af0 |last1=Espinoza |first1=Néstor |last2=Pallé |first2=Enric |last3=Kemmer |first3=Jonas |last4=Luque |first4=Rafael |last5=Caballero |first5=José A. |last6=Cifuentes |first6=Carlos |last7=Herrero |first7=Enrique |last8=Sánchez Béjar |first8=Víctor J. |last9=Stock |first9=Stephan |last10=Molaverdikhani |first10=Karan |last11=Morello |first11=Giuseppe |last12=Kossakowski |first12=Diana |last13=Schlecker |first13=Martin |last14=Amado |first14=Pedro J. |last15=Bluhm |first15=Paz |last16=Cortés-Contreras |first16=Miriam |last17=Henning |first17=Thomas |last18=Kreidberg |first18=Laura |last19=Kürster |first19=Martin |last20=Lafarga |first20=Marina |last21=Lodieu |first21=Nicolas |last22=Morales |first22=Juan Carlos |last23=Oshagh |first23=Mahmoudreza |last24=Passegger |first24=Vera M. |last25=Pavlov |first25=Alexey |last26=Quirrenbach |first26=Andreas |last27=Reffert |first27=Sabine |last28=Reiners |first28=Ansgar |last29=Ribas |first29=Ignasi |last30=Rodríguez |first30=Eloy |journal=The Astronomical Journal |volume=163 |issue=3 |page=133 |bibcode=2022AJ....163..133E |s2cid=246485680 |display-authors=1 |doi-access=free }}{{citation|arxiv=2202.01259|year=2022|title=TOI-1759 b: A transiting sub-Neptune around a low mass star characterized with SPIRou and TESS|doi=10.1051/0004-6361/202142540 |last1=Martioli |first1=E. |last2=Hébrard |first2=G. |last3=Fouqué |first3=P. |last4=Artigau |first4=É. |last5=Donati |first5=J.-F. |last6=Cadieux |first6=C. |last7=Bellotti |first7=S. |last8=Lecavelier Des Etangs |first8=A. |last9=Doyon |first9=R. |last10=Do Nascimento |first10=J.-D. |last11=Arnold |first11=L. |last12=Carmona |first12=A. |last13=Cook |first13=N. J. |last14=Cortes-Zuleta |first14=P. |last15=De Almeida |first15=L. |last16=Delfosse |first16=X. |last17=Folsom |first17=C. P. |last18=König |first18=P.-C. |last19=Moutou |first19=C. |last20=Ould-Elhkim |first20=M. |last21=Petit |first21=P. |last22=Stassun |first22=K. G. |last23=Vidotto |first23=A. A. |last24=Vandal |first24=T. |last25=Benneke |first25=B. |last26=Boisse |first26=I. |last27=Bonfils |first27=X. |last28=Boyd |first28=P. |last29=Brasseur |first29=C. |last30=Charbonneau |first30=D. |journal=Astronomy & Astrophysics |volume=660 |pages=A86 |bibcode=2022A&A...660A..86M |s2cid=246485686 |display-authors=1 }}

|0.974{{±|0.075|0.076}}

|1.002{{±|0.026|0.024}}

|3.7130818{{±|0.0000028}}

|0.04393{{±|0.00058|0.00054}}

|961.5{{±|8}}

| style="background:#FFFF00" |transit

|418{{±|3}}

|0.819{{±|0.033|0.030}}

|4753{{±|54|55}}

|{{citation|arxiv=2205.05709|year=2023|title=Another shipment of six short-period giant planets from TESS|last1=Rodriguez |first1=Joseph E. |last2=Quinn |first2=Samuel N. |last3=Vanderburg |first3=Andrew |last4=Zhou |first4=George |last5=Eastman |first5=Jason D. |last6=Thygesen |first6=Erica |last7=Cale |first7=Bryson |last8=Ciardi |first8=David R. |last9=Reed |first9=Phillip A. |last10=Oelkers |first10=Ryan J. |last11=Collins |first11=Karen A. |last12=Bieryla |first12=Allyson |last13=Latham |first13=David W. |last14=Scott Gaudi |first14=B. |last15=Hellier |first15=Coel |last16=Sokolovsky |first16=Kirill |last17=Schulte |first17=Jack |last18=Srdoc |first18=Gregor |last19=Kielkopf |first19=John |author20=Ferran Grau Horta |last21=Massey |first21=Bob |last22=Evans |first22=Phil |last23=Stephens |first23=Denise C. |last24=McLeod |first24=Kim K. |last25=Chazov |first25=Nikita |last26=Krushinsky |first26=Vadim |last27=Ghachoui |first27=Mourad |last28=Safonov |first28=Boris |last29=Dedrick |first29=Cayla M. |last30=Conti |first30=Dennis |journal=Monthly Notices of the Royal Astronomical Society |volume=521 |issue=2 |pages=2765–2785 |doi=10.1093/mnras/stad595 |doi-access=free |display-authors=1 }}

|2.3{{±|0.2}}

|1.12{{±|0.02}}

|4.860700{{±|0.000010}}

|0.069{{±|0.005}}

|1295{{±|11}}

| style="background:#FFFF00" |transit

|807{{±|13}}

|1.04{{±|0.13}}

|5734{{±|50}}

|{{citation|arxiv=2204.13956|year=2022|title=Confirmation and characterisation of three giant planets detected by TESS from the FIES/NOT and Tull/Mc Donald spectrographs|last1=Knudstrup |first1=E. |last2=Serrano |first2=L. M. |last3=Gandolfi |first3=D. |last4=Albrecht |first4=S. H. |last5=Cochran |first5=W. D. |last6=Endl |first6=M. |last7=Macqueen |first7=P. |last8=Tronsgaard |first8=R. |last9=Bieryla |first9=A. |last10=Buchhave |first10=Lars A. |last11=Stassun |first11=K. |last12=Collins |first12=K. A. |last13=Nowak |first13=G. |last14=Deeg |first14=H. J. |last15=Barkaoui |first15=K. |last16=Safonov |first16=B. S. |last17=Strakhov |first17=I. A. |last18=Belinski |first18=A. A. |last19=Twicken |first19=J. D. |last20=Jenkins |first20=J. M. |last21=Howard |first21=A. W. |last22=Isaacson |first22=H. |last23=Winn |first23=J. N. |last24=Collins |first24=K. I. |last25=Conti |first25=D. M. |last26=Furesz |first26=G. |last27=Gan |first27=T. |last28=Kielkopf |first28=John F. |last29=Massey |first29=B. |last30=Murgas |first30=F. |journal=Astronomy & Astrophysics |volume=667 |pages=A22 |doi=10.1051/0004-6361/202243656 |bibcode=2022A&A...667A..22K |s2cid=251083570 |display-authors=1 }}

|

|0.117{{±|0.005}}

|1.0662107{{±|0.0000014}}

|0.0204{{±|0.0002}}

|1885{{±|28}}

| style="background:#FFFF00" |transit

|149.8

|0.99{{±|0.03}}

|5752{{±|100}}

|

|2.01{{±|0.17|0.16}}

|1.247{{±|0.059|0.062}}

|0.94667944{{±|0.00000047}}

|0.01932{{±|0.00035|0.00039}}

|2097{{±|35|36}}

| style="background:#FFFF00" |transit

|1366{{±|6}}

|1.072{{±|0.059|0.064}}

|5814{{±|91|93}}

|{{citation|arxiv=2210.15473|year=2023|title=The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets|last1=Yee |first1=Samuel W. |last2=Winn |first2=Joshua N. |last3=Hartman |first3=Joel D. |last4=Bouma |first4=Luke G. |last5=Zhou |first5=George |last6=Quinn |first6=Samuel N. |last7=Latham |first7=David W. |last8=Bieryla |first8=Allyson |last9=Rodriguez |first9=Joseph E. |last10=Collins |first10=Karen A. |last11=Alfaro |first11=Owen |last12=Barkaoui |first12=Khalid |last13=Beard |first13=Corey |last14=Belinski |first14=Alexander A. |last15=Benkhaldoun |first15=Zouhair |last16=Benni |first16=Paul |last17=Bernacki |first17=Krzysztof |last18=Boyle |first18=Andrew W. |last19=Paul Butler |first19=R. |last20=Caldwell |first20=Douglas A. |last21=Chontos |first21=Ashley |last22=Christiansen |first22=Jessie L. |last23=Ciardi |first23=David R. |last24=Collins |first24=Kevin I. |last25=Conti |first25=Dennis M. |last26=Crane |first26=Jeffrey D. |last27=Daylan |first27=Tansu |last28=Dressing |first28=Courtney D. |last29=Eastman |first29=Jason D. |last30=Essack |first30=Zahra |journal=The Astrophysical Journal Supplement Series |volume=265 |issue=1 |page=1 |doi=10.3847/1538-4365/aca286 |bibcode=2023ApJS..265....1Y |s2cid=253157404 |display-authors=1 |doi-access=free }}

|0.0324{{±|0.0070}}

|0.236{{±|0.010}}

|3.098331{{±|0.000021|0.000019}}

|0.04260{{±|0.00076|0.00067}}

|1475{{±|120|158}}

| style="background:#FFFF00" |transit

|566.3{{±|1.0}}

|1.074{{±|0.059|0.050}}

|5607{{±|86|82}}

|{{citation|arxiv=2209.14396|year=2023|title=TESS spots a mini-neptune interior to a hot saturn in the TOI-2000 system|last1=Sha |first1=Lizhou |last2=Vanderburg |first2=Andrew M. |last3=Huang |first3=Chelsea X. |last4=Armstrong |first4=David J. |last5=Brahm |first5=Rafael |last6=Giacalone |first6=Steven |last7=Wood |first7=Mackenna L. |last8=Collins |first8=Karen A. |last9=Nielsen |first9=Louise D. |last10=Hobson |first10=Melissa J. |last11=Ziegler |first11=Carl |last12=Howell |first12=Steve B. |last13=Torres-Miranda |first13=Pascal |last14=Mann |first14=Andrew W. |last15=Zhou |first15=George |last16=Delgado-Mena |first16=Elisa |last17=Rojas |first17=Felipe I. |last18=Abe |first18=Lyu |last19=Trifonov |first19=Trifon |last20=Adibekyan |first20=Vardan |last21=Sousa |first21=Sérgio G. |last22=Fajardo-Acosta |first22=Sergio B. |last23=Guillot |first23=Tristan |last24=Howard |first24=Saburo |last25=Littlefield |first25=Colin |last26=Hawthorn |first26=Faith |last27=Schmider |first27=François-Xavier |last28=Eberhardt |first28=Jan |last29=Tan |first29=Thiam-Guan |last30=Osborn |first30=Ares |journal=Monthly Notices of the Royal Astronomical Society |volume=524 |pages=1113–1138 |doi=10.1093/mnras/stad1666 |doi-access=free |display-authors=1 }}

|0.238{{±|0.012}}

|0.711{{±|0.011}}

|9.1270553{{±|0.0000073}}

|0.0875{{±|0.0016|0.0014}}

|1029{{±|84|111}}

| style="background:#FFFF00" |transit

|566.3{{±|1.0}}

|1.074{{±|0.059|0.050}}

|5607{{±|86|82}}

|

|4.4{{±|0.4}}

|1.120{{±|0.009}}

|8.872086{{±|0.000009}}

|0.089{{±|0.004}}

|1186{{±|11}}

| style="background:#FFFF00" |transit

|1106{{±|7}}

|1.32{{±|0.14}}

|5880{{±|53}}

|

|3.51{{±|0.36|0.35}}

|1.118{{±|0.031|0.030}}

|8.8720942{{±|0.0000080|0.0000079}}

|0.0886{{±|0.0019|0.0024}}

|1172{{±|18|17}}

| style="background:#FFFF00" |transit

|1095{{±|11}}

|1.176{{±|0.079|0.091}}

|5928{{±|76|75}}

|

|2.30{{±|0.08}}

|1.44{{±|0.11}}

|1.4971842{{±|0.0000031|0.0000033}}

|

|1998

| style="background:#FFFF00" |transit

|940{{±|3}}

|1.153{{±|0.100|0.093}}

|6160{{±|100}}

|Young host star

|

|0.184{{±|0.018}}

|13.79019{{±|0.00065|0.00084}}

|

|640{{±|20}}

| style="background:#FFFF00" |transit

|379.7{{±|0.5}}

|0.83{{±|0.03}}

|5185{{±|60}}

|Young host star belongs to NGC 3532{{citation|arxiv=2206.06254|year=2022|title=TESS Hunt for Young and Maturing Exoplanets (THYME). VII. Membership, Rotation, and Lithium in the Young Cluster Group-X and a New Young Exoplanet|doi=10.3847/1538-3881/ac8154 |last1=Newton |first1=Elisabeth R. |last2=Rampalli |first2=Rayna |last3=Kraus |first3=Adam L. |last4=Mann |first4=Andrew W. |last5=Curtis |first5=Jason L. |last6=Vanderburg |first6=Andrew |last7=Krolikowski |first7=Daniel M. |last8=Huber |first8=Daniel |last9=Petter |first9=Grayson C. |last10=Bieryla |first10=Allyson |last11=Tofflemire |first11=Benjamin M. |last12=Thao |first12=Pa Chia |last13=Wood |first13=Mackenna L. |last14=Kerr |first14=Ronan |last15=Safanov |first15=Boris S. |last16=Strakhov |first16=Ivan A. |last17=Ciardi |first17=David R. |last18=Giacalone |first18=Steven |last19=Dressing |first19=Courtney D. |last20=Gill |first20=Holden |last21=Savel |first21=Arjun B. |last22=Collins |first22=Karen A. |last23=Brown |first23=Peyton |last24=Murgas |first24=Felipe |last25=Isogai |first25=Keisuke |last26=Narita |first26=Norio |last27=Palle |first27=Enric |last28=Quinn |first28=Samuel N. |last29=Eastman |first29=Jason D. |last30=Fűrész |first30=Gábor |journal=The Astronomical Journal |volume=164 |issue=3 |page=115 |bibcode=2022AJ....164..115N |s2cid=249626353 |display-authors=1 |doi-access=free }}

|0.0157{{±|0.0151|0.0076}}

|0.182{{±|0.046}}

|10.50534{{±|0.00007|0.00008}}

|0.0752{{±|0.0047|0.0119}}

|488{{±|28|52}}

| style="background:#FFFF00" |transit

|203.26{{±|0.16}}

|0.540{{±|0.080}}

|3800{{±|100}}

|

|0.0200{{±|0.0077|0.0072}}

|0.196{{±|0.015}}

|7.851928{{±|0.000018|0.000016}}

|0.057{{±|0.006}}

|395{{±|24|22}}

| style="background:#FFFF00" |transit

|108.82{{±|0.07}}

|0.34{{±|0.02}}

|3342{{±|100}}

|{{citation|arxiv=2202.10024|year=2022|title=TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136|doi=10.1093/mnras/stac1448 |last1=Gan |first1=Tianjun |last2=Soubkiou |first2=Abderahmane |last3=Wang |first3=Sharon X. |last4=Benkhaldoun |first4=Zouhair |last5=Mao |first5=Shude |last6=Artigau |first6=Étienne |last7=Fouqué |first7=Pascal |last8=Giacalone |first8=Steven |last9=Theissen |first9=Christopher A. |last10=Aganze |first10=Christian |last11=Collins |first11=Karen A. |last12=Shporer |first12=Avi |last13=Barkaoui |first13=Khalid |last14=Ghachoui |first14=Mourad |last15=Howell |first15=Steve B. |last16=Lamman |first16=Claire |last17=Demangeon |first17=Olivier D. S. |last18=Burdanov |first18=Artem |last19=Cadieux |first19=Charles |last20=Chouqar |first20=Jamila |last21=Collins |first21=Kevin I. |last22=Cook |first22=Neil J. |last23=Delrez |first23=Laetitia |last24=Demory |first24=Brice-Olivier |last25=Doyon |first25=René |last26=Dransfield |first26=Georgina |last27=Dressing |first27=Courtney D. |last28=Ducrot |first28=Elsa |last29=Fan |first29=Jiahao |last30=Garcia |first30=Lionel |journal=Monthly Notices of the Royal Astronomical Society |volume=514 |issue=3 |pages=4120–4139 |doi-access=free |display-authors=1 }}{{citation|arxiv=2202.10182|year=2022|title=Validation and atmospheric exploration of the sub-Neptune TOI-2136b around a nearby M3 dwarf|last1=Kawauchi |first1=K. |last2=Murgas |first2=F. |last3=Palle |first3=E. |last4=Narita |first4=N. |last5=Fukui |first5=A. |last6=Hirano |first6=T. |last7=Parviainen |first7=H. |last8=Ishikawa |first8=H. T. |last9=Watanabe |first9=N. |last10=Esparaza-Borges |first10=E. |last11=Kuzuhara |first11=M. |last12=Orell-Miquel |first12=J. |last13=Krishnamurthy |first13=V. |last14=Mori |first14=M. |last15=Kagetani |first15=T. |last16=Zou |first16=Y. |last17=Isogai |first17=K. |last18=Livingston |first18=J. H. |last19=Howell |first19=S. B. |last20=Crouzet |first20=N. |last21=de Leon |first21=J. P. |last22=Kimura |first22=T. |last23=Kodama |first23=T. |last24=Korth |first24=J. |last25=Kurita |first25=S. |last26=Laza-Ramos |first26=A. |last27=Luque |first27=R. |last28=Madrigal-Aguado |first28=A. |last29=Miyakawa |first29=K. |last30=Morello |first30=G. |journal=Astronomy & Astrophysics |volume=666 |pages=A4 |doi=10.1051/0004-6361/202243381 |bibcode=2022A&A...666A...4K |s2cid=247011479 |display-authors=1 }}

|5.35{{±|0.32|0.35}}

|1.103{{±|0.031|0.029}}

|10.261081{{±|0.000026|0.000027}}

|0.1108{{±|0.0012|0.0015}}

|1484{{±|16|14}}

| style="background:#FFFF00" |transit

|733{{±|5}}

|1.720{{±|0.057|0.068}}

|6189{{±|67}}

|Host star also known as HIP 86040

|2.83{{±|0.38|0.37}}

|1.281{{±|0.050|0.046}}

|3.3773512{{±|0.0000060|0.0000061}}

|0.05064{{±|0.00093|0.0011}}

|1802{{±|60|54}}

| style="background:#FFFF00" |transit

|988{{±|13}}

|1.516{{±|0.085|0.10}}

|6630{{±|300|290}}

|Planet orbiting primary of binary star

|0.92{{±|0.19|0.18}}

|1.453{{±|0.053|0.048}}

|3.8240801{{±|0.0000025}}

|0.0513{{±|0.0011|0.0013}}

|1580{{±|27}}

| style="background:#FFFF00" |transit

|967{{±|10}}

|1.233{{±|0.077|0.090}}

|6280{{±|160}}

|

|2.755{{±|0.087|0.081}}

|1.010{{±|0.022|0.019}}

|260.79{{±|0.59|0.58}}

|0.828{{±|0.012}}

|348.0{{±|3.3|3.6}}

| style="background:#FFFF00" |transit

|379.4{{±|0.8}}

|1.111{{±|0.047|0.046}}

|5695{{±|58|60}}

|{{citation|arxiv=2201.04146|year=2022|title=The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 Day Orbit with the Automated Planet Finder Telescope|doi=10.3847/1538-3881/ac415b |last1=Dalba |first1=Paul A. |last2=Kane |first2=Stephen R. |last3=Dragomir |first3=Diana |last4=Villanueva |first4=Steven |last5=Collins |first5=Karen A. |last6=Jacobs |first6=Thomas Lee |last7=Lacourse |first7=Daryll M. |last8=Gagliano |first8=Robert |last9=Kristiansen |first9=Martti H. |last10=Omohundro |first10=Mark |last11=Schwengeler |first11=Hans M. |last12=Terentev |first12=Ivan A. |last13=Vanderburg |first13=Andrew |last14=Fulton |first14=Benjamin |last15=Isaacson |first15=Howard |last16=Van Zandt |first16=Judah |last17=Howard |first17=Andrew W. |last18=Thorngren |first18=Daniel P. |last19=Howell |first19=Steve B. |last20=Batalha |first20=Natalie M. |last21=Chontos |first21=Ashley |last22=Crossfield |first22=Ian J. M. |last23=Dressing |first23=Courtney D. |last24=Huber |first24=Daniel |last25=Petigura |first25=Erik A. |last26=Robertson |first26=Paul |last27=Roy |first27=Arpita |last28=Weiss |first28=Lauren M. |last29=Behmard |first29=Aida |last30=Beard |first30=Corey |journal=The Astronomical Journal |volume=163 |issue=2 |page=61 |bibcode=2022AJ....163...61D |s2cid=245877799 |display-authors=1 |doi-access=free }}

|0.82{{±|0.08}}

|0.960{{±|0.012}}

|8.60077{{±|0.00003}}

|0.075{{±|0.004}}

|1188{{±|10}}

| style="background:#FFFF00" |transit

|652{{±|3}}

|1.12{{±|0.12}}

|5673{{±|50}}

|

|0.94{{±|0.18}}

|1.77

|2.1225735{{±|0.0000016}}

|0.03319{{±|0.00052|0.00051}}

|1763{{±|21|22}}

| style="background:#FFFF00" |transit

|1126{{±|3}}

|1.082{{±|0.052|0.049}}

|5974{{±|110}}

|Also 0.54{{Solar_mass}} star in the system{{citation|arxiv=2205.09728|year=2022|title=The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets|last1=Yee |first1=Samuel W. |last2=Winn |first2=Joshua N. |last3=Hartman |first3=Joel D. |last4=Rodriguez |first4=Joseph E. |last5=Zhou |first5=George |last6=Quinn |first6=Samuel N. |last7=Latham |first7=David W. |last8=Bieryla |first8=Allyson |last9=Collins |first9=Karen A. |last10=Addison |first10=Brett C. |last11=Angelo |first11=Isabel |last12=Barkaoui |first12=Khalid |last13=Benni |first13=Paul |last14=Boyle |first14=Andrew W. |last15=Brahm |first15=Rafael |last16=Paul Butler |first16=R. |last17=Ciardi |first17=David R. |last18=Collins |first18=Kevin I. |last19=Conti |first19=Dennis M. |last20=Crane |first20=Jeffrey D. |last21=Dai |first21=Fei |last22=Dressing |first22=Courtney D. |last23=Eastman |first23=Jason D. |last24=Essack |first24=Zahra |last25=Forés-Toribio |first25=Raquel |last26=Furlan |first26=Elise |last27=Gan |first27=Tianjun |last28=Giacalone |first28=Steven |last29=Gill |first29=Holden |last30=Girardin |first30=Eric |journal=The Astronomical Journal |volume=164 |issue=2 |page=70 |doi=10.3847/1538-3881/ac73ff |bibcode=2022AJ....164...70Y |s2cid=248887656 |display-authors=1 |doi-access=free }}

|0.0818{{±|0.0041}}

|0.313{{±|0.013}}

|1.1947268{{±|0.0000079|0.0000093}}

|0.02234{{±|0.00060}}

|1860{{±|20}}

| style="background:#FFFF00" |transit

|861{{±|3}}

|1.032{{±|0.038}}

|5634{{±|31}}

|Neptunian desert planet{{citation|arxiv=2208.05797|year=2022|title=TOI-2196 b: Rare planet in the hot Neptune desert transiting a G-type star|last1=Persson |first1=Carina M. |last2=Georgieva |first2=Iskra Y. |last3=Gandolfi |first3=Davide |last4=Acuña |first4=Lorena |last5=Aguichine |first5=Artem |last6=Muresan |first6=Alexandra |last7=Guenther |first7=Eike |last8=Livingston |first8=John |last9=Collins |first9=Karen A. |last10=Fridlund |first10=Malcolm |last11=Goffo |first11=Elisa |last12=Jenkins |first12=James S. |last13=Kabáth |first13=Petr |last14=Korth |first14=Judith |last15=Levine |first15=Alan M. |last16=Serrano |first16=Luisa M. |last17=Vines |first17=José |last18=Barragán |first18=Oscar |last19=Carleo |first19=Ilaria |last20=Colon |first20=Knicole D. |last21=Cochran |first21=William D. |last22=Christiansen |first22=Jessie L. |last23=Deeg |first23=Hans J. |last24=Deleuil |first24=Magali |last25=Dragomir |first25=Diana |last26=Esposito |first26=Massimiliamo |last27=Gan |first27=Tianjun |last28=Grziwa |first28=Sascha |last29=Hatzes |first29=Artie P. |last30=Hesse |first30=Katharine |journal=Astronomy & Astrophysics |volume=666 |pages=A184 |doi=10.1051/0004-6361/202244118 |bibcode=2022A&A...666A.184P |s2cid=251478602 |display-authors=1 }}

|0.64{{±|0.10|0.12}}

|0.995{{±|0.028|0.027}}

|8.001968{{±|0.000024|0.000025}}

|0.0854{{±|0.0015|0.0016}}

|1259{{±|16|15}}

| style="background:#FFFF00" |transit

|1242{{±|9}}

|1.296{{±|0.069|0.072}}

|6075{{±|110}}

|

|

|0.145{{±|0.012}}

|0.3524728{{±|0.0000047}}

|0.0097{{±|0.0001}}

|2609{{±|86}}

| style="background:#FFFF00" |transit

|331.2

|0.99{{±|0.04}}

|5534{{±|100}}

|

|1.58{{±|0.40|0.39}}

|1.282{{±|0.032|0.031}}

|3.5315902{{±|0.0000026}}

|0.05009{{±|0.00080|0.00082}}

|1688{{±|19|21}}

| style="background:#FFFF00" |transit

|1149{{±|5}}

|1.343{{±|0.066|0.065}}

|6164{{±|50}}

|

|1.60{{±|0.15}}

|0.9{{±|0.1}}

|2.99432{{±|0.00008}}

|0.04467

|

| style="background:#FFFF00" |transit

|1780{{±|20}}

|1.325{{±|0.118}}

|4780{{±|100}}

|{{citation|arxiv=2201.04140|year=2022|title=TESS Giants Transiting Giants. II. The Hottest Jupiters Orbiting Evolved Stars|doi=10.3847/1538-3881/ac4972 |last1=Grunblatt |first1=Samuel K. |last2=Saunders |first2=Nicholas |last3=Sun |first3=Meng |last4=Chontos |first4=Ashley |last5=Soares-Furtado |first5=Melinda |last6=Eisner |first6=Nora |last7=Pereira |first7=Filipe |last8=Komacek |first8=Thaddeus |last9=Huber |first9=Daniel |last10=Collins |first10=Karen |last11=Wang |first11=Gavin |last12=Stockdale |first12=Chris |last13=Quinn |first13=Samuel N. |last14=Tronsgaard |first14=Rene |last15=Zhou |first15=George |last16=Nowak |first16=Grzegorz |last17=Deeg |first17=Hans J. |last18=Ciardi |first18=David R. |last19=Boyle |first19=Andrew |last20=Rice |first20=Malena |last21=Dai |first21=Fei |last22=Blunt |first22=Sarah |last23=Van Zandt |first23=Judah |last24=Beard |first24=Corey |last25=Akana Murphy |first25=Joseph M. |last26=Dalba |first26=Paul A. |last27=Lubin |first27=Jack |last28=Polanski |first28=Alex |last29=Brinkman |first29=Casey Lynn |last30=Howard |first30=Andrew W. |journal=The Astronomical Journal |volume=163 |issue=3 |page=120 |bibcode=2022AJ....163..120G |s2cid=245877793 |display-authors=1 |doi-access=free }}

|0.225{{±|0.043|0.049}}

|0.768{{±|0.023|0.018}}

|4.0197517{{±|0.0000043}}

|0.04871{{±|0.00069|0.00079}}

|1091{{±|17|14}}

| style="background:#FFFF00" |transit

|713{{±|6}}

|0.954{{±|0.041|0.046}}

|5306{{±|76|68}}

|

|

|0.150{{±|0.010}}

|0.7826942{{±|0.0000037}}

|0.0144{{±|0.0001}}

|1355{{±|45}}

| style="background:#FFFF00" |transit

|194.5

|0.65{{±|0.02}}

|4099{{±|123}}

|

|0.333{{±|0.079}}

|0.925{{±|0.035|0.034}}

|4.3474032{{±|0.0000079|0.0000078}}

|0.0543{{±|0.0021|0.0010}}

|1534{{±|20|28}}

| style="background:#FFFF00" |transit

|1067{{±|7}}

|1.131{{±|0.130|0.064}}

|5577{{±|50}}

|

|

|0.161{{±|0.011}}

|1.3060011{{±|0.0000102}}

|0.0202{{±|0.0002}}

|1117{{±|46}}

| style="background:#FFFF00" |transit

|93.1

|0.64{{±|0.02}}

|4072{{±|121}}

|

|

|0.112{{±|0.007}}

|0.3711281{{±|0.0000005}}

|0.0064{{±|0.0001}}

|1060{{±|54}}

| style="background:#FFFF00" |transit

|158.7

|0.25{{±|0.01}}

|3333{{±|157}}

|

|5.21{{±|0.52}}

|1.000{{±|0.040|0.038}}

|10.655661{{±|0.000026}}

|0.1167{{±|0.0018|0.0017}}

| 1596{{±|44|41}}

| style="background:#FFFF00" |transit

|930{{±|14}}

|1.861{{±|0.086|0.081}}

|7360{{±|290|270}}

|

|0.201{{±|0.034|0.031}}

|0.975{{±|0.031|0.029}}

|5.983944{{±|0.000013}}

|0.0672{{±|0.0024|0.0012}}

|1352{{±|18|19}}

| style="background:#FFFF00" |transit

|1691{{±|8}}

|1.130{{±|0.130|0.059}}

|5650{{±|50}}

|

|0.820{{±|0.063|0.065}}

|1.217{{±|0.035|0.034}}

|2.9887615{{±|0.0000022}}

|0.04145{{±|0.00081|0.00086}}

|1431{{±|24|23}}

| style="background:#FFFF00" |transit

|1179{{±|6}}

|1.063{{±|0.063|0.065}}

|5765{{±|50}}

|

|0.250{{±|0.058|0.056}}

|1.290{{±|0.040|0.033}}

|4.5207265{{±|0.0000049}}

|0.0571{{±|0.0010|0.0013}}

|1456{{±|19|16}}

| style="background:#FFFF00" |transit

|1831{{±|9}}

|1.215{{±|0.063|0.082}}

|5936{{±|65|68}}

|

|0.218{{±|0.054|0.046}}

|1.077{{±|0.042|0.040}}

|5.456640{{±|0.000011}}

|0.0635{{±|0.0025|0.0013}}

|1445{{±|23|26}}

| style="background:#FFFF00" |transit

|1242{{±|10}}

|1.15{{±|0.14|0.07}}

|5760{{±|80|79}}

|

|0.61{{±|0.19}}

|1.76{{±|0.16}}

|6.2034{{±|0.0001}}

|

|

| style="background:#FFFF00" |transit

|1294{{±|9}}

|1.19{{±|0.16}}

|4800{{±|100}}

|

|0.44{{±|0.10|0.11}}

|1.59

|4.8084983{{±|0.0000057|0.0000056}}

|0.0569{{±|0.0010|0.0011}}

|1205{{±|18|17}}

| style="background:#FFFF00" |transit

|1150{{±|6}}

|1.063{{±|0.057|0.062}}

|5764{{±|81|78}}

|

|0.975{{±|0.083|0.070}}

|1.616{{±|0.034|0.032}}

|1.96229325{{±|0.00000082}}

|0.03185{{±|0.00052}}

|1893{{±|29|28}}

| style="background:#FFFF00" |transit

|1635{{±|9}}

|1.118{{±|0.056|0.054}}

|6280{{±|99|96}}

|

|0.71{{±|0.26}}

|1.363{{±|0.046|0.045}}

|4.0397090{{±|0.0000024|0.0000023}}

|0.0493{{±|0.0010|0.0008}}

|1376{{±|26|24}}

| style="background:#FFFF00" |transit

|1028{{±|3}}

|0.977{{±|0.063|0.049}}

|5721{{±|88|83}}

|

|0.370{{±|0.052|0.047}}

|1.146{{±|0.051|0.048}}

|3.5514058{{±|0.0000077|0.0000078}}

|0.0475{{±|0.0010|0.0011}}

|1471{{±|29|27}}

| style="background:#FFFF00" |transit

|1501{{±|8}}

|1.135{{±|0.077|0.079}}

|5910{{±|100}}

|

|1.68{{±|0.26|0.25}}

|1.174{{±|0.031|0.027}}

|2.3505614{{±|0.0000025}}

|0.03386{{±|0.00067|0.00050}}

|1544{{±|26}}

| style="background:#FFFF00" |transit

|1160{{±|30}}

|0.936{{±|0.057|0.041}}

|5691{{±|94|93}}

|

|0.62{{±|0.10|0.09}}

|1.466{{±|0.043|0.032}}

|3.9014971{{±|0.0000031}}

|0.0505{{±|0.0015|0.0009}}

|1596{{±|24|25}}

| style="background:#FFFF00" |transit

|1281{{±|5}}

|1.12{{±|0.11|0.06}}

|5760{{±|85|88}}

|

|2.27{{±|0.16}}

|1.158{{±|0.043}}

|2.0180231{{±|0.0000043|0.0000044}}

|0.03144{{±|0.00048|0.00055}}

|1488{{±|31|29}}

| style="background:#FFFF00" |transit

|733{{±|4}}

|1.016{{±|0.047|0.052}}

|5521{{±|110}}

|Also 0.6{{Solar_mass}} star in the system

|1.67{{±|0.12|0.13}}

|1.091{{±|0.038|0.032}}

|5.8768918{{±|0.0000069}}

|0.0675{{±|0.0011|0.0016}}

|1264{{±|22|21}}

| style="background:#FFFF00" |transit

|899{{±|3}}

|1.186{{±|0.059|0.083}}

|5706{{±|95|91}}

|

|1.18{{±|0.14}}

|2.10

|3.1199990{{±|0.0000079}}

|0.04289{{±|0.00092|0.00093}}

|1498{{±|22}}

| style="background:#FFFF00" |transit

|921{{±|10}}

|1.081{{±|0.071|0.069}}

|5969{{±|50}}

|Also 0.8{{Solar_mass}} star in the system

|0.26{{±|0.02}}

|0.74{{±|0.02}}

|3.936551{{±|0.000005|0.000006}}

|0.043{{±|0.002}}

|690{{±|20}}

| style="background:#FFFF00" |transit

|423.1{{±|1.0}}

|0.63{{±|0.02}}

|3870{{±|90}}

|

|0.98{{±|0.10|0.11}}

|1.167{{±|0.048|0.044}}

|3.246075{{±|0.000012}}

|0.04560{{±|0.00089|0.00098}}

|1534{{±|29|28}}

| style="background:#FFFF00" |transit

|1308{{±|6}}

|1.199{{±|0.072|0.076}}

|5950{{±|100}}

|

| 1.02{{±|0.24|0.22}}

| 1.124{{±|0.029|0.023}}

|9.088516{{±|0.000026|0.000027}}

|0.0813{{±|0.0011|0.0012}}

|801{{±|13|12}}

| style="background:#FFFF00" |transit

|576{{±|2}}

|0.867{{±|0.036|0.037}}

|5274{{±|50}}

|

|0.70{{±|0.003}}

|1.01{{±|0.03}}

|2.154849{{±|0.000001}}

|0.027{{±|0.001}}

|750{{±|20}}

| style="background:#FFFF00" |transit

|367.0{{±|0.6|1.3}}

|0.53{{±|0.02}}

|3660{{±|90}}

|{{citation|arxiv=2201.09963|year=2022|title=TOI-3714 b and TOI-3629 b: Two Gas Giants Transiting M Dwarfs Confirmed with the Habitable-zone Planet Finder and NEID|last1=Cañas |first1=Caleb I. |last2=Kanodia |first2=Shubham |last3=Bender |first3=Chad F. |last4=Mahadevan |first4=Suvrath |last5=Stefánsson |first5=Guðmundur |last6=Cochran |first6=William D. |last7=Lin |first7=Andrea S. J. |last8=Powers |first8=Luke |last9=Monson |first9=Andrew |last10=Green |first10=Elizabeth M. |last11=Parker |first11=Brock A. |last12=Swaby |first12=Tera N. |last13=Kobulnicky |first13=Henry A. |last14=Wisniewski |first14=John |last15=Gupta |first15=Arvind F. |last16=Everett |first16=Mark E. |last17=Jones |first17=Sinclaire |last18=Anjakos |first18=Benjamin |last19=Beard |first19=Corey |last20=Blake |first20=Cullen H. |last21=Diddams |first21=Scott A. |last22=Dong |first22=Zehao |last23=Fredrick |first23=Connor |last24=Hakemiamjad |first24=Elnaz |last25=Hebb |first25=Leslie |last26=Libby-Roberts |first26=Jessica E. |last27=Logsdon |first27=Sarah E. |last28=McElwain |first28=Michael W. |last29=Metcalf |first29=Andrew J. |last30=Ninan |first30=Joe P. |journal=The Astronomical Journal |volume=164 |issue=2 |page=50 |doi=10.3847/1538-3881/ac7804 |bibcode=2022AJ....164...50C |s2cid=246275821 |display-authors=1 |doi-access=free }}

|0.2684{{±|0.0276}}

|1.07{{±|0.04|0.05}}

|3.4387530{{±|0.0000039|0.0000040}}

|0.03845{{±|0.00043}}

|759{{±|13}}

| style="background:#FFFF00" |transit

|579{{±|2}}

|0.64{{±|0.02}}

|3913{{±|56}}

|{{citation|arxiv=2203.07178|year=2022|title=TOI-3757 b: A Low-density Gas Giant Orbiting a Solar-metallicity M Dwarf|last1=Kanodia |first1=Shubham |last2=Libby-Roberts |first2=Jessica |last3=Canas |first3=Caleb I. |last4=Ninan |first4=Joe P. |last5=Mahadevan |first5=Suvrath |last6=Stefansson |first6=Gudmundur |last7=Lin |first7=Andrea S. J. |last8=Jones |first8=Sinclaire |last9=Monson |first9=Andrew |last10=Parker |first10=Brock A. |last11=Kobulnicky |first11=Henry A. |last12=Swaby |first12=Tera N. |last13=Powers |first13=Luke |last14=Beard |first14=Corey |last15=Bender |first15=Chad F. |last16=Blake |first16=Cullen H. |last17=Cochran |first17=William D. |last18=Dong |first18=Jiayin |last19=Diddams |first19=Scott A. |last20=Fredrick |first20=Connor |last21=Gupta |first21=Arvind F. |last22=Halverson |first22=Samuel |last23=Hearty |first23=Fred |last24=Logsdon |first24=Sarah E. |last25=Metcalf |first25=Andrew J. |last26=McElwain |first26=Michael W. |last27=Morley |first27=Caroline |last28=Rajagopal |first28=Jayadev |last29=Ramsey |first29=Lawrence W. |last30=Robertson |first30=Paul |journal=The Astronomical Journal |volume=164 |issue=3 |page=81 |doi=10.3847/1538-3881/ac7c20 |bibcode=2022AJ....164...81K |s2cid=247446993 |display-authors=1 |doi-access=free }}

|1.04{{±|0.15|0.14}}

|2.00

|2.8989727{{±|0.0000038|0.0000039}}

|0.0421{{±|0.0007|0.0011}}

|1646{{±|25|24}}

| style="background:#FFFF00" |transit

|1399{{±|7}}

|1.181{{±|0.064|0.092}}

|5772{{±|84|80}}

|

|1.11{{±|0.18|0.20}}

|1.172{{±|0.036|0.035}}

|3.2443141{{±|0.0000055}}

|0.04611{{±|0.00069|0.00096}}

|1633{{±|21|19}}

| style="background:#FFFF00" |transit

|1834{{±|17}}

|1.242{{±|0.057|0.076}}

|5859{{±|72|71}}

|

|0.0519{{±|0.0110|0.0057}}

|0.563{{±|0.025}}

|4.5445697{{±|0.0000094}}

|0.0354{{±|0.0014}}

|463{{±|12}}

| style="background:#FFFF00" |transit

|141.37{{±|0.16}}

|0.2813{{±|0.0067}}

|3269{{±|70}}

|{{citation|arxiv=2210.10909|year=2022|title=TOI-3884 b: A rare 6-RE planet that transits a low-mass star with a giant and likely polar spot|doi=10.1051/0004-6361/202244791 |last1=Almenara |first1=J. M. |last2=Bonfils |first2=X. |last3=Forveille |first3=T. |last4=Astudillo-Defru |first4=N. |last5=Ciardi |first5=D. R. |last6=Schwarz |first6=R. P. |last7=Collins |first7=K. A. |last8=Cointepas |first8=M. |last9=Lund |first9=M. B. |last10=Bouchy |first10=F. |last11=Charbonneau |first11=D. |last12=Díaz |first12=R. F. |last13=Delfosse |first13=X. |last14=Kidwell |first14=R. C. |last15=Kunimoto |first15=M. |last16=Latham |first16=D. W. |last17=Lissauer |first17=J. J. |last18=Murgas |first18=F. |last19=Ricker |first19=G. |last20=Seager |first20=S. |last21=Vezie |first21=M. |last22=Watanabe |first22=D. |journal=Astronomy & Astrophysics |volume=667 |pages=L11 |bibcode=2022A&A...667L..11A |s2cid=253018639 }}{{citation|arxiv=2302.04757|year=2023|title=An In-Depth Look at TOI-3884b: a Super-Neptune Transiting a M4 Dwarf with Persistent Star Spot Crossings |last1=Libby-Roberts |first1=Jessica E. |last2=Schutte |first2=Maria |last3=Hebb |first3=Leslie |last4=Kanodia |first4=Shubham |last5=Canas |first5=Caleb |last6=Stefansson |first6=Gudmundur |last7=Lin |first7=Andrea S. J. |author8-link=Suvrath Mahadevan |last8=Mahadevan |first8=Suvrath |last9=Parts |first9=Winter |last10=Powers |first10=Luke |last11=Wisniewski |first11=John |last12=Bender |first12=Chad F. |last13=Cochran |first13=William D. |last14=Diddams |first14=Scott A. |last15=Everett |first15=Mark E. |last16=Gupta |first16=Arvind F. |last17=Halverson |first17=Samuel |last18=Kobulnicky |first18=Henry A. |last19=Kowalski |first19=Adam F. |last20=Larsen |first20=Alexander |last21=Monson |first21=Andrew |last22=Ninan |first22=Joe P. |last23=Parker |first23=Brock A. |last24=Ramsey |first24=Lawrence W. |last25=Robertson |first25=Paul |last26=Schwab |first26=Christian |last27=Swaby |first27=Tera N. |last28=Terrien |first28=Ryan C. }}

|0.406{{±|0.071|0.068}}

|1.274{{±|0.041|0.040}}

|3.4936264{{±|0.0000038}}

|0.0463{{±|0.0012|0.0010}}

|1512{{±|20}}

| style="background:#FFFF00" |transit

|1533{{±|9}}

|1.088{{±|0.086|0.070}}

|5725{{±|69|68}}

|

|0.175{{±|0.037|0.036}}

|1.095{{±|0.036|0.035}}

|6.607662{{±|0.000016|0.000015}}

|0.0743{{±|0.0013|0.0014}}

|1295{{±|16|14}}

| style="background:#FFFF00" |transit

|1703{{±|8}}

|1.254{{±|0.067|0.072}}

|5975{{±|70|69}}

|

|0.73{{±|0.14}}

|1.164{{±|0.025|0.024}}

|3.17748350{{±|0.00000094}}

|0.04469{{±|0.00048|0.00054}}

|1458{{±|20|17}}

| style="background:#FFFF00" |transit

|1013{{±|4}}

|1.178{{±|0.039|0.042}}

|6060{{±|74|67}}

|

|1.44{{±|0.17|0.15}}

|1.211{{±|0.040|0.039}}

|3.8016122{{±|0.0000065}}

|0.05222{{±|0.00089|0.00096}}

|1570{{±|25|24}}

| style="background:#FFFF00" |transit

|1128{{±|7}}

|1.313{{±|0.068|0.071}}

|6134{{±|50}}

|

|0.43{{±|0.13}}

|1.187{{±|0.032|0.031}}

|4.0664428{{±|0.0000058}}

|0.04823{{±|0.00075|0.00079}}

|1074{{±|19|16}}

| style="background:#FFFF00" |transit

|668.7{{±|1.3}}

|0.905{{±|0.043|0.044}}

|5281{{±|86|76}}

|

|0.45{{±|0.09}}

|1.50{{±|0.19}}

|2.9223{{±|0.00015}}

|

|

| style="background:#FFFF00" |transit

|2258{{±|16}}

|1.538{{±|0.049}}

|6000{{±|100}}

|

|0.794{{±|0.039|0.040}}

|1.183{{±|0.064|0.045}}

|2.8807198{{±|0.0000028|0.0000027}}

|0.04036{{±|0.00074|0.00082}}

|1395{{±|25|22}}

| style="background:#FFFF00" |transit

|579.5{{±|1.8}}

|1.056{{±|0.059|0.063}}

|5640{{±|89|82}}

|

|0.0261{{±|0.0252|0.0126}}

|0.252{{±|0.057}}

|1.15890{{±|0.00001|0.00002}}

|0.0164{{±|0.0015|0.0029}}

|861{{±|64|103}}

| style="background:#FFFF00" |transit

|262.9{{±|0.3}}

|0.452{{±|0.090}}

|3400{{±|100}}

|{{citation|arxiv=2206.10643|year=2022|title=A hot sub-Neptune in the desert and a temperate super-Earth around faint M dwarfs|doi=10.1051/0004-6361/202243731 |last1=Esparza-Borges |first1=E. |last2=Parviainen |first2=H. |last3=Murgas |first3=F. |last4=Pallé |first4=E. |last5=Maas |first5=A. |last6=Morello |first6=G. |last7=Zapatero-Osorio |first7=M. R. |last8=Barkaoui |first8=K. |last9=Narita |first9=N. |last10=Fukui |first10=A. |last11=Casasayas-Barris |first11=N. |last12=Oshagh |first12=M. |last13=Crouzet |first13=N. |last14=Galán |first14=D. |last15=Fernández |first15=G. E. |last16=Kagetani |first16=T. |last17=Kawauchi |first17=K. |last18=Kodama |first18=T. |last19=Korth |first19=J. |last20=Kusakabe |first20=N. |last21=Laza-Ramos |first21=A. |last22=Luque |first22=R. |last23=Livingston |first23=J. |last24=Madrigal-Aguado |first24=A. |last25=Mori |first25=M. |last26=Orell-Miquel |first26=J. |last27=Puig-Subirà |first27=M. |last28=Stangret |first28=M. |last29=Terada |first29=Y. |last30=Watanabe |first30=N. |journal=Astronomy & Astrophysics |volume=666 |pages=A10 |s2cid=249926978 |display-authors=1 }}

|3.29{{±|1.88|0.82}}

|1.072{{±|0.044|0.043}}

|225.11757{{±|0.00027|0.00025}}

|0.771{{±|0.013}}

|349{{±|10}}

| style="background:#FFFF00" |transit

|1131{{±|12}}

|1.218{{±|0.054|0.048}}

|6096{{±|32}}

|Highly eccentric orbit{{citation|arxiv=2208.10854|year=2023|title=TOI-4562b: A Highly Eccentric Temperate Jupiter Analog Orbiting a Young Field Star|last1=Heitzmann |first1=Alexis |last2=Zhou |first2=George |last3=Quinn |first3=Samuel N. |last4=Huang |first4=Chelsea X. |last5=Dong |first5=Jiayin |last6=Bouma |first6=Luke G. |last7=Dawson |first7=Rebekah I. |last8=Marsden |first8=Stephen C. |last9=Wright |first9=Duncan |last10=Petit |first10=Pascal |last11=Collins |first11=Karen A. |last12=Barkaoui |first12=Khalid |last13=Wittenmyer |first13=Robert A. |last14=Gillen |first14=Edward |last15=Brahm |first15=Rafael |last16=Hobson |first16=Melissa |last17=Hellier |first17=Coel |last18=Ziegler |first18=Carl |last19=Briceño |first19=César |last20=Law |first20=Nicholas |last21=Mann |first21=Andrew W. |last22=Howell |first22=Steve B. |last23=Gnilka |first23=Crystal L. |last24=Littlefield |first24=Colin |last25=Latham |first25=David W. |last26=Lissauer |first26=Jack J. |last27=Newton |first27=Elisabeth R. |last28=Krolikowski |first28=Daniel M. |last29=Kerr |first29=Ronan |last30=Rampalli |first30=Rayna |journal=The Astronomical Journal |volume=165 |issue=3 |page=121 |doi=10.3847/1538-3881/acb5a2 |bibcode=2023AJ....165..121H |s2cid=251741424 |display-authors=1 |doi-access=free }}

|0.53{{±|0.05}}

|0.94{{±|0.09|0.12}}

|31.034{{±|0.001}}

|

|

| style="background:#FFFF00" |transit

|1242

|1.34{{±|0.06}}

|5190{{±|100}}

|Evolved star, eccentric planetary orbit{{citation|arxiv=2210.17062|year=2023|title=TESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period−Eccentricity Relation for Giant Planets Transiting Evolved Stars|last1=Grunblatt |first1=Samuel K. |last2=Saunders |first2=Nicholas |last3=Chontos |first3=Ashley |last4=Hattori |first4=Soichiro |last5=Veras |first5=Dimitri |last6=Huber |first6=Daniel |last7=Angus |first7=Ruth |last8=Rice |first8=Malena |last9=Breivik |first9=Katelyn |last10=Blunt |first10=Sarah |last11=Giacalone |first11=Steven |last12=Lubin |first12=Jack |last13=Isaacson |first13=Howard |last14=Howard |first14=Andrew W. |last15=Ciardi |first15=David R. |last16=Safonov |first16=Boris S. |last17=Strakhov |first17=Ivan A. |last18=Latham |first18=David W. |last19=Bieryla |first19=Allyson |last20=Ricker |first20=George R. |last21=Jenkins |first21=Jon M. |last22=Tenenbaum |first22=Peter |last23=Shporer |first23=Avi |last24=Morgan |first24=Edward H. |last25=Kostov |first25=Veselin |last26=Osborn |first26=Hugh P. |last27=Dragomir |first27=Diana |last28=Seager |first28=Sara |last29=Vanderspek |first29=Roland K. |last30=Winn |first30=Joshua N. |journal=The Astronomical Journal |volume=165 |issue=2 |page=44 |doi=10.3847/1538-3881/aca670 |bibcode=2023AJ....165...44G |s2cid=253237700 |doi-access=free }}

|2.31{{±|0.32|0.33}}

|1.110{{±|0.050}}

|4.280880{{±|0.000022|0.000023}}

|0.0555{{±|0.0011|0.0012}}

|1472{{±|26|24}}

| style="background:#FFFF00" |transit

|1051{{±|6}}

|1.242{{±|0.072|0.077}}

|6058{{±|99|94}}

|

|3.26{{±|0.18|0.17}}

|1.06{{±|0.04}}

|20.33003{{±|0.00007}}

|0.158{{±|0.006}}

|906{{±|13}}

| style="background:#FFFF00" |transit

|1272.336{{±|11}}

|1.24{{±|0.07}}

|6300{{±|80}}

|

|{{Val|0.07801}}

|{{Val|0.47667}}

|{{Val|12.214}}

|

|

| style="background:#FFFF00" |transit

|

|{{Val|1.0|0.125}}

|

|{{Cite encyclopedia |title=The Extrasolar Planet Encyclopaedia — TOI-5174 b |url=https://exoplanet.eu/catalog/toi_5174_b--8418/ |access-date=2023-01-16 |encyclopedia=Extrasolar Planets Encyclopaedia |date=3 December 1995 }}{{Cite web |title=Exoplanet-catalog |url=https://exoplanets.nasa.gov/exoplanet-catalog/8659/toi-5174-b/#:~:text=TOI-5174%20b%20is%20a,discovery%20was%20announced%20in%202022. |access-date=2023-01-16 |website=Exoplanet Exploration: Planets Beyond our Solar System |language=en}}

|1.08{{±|0.06}}

|1.03{{±|0.03}}

|1.630757{{±|0.000001}}

|0.0199{{±|0.0002}}

|737{{±|15}}

| style="background:#FFFF00" |transit

|283.35{{±|0.16}}

|0.392{{±|0.015}}

|3430{{±|54}}

|{{citation|arxiv=2209.11160|year=2023|title=TOI-5205b: A Short-period Jovian Planet Transiting a Mid-M Dwarf|last1=Kanodia |first1=Shubham |last2=Mahadevan |first2=Suvrath |last3=Libby-Roberts |first3=Jessica |last4=Stefansson |first4=Gudmundur |last5=Canas |first5=Caleb I. |last6=Piette |first6=Anjali A. A. |last7=Boss |first7=Alan |last8=Teske |first8=Johanna |last9=Chambers |first9=John |last10=Zeimann |first10=Greg |last11=Monson |first11=Andrew |last12=Robertson |first12=Paul |last13=Ninan |first13=Joe P. |last14=Lin |first14=Andrea S. J. |last15=Bender |first15=Chad F. |last16=Cochran |first16=William D. |last17=Diddams |first17=Scott A. |last18=Gupta |first18=Arvind F. |last19=Halverson |first19=Samuel |last20=Hawley |first20=Suzanne |last21=Kobulnicky |first21=Henry A. |last22=Metcalf |first22=Andrew J. |last23=Parker |first23=Brock A. |last24=Powers |first24=Luke |last25=Ramsey |first25=Lawrence W. |last26=Roy |first26=Arpita |last27=Schwab |first27=Christian |last28=Swaby |first28=Tera N. |last29=Terrien |first29=Ryan C. |last30=Wisniewski |first30=John |journal=The Astronomical Journal |volume=165 |issue=3 |page=120 |doi=10.3847/1538-3881/acabce |bibcode=2023AJ....165..120K |s2cid=257050897 |doi-access=free }}

|1.32{{±|0.10}}

|1.009{{±|0.036|0.035}}

|75.12375{{±|0.00019|0.00018}}

|0.332{{±|0.016}}

|441{{±|48|74}}

| style="background:#FFFF00" |transit

|1154{{±|12}}

|0.890{{±|0.056|0.031}}

|5700{{±|80}}

|{{citation|arxiv=2209.14830|year=2022|title=An old warm Jupiter orbiting the metal-poor G-dwarf TOI-5542|last1=Grieves |first1=Nolan |last2=Bouchy |first2=François |last3=Ulmer-Moll |first3=Solène |last4=Gill |first4=Samuel |last5=Anderson |first5=David R. |last6=Psaridi |first6=Angelica |last7=Lendl |first7=Monika |last8=Stassun |first8=Keivan G. |last9=Jenkins |first9=Jon M. |last10=Burleigh |first10=Matthew R. |last11=Acton |first11=Jack S. |last12=Boyd |first12=Patricia T. |last13=Casewell |first13=Sarah L. |last14=Eigmüller |first14=Philipp |last15=Goad |first15=Michael R. |last16=Goeke |first16=Robert F. |last17=Günther |first17=Maximilian N. |last18=Hawthorn |first18=Faith |last19=Henderson |first19=Beth A. |last20=Henze |first20=Christopher E. |last21=Jordán |first21=Andrés |last22=Kendall |first22=Alicia |last23=Mishra |first23=Lokesh |last24=Moldovan |first24=Dan |last25=Moyano |first25=Maximiliano |last26=Osborn |first26=Hugh |last27=Revol |first27=Alexandre |last28=Sefako |first28=Ramotholo R. |last29=Tilbrook |first29=Rosanna H. |last30=Udry |first30=Stéphane |journal=Astronomy & Astrophysics |volume=668 |pages=A29 |doi=10.1051/0004-6361/202244077 |bibcode=2022A&A...668A..29G |s2cid=252595745 |display-authors=1 }}

|0.69{{±|0.47|0.43}}

|1.41{{±|0.14}}

|5.616531{{±|0.000023}}

|0.066{{±|0.007}}

|961.5{{±|8}}

| style="background:#FFFF00" |transit

|20{{±|60}}

|1.32{{±|0.09}}

|4200{{±|140}}

|

|0.33{{±|0.02}}

|

|691.90{{±|8.77|8.61}}

|1.22{{±|0.02}}

|

| style="background:#00FF00" |radial vel.

|50.512{{±|0.016}}

|0.498{{±|0.019}}

|3734{{±|54}}

|{{citation|arxiv=2203.16504|year=2022|title=The CARMENES search for exoplanets around M dwarfs|last1=Quirrenbach |first1=A. |last2=Passegger |first2=V. M. |last3=Trifonov |first3=T. |last4=Amado |first4=P. J. |last5=Caballero |first5=J. A. |last6=Reiners |first6=A. |last7=Ribas |first7=I. |last8=Aceituno |first8=J. |last9=Bejar |first9=V. J. S. |last10=Chaturvedi |first10=P. |last11=Gonzalez-Cuesta |first11=L. |last12=Henning |first12=T. |last13=Herrero |first13=E. |last14=Kaminski |first14=A. |last15=Kuerster |first15=M. |last16=Lalitha |first16=S. |last17=Lodieu |first17=N. |last18=Lopez-Gonzalez |first18=M. J. |last19=Montes |first19=D. |last20=Palle |first20=E. |last21=Perger |first21=M. |last22=Pollacco |first22=D. |last23=Reffert |first23=S. |last24=Rodriguez |first24=E. |last25=Rodriguez Lopez |first25=C. |last26=Shan |first26=Y. |last27=Tal-Or |first27=L. |last28=Zapatero Osorio |first28=M. R. |last29=Zechmeister |first29=M. |journal=Astronomy & Astrophysics |volume=663 |pages=A48 |doi=10.1051/0004-6361/202142915 |s2cid=247835988 }}

|0.165{{±|0.009}}

|

|1.011534{{±|0.000005}}

|0.0182{{±|0.0003}}

|

|style="background:#FFFF00"|transit

|390

|0.782{{±|0.034}}

|4714{{±|87|88}}

|{{citation|arxiv=2205.02501|year=2022|title=The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 B|last1=Hord |first1=Benjamin J. |last2=Colón |first2=Knicole D. |last3=Berger |first3=Travis A. |last4=Kostov |first4=Veselin |last5=Silverstein |first5=Michele L. |last6=Stassun |first6=Keivan G. |last7=Lissauer |first7=Jack J. |last8=Collins |first8=Karen A. |last9=Schwarz |first9=Richard P. |last10=Sefako |first10=Ramotholo |last11=Ziegler |first11=Carl |last12=Briceño |first12=César |last13=Law |first13=Nicholas |last14=Mann |first14=Andrew W. |last15=Ricker |first15=George R. |last16=Latham |first16=David W. |last17=Seager |first17=Sara |last18=Winn |first18=Joshua N. |last19=Jenkins |first19=Jon M. |last20=Bouma |first20=Luke G. |last21=Falk |first21=Ben |last22=Torres |first22=Guillermo |last23=Twicken |first23=Joseph D. |last24=Vanderburg |first24=Andrew |journal=The Astronomical Journal |volume=164 |issue=1 |page=13 |doi=10.3847/1538-3881/ac6f57 |bibcode=2022AJ....164...13H |s2cid=248524687 |doi-access=free }}