List of exoplanets discovered in 2023

!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

|0.9120{{±|0.0880|0.1430}}

|

|2051.62{{±|45.98|40.47}}

|3.929{{+-|0.058|0.052}}

|

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

|270.58326 ±2.36023

|1.92{{+-|0.07|0.08}}

|4809

|{{Cite arXiv |last1=Teng |first1=Huan-Yu |last2=Sato |first2=Bun'ei |last3=Kuzuhara |first3=Masayuki |last4=Takarada |first4=Takuya |last5=Omiya |first5=Masashi |last6=Harakawa |first6=Hiroki |last7=Izumiura |first7=Hideyuki |last8=Kambe |first8=Eiji |last9=Yilmaz |first9=Mesut |last10=Bikmaev |first10=Ilfan |last11=Selam |first11=Selim O. |last12=Brandt |first12=Timothy D. |last13=Xiao |first13=Guang-Yao |last14=Yoshida |first14=Michitoshi |last15=Itoh |first15=Yoichi |date=2023 |title=Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars |class=astro-ph.EP |eprint=2308.05343}}

|3.2{{±|0.7|0.6}}

|

|8030 ±1800

|8.4{{±|1.1|1.3}}

|1400 ±300

| style="background:#FF6CDA" |imaging

|87.562 ±0.046

|1.20 ±0.06

|6130 ±60

|Host star also known as HD 35850{{cite journal |last1=Franson |first1=Kyle |last2=Bowler |first2=Brendan P. |last3=Zhou |first3=Yifan |last4=Pearce |first4=Tim D. |last5=Bardalez Gagliuffi |first5=Daniella C. |last6=Biddle |first6=Lauren |last7=Brandt |first7=Timothy D. |last8=Crepp |first8=Justin R. |last9=Dupuy |first9=Trent J. |last10=Faherty |first10=Jacqueline |last11=Jensen-Clem |first11=Rebecca |last12=Morgan |first12=Marvin |last13=Sanghi |first13=Aniket |last14=Theissen |first14=Christopher A. |last15=Tran |first15=Quang H. |last16=Wolf |first16=Trevor A. |date=February 2023 |title=Astrometric Accelerations as Dynamical Beacons: A Giant Planet Imaged Inside the Debris Disk of the Young Star AF Lep |journal=The Astrophysical Journal Letters |volume=950 |issue=2 |pages=L19 |doi=10.3847/2041-8213/acd6f6 |arxiv=2302.05420 |bibcode=2023ApJ...950L..19F |s2cid=256808203 |doi-access=free}}{{cite journal |last1=De Rosa |first1=Robert J. |last2=Nielsen |first2=Eric L. |last3=Wahhaj |first3=Zahed |last4=Ruffio |first4=Jean-Baptise |last5=Kalas |first5=Paul G. |last6=Peck |first6=Anne E. |last7=Hirsch |first7=Lea A. |last8=Roberson |first8=William |date=February 2023 |title=Direct imaging discovery of a super-Jovian around the young Sun-like star AF Leporis |journal=Astronomy & Astrophysics |volume=672 |issue= |pages=A94 |doi=10.1051/0004-6361/202345877 |arxiv=2302.06332 |bibcode=2023A&A...672A..94D |s2cid=256827414}}{{cite journal |last1=Mesa |first1=D. |last2=Gratton |first2=R. |display-authors=etal |date=February 2023 |title=AF Lep b: the lowest mass planet detected coupling astrometric and direct imaging data |journal=Astronomy & Astrophysics |volume=672 |issue= |pages=A93 |doi=10.1051/0004-6361/202345865 |arxiv=2302.06213 |bibcode=2023A&A...672A..93M |s2cid=256827302}}

|0.00331 ±0.00161

|

|12.73596 ±0.00793

|0.1108 ±0.0020

|459{{±|13|12}}

| style="background:#FFFF00" |transit

|32

|0.510{{±|0.028|0.027}}

|3678{{±|90|88}}

|Potentially rocky super-Earth.{{Cite journal |last1=Wittrock |first1=Justin M. |last2=Plavchan |first2=Peter P. |last3=Cale |first3=Bryson L. |last4=Barclay |first4=Thomas |last5=Ludwig |first5=Mathis R. |last6=Schwarz |first6=Richard P. |last7=Mékarnia |first7=Djamel |last8=J. Triaud |first8=Amaury H. M. |last9=Abe |first9=Lyu |last10=Suarez |first10=Olga |last11=Guillot |first11=Tristan |last12=Conti |first12=Dennis M. |last13=Collins |first13=Karen A. |last14=Waite |first14=Ian A. |last15=Kielkopf |first15=John F. |date=2023-12-01 |title=Validating AU Microscopii d with Transit Timing Variations |journal=The Astronomical Journal |volume=166 |issue=6 |pages=232 |doi=10.3847/1538-3881/acfda8 |arxiv=2302.04922 |bibcode=2023AJ....166..232W |doi-access=free|issn=0004-6256}}{{Cite web |title=AU Microscopii d - Exoplanet-catalog |url=https://exoplanets.nasa.gov/exoplanet-catalog/9050/au-microscopii-d/ |access-date=2023-12-03 |website=Exoplanet Exploration: Planets Beyond our Solar System |language=en |archive-date=3 December 2023 |archive-url=https://web.archive.org/web/20231203192423/https://exoplanets.nasa.gov/exoplanet-catalog/9050/au-microscopii-d/ |url-status=live }}

|0.7 ±0.1

|

|1891{{±|56|48}}

|2.63{{±|0.06|0.05}}

|

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

|77.4046{{±|0.0744|0.0740}}

|0.679 ±0.017

|4051 ±239

|{{Cite journal |last1=Frensch |first1=Y. G. C. |last2=Curto |first2=G. Lo |last3=Bouchy |first3=F. |last4=Mayor |first4=M. |last5=Hébrard |first5=G. |last6=Lovis |first6=C. |last7=Moutou |first7=C. |last8=Pepe |first8=F. A. |last9=Queloz |first9=D. |last10=Santos |first10=N. |last11=Segransan |first11=D. |last12=Udry |first12=S. |last13=Unger |first13=N. |date=2023-07-01 |title=The HARPS search for southern extra-solar planets - XLVII. Five Jupiter-mass planets in long-period orbits, one highly irradiated Neptune, one brown dwarf, and five stellar binaries |url=https://www.aanda.org/articles/aa/abs/2023/07/aa46203-23/aa46203-23.html |journal=Astronomy & Astrophysics |language=en |volume=675 |pages=A173 |doi=10.1051/0004-6361/202346203 |arxiv=2306.04420 |bibcode=2023A&A...675A.173F |s2cid=265829649 |issn=0004-6361 |access-date=26 July 2023 |archive-date=16 December 2023 |archive-url=https://web.archive.org/web/20231216084516/https://www.aanda.org/articles/aa/abs/2023/07/aa46203-23/aa46203-23.html |url-status=live }}

|2.4{{+-|1.5|0.7}}

|

|6360{{±|6260|711}}

|5.9{{±|3.4|0.5}}

|

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

|77.4046{{±|0.0744|0.0740}}

|0.679 ±0.017

|4051 ±239

|

|0.0384{{+-|0.0057|0.0060}}

|

|3.4982{{+-|0.0022|0.2327}}

|

|

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

|82.6101{{+-|0.1246|0.1239}}

|1.25 ±0.02

|6400 ±50

|{{Cite journal |last1=Barnes |first1=J R |last2=Standing |first2=M R |last3=Haswell |first3=C A |last4=Staab |first4=D |last5=Doherty |first5=J P J |last6=Waller-Bridge |first6=M |last7=Fossati |first7=L |last8=Soto |first8=M |last9=Anglada-Escudé |first9=G |last10=Llama |first10=J |last11=McCune |first11=C |last12=Lewis |first12=F W |date=2023-07-29 |title=DMPP-4: candidate sub-Neptune mass planets orbiting a naked-eye star |url=https://academic.oup.com/mnras/article/524/4/5196/7224603 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=524 |issue=4 |pages=5196–5212 |doi=10.1093/mnras/stad2109 |issn=0035-8711 |doi-access=free |access-date=26 August 2023 |archive-date=26 August 2023 |archive-url=https://web.archive.org/web/20230826155414/https://academic.oup.com/mnras/article/524/4/5196/7224603 |url-status=live |arxiv=2307.07530 }}

|0.0327{{±|0.0050|0.0047}}

|0.2080{{±|0.0071|0.0084}}

|16.141132 ±0.000019

|0.1237 ±0.0017

|804 ±10

| style="background:#FFFF00" |transit

|398.255{{+-|2.867|2.825}}

|0.970 ±0.040

|5868 ±60

|{{Cite journal |last1=Bonomo |first1=A. S. |last2=Dumusque |first2=X. |last3=Massa |first3=A. |last4=Mortier |first4=A. |last5=Bongiolatti |first5=R. |last6=Malavolta |first6=L. |last7=Sozzetti |first7=A. |last8=Buchhave |first8=L. A. |last9=Damasso |first9=M. |last10=Haywood |first10=R. D. |last11=Morbidelli |first11=A. |last12=Latham |first12=D. W. |last13=Molinari |first13=E. |last14=Pepe |first14=F. |last15=Poretti |first15=E. |date=2023 |title=Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities |journal=Astronomy & Astrophysics |volume=677 |pages=A33 |doi=10.1051/0004-6361/202346211 |arxiv=2304.05773|bibcode=2023A&A...677A..33B |s2cid=258078829 }}

|0.0673{{±|0.0107|0.0101}}

|

|241.8{{+-|1.3|1.7}}

|0.657{{±|0.026|0.028}}

|

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

|66.96874 ±0.54957

|0.65 ±0.08

|3897 ±71

|{{Cite journal |last1=Pinamonti |first1=M. |last2=Barbato |first2=D. |last3=Sozzetti |first3=A. |last4=Affer |first4=L. |last5=Benatti |first5=S. |last6=Biazzo |first6=K. |last7=Bignamini |first7=A. |last8=Borsa |first8=F. |last9=Damasso |first9=M. |last10=Desidera |first10=S. |last11=Lanza |first11=A. F. |last12=Maldonado |first12=J. |last13=Mancini |first13=L. |last14=Naponiello |first14=L. |last15=Nardiello |first15=D. |date=2023 |title=The GAPS programme at TNG |journal=Astronomy & Astrophysics |volume=677 |pages=A122 |doi=10.1051/0004-6361/202346476 |arxiv=2306.04419|s2cid=259095781 }}

|0.0130 ±0.0011

|

|11.5301 ±0.0078

|

|

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

|30.69986 ±0.00925

|0.455 ±0.011

|3522 ±70

|{{Cite journal|last1=Goffo |first1=Elisa |last2=Gandolfi |first2=Davide |last3=Egger |first3=Jo Ann |last4=Mustill |first4=Alexander J. |last5=Albrecht |first5=Simon H. |last6=Hirano |first6=Teruyuki |last7=Kochukhov |first7=Oleg |last8=Astudillo-Defru |first8=Nicola |last9=Barragan |first9=Oscar |last10=Serrano |first10=Luisa M. |last11=Hatzes |first11=Artie P. |last12=Alibert |first12=Yann |last13=Guenther |first13=Eike |last14=Dai |first14=Fei |last15=Lam |first15=Kristine W. F. |date=2023 |title=Company for the ultra-high density, ultra-short period sub-Earth GJ 367 b: discovery of two additional low-mass planets at 11.5 and 34 days |journal=The Astrophysical Journal |volume=955 |issue=1 |pages=L3 |doi=10.3847/2041-8213/ace0c7 |arxiv=2307.09181|bibcode=2023ApJ...955L...3G |doi-access=free }}

|0.0190 ±0.0015

|

|34.369 ±0.073

|

|

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

|30.69986 ±0.00925

|0.455 ±0.011

|3522 ±70

|

|0.006 ±0.00053

|0.11874 ±0.00205

|0.9263237 ±0.0000009

|0.1406 ±0.0003

|940.0 ±10.0

| style="background:#FFFF00" |transit

|39.348

|0.413 ±0.011

|3600 ±16

|{{cite journal |last1=Palle |first1=E. |last2=Orell-Miquel |first2=J. |display-authors=etal |arxiv=2301.06873 |title=GJ 806 (TOI-4481): A bright nearby multi-planetary system with a transiting hot low-density super-Earth |journal=Astronomy & Astrophysics |date=January 2023|volume=678 |pages=A80 |doi=10.1051/0004-6361/202244261 |bibcode=2023A&A...678A..80P |s2cid=255941564 }} Host star also known as TOI-4481{{Cite encyclopedia |title=The Extrasolar Planet Encyclopaedia — TOI-4481 b |url=https://exoplanet.eu/catalog/toi_4481_b--8583/ |access-date=2023-01-19 |encyclopedia=Extrasolar Planets Encyclopaedia |date=23 October 1995 }}

|0.0182 ±0.0009

|

|6.65064 ±0.00025

|0.0523 ±0.001

|480.0 ±5.0

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

|39.348

|0.413 ±0.011

|3600 ±16

| Host star also known as TOI-4481{{Cite encyclopedia |title=The Extrasolar Planet Encyclopaedia — TOI-4481 c |url=https://exoplanet.eu/catalog/toi_4481_c--8584/ |access-date=2023-01-19 |encyclopedia=Extrasolar Planets Encyclopaedia |date=23 October 1995 }}

|0.03341{{±|0.00412|0.00463}}

|0.29{{Cite web |title=Exoplanet-catalog |url=https://exoplanets.nasa.gov/exoplanet-catalog/8732/gj-1151-c/ |access-date=2023-11-09 |website=Exoplanet Exploration: Planets Beyond our Solar System |language=en |archive-date=9 November 2023 |archive-url=https://web.archive.org/web/20231109051117/https://exoplanets.nasa.gov/exoplanet-catalog/8732/gj-1151-c/ |url-status=live }}

|389.7{{±|5.4|6.5}}

|0.5714{{±|0.0053|0.0064}}

|

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

|26.23 ±0.01

|0.1639 ±0.0093

|3143 ±26

|{{cite journal |last1=Blanco-Pozo |first1=J. |last2=Perger |first2=M. |display-authors=etal |date=March 2023 |title=The CARMENES search for exoplanets around M dwarfs. A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data |journal=Astronomy & Astrophysics |volume=671 |issue= |pages=A50 |doi=10.1051/0004-6361/202245053 |arxiv=2301.04442 |bibcode=2023A&A...671A..50B|s2cid=265978783 }} Planet on 2-day orbit was suspected but refuted in 2021{{cite journal |display-authors=1 |arxiv=2102.02233|year=2021|title=The Habitable-zone Planet Finder Detects a Terrestrial-mass Planet Candidate Closely Orbiting Gliese 1151: The Likely Source of Coherent Low-frequency Radio Emission from an Inactive Star|author1-link=Suvrath Mahadevan|last1=Mahadevan|first1=Suvrath|last2=Stefánsson|first2=Guðmundur|last3=Robertson|first3=Paul|last4=Terrien|first4=Ryan C.|last5=Ninan|first5=Joe P.|last6=Holcomb|first6=Rae J.|last7=Halverson|first7=Samuel|last8=Cochran|first8=William D.|last9=Kanodia|first9=Shubham|last10=Ramsey|first10=Lawrence W.|last11=Wolszczan|first11=Alexander|last12=Endl|first12=Michael|last13=Bender|first13=Chad F.|last14=Diddams|first14=Scott A.|last15=Fredrick|first15=Connor|last16=Hearty|first16=Fred|last17=Monson|first17=Andrew|last18=Metcalf|first18=Andrew J.|last19=Roy|first19=Arpita|last20=Schwab|first20=Christian|journal=The Astrophysical Journal Letters |volume=919 |issue=1 |pages=L9 |doi=10.3847/2041-8213/abe2b2 |bibcode=2021ApJ...919L...9M |s2cid=231802021 |doi-access=free }}{{cite journal|display-authors=1|arxiv=2103.10216|year=2021|title=The CARMENES search for exoplanets around M dwarfs|doi=10.1051/0004-6361/202140786|last1=Perger|first1=M.|last2=Ribas|first2=I.|last3=Anglada-Escudé|first3=G.|last4=Morales|first4=J. C.|last5=Amado|first5=P. J.|last6=Caballero|first6=J. A.|last7=Quirrenbach|first7=A.|last8=Reiners|first8=A.|last9=Béjar|first9=V. J. S.|last10=Dreizler|first10=S.|last11=Galadí-Enríquez|first11=D.|last12=Hatzes|first12=A. P.|last13=Henning|first13=Th.|last14=Jeffers|first14=S. V.|last15=Kaminski|first15=A.|last16=Kürster|first16=M.|last17=Lafarga|first17=M.|last18=Montes|first18=D.|last19=Pallé|first19=E.|last20=Rodríguez-López|first20=C.|last21=Schweitzer|first21=A.|last22=Zapatero Osorio|first22=M. R.|last23=Zechmeister|first23=M.|journal=Astronomy & Astrophysics|volume=649|pages=L12|bibcode=2021A&A...649L..12P |s2cid=232269942}}

|0.0116 ±0.0013

|

|6.9442 ±0.0010

|0.0405{{+-|0.0011|0.0012}}

|

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

|32.32369 ±0.01357

|0.1842 ±0.0153

|3273 ±101

|{{Cite journal |last1=Gorrini |first1=P. |last2=Kemmer |first2=J. |last3=Dreizler |first3=S. |last4=Burn |first4=R. |last5=Hirano |first5=T. |last6=Pozuelos |first6=F. J. |last7=Kuzuhara |first7=M. |last8=Caballero |first8=J. A. |last9=Amado |first9=P. J. |last10=Harakawa |first10=H. |last11=Kudo |first11=T. |last12=Quirrenbach |first12=A. |last13=Reiners |first13=A. |last14=Ribas |first14=I. |last15=Béjar |first15=V. J. S. |date=December 2023 |title=Planetary companions orbiting the M dwarfs GJ 724 and GJ 3988: A CARMENES and IRD collaboration |url=https://www.aanda.org/articles/aa/pdf/2023/12/aa47108-23.pdf |journal=Astronomy & Astrophysics |volume=680 |pages=A28 |doi=10.1051/0004-6361/202347108 |arxiv=2310.05599 |bibcode=2023A&A...680A..28G |issn=0004-6361}}

|0.0374 ±0.0060

|

|13.4586{{±|0.0044|0.0067}}

|0.0943 ±0.0036

|

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

|77.8988{{±|0.0828|0.0825}}

|0.62 ±0.07

|

|{{Cite journal |last1=Baycroft |first1=Thomas A. |last2=Badnell |first2=Harry |last3=Blacker |first3=Samuel |last4=Triaud |first4=Amaury H. M. J. |date=2023-08-01 |title=GJ 9404 b: A Confirmed Eccentric Planet, and not a Candidate |journal=Research Notes of the American Astronomical Society |volume=7 |issue=8 |pages=175 |doi=10.3847/2515-5172/acefc5 |arxiv=2308.12309 |bibcode=2023RNAAS...7..175B |issn=2515-5172 |doi-access=free }}

|10.7{{±|5.2|2.2}}

|

|8500{{±|2600|1500}}

|

|

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

|416.744{{±|1.386|1.380}}

|1.33 ±0.03

|6412.830{{±|102.682|110.120}}

|Also known as HD 147506 c{{Cite journal |last1=de Beurs |first1=Zoë L. |last2=de Wit |first2=Julien |last3=Venner |first3=Alexander |last4=Berardo |first4=David |last5=Bryan |first5=Jared |last6=Winn |first6=Joshua N. |last7=Fulton |first7=Benjamin J. |last8=Howard |first8=Andrew W. |date=2023-10-01 |title=Revisiting Orbital Evolution in HAT-P-2 b and Confirmation of HAT-P-2 c |journal=The Astronomical Journal |volume=166 |issue=4 |pages=136 |doi=10.3847/1538-3881/acedf1 |arxiv=2309.03256 |bibcode=2023AJ....166..136D |doi-access=free|issn=0004-6256}}

|28.26{{+-|2.05|2.17}}

|

|663.87{{+-|4.61|4.31}}

|2.03 ±0.01

|

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

|199.36184 ±9.26130

|2.49

|3802

|Host star also known as Mirach{{Cite journal |last1=Lee |first1=Byeong-Cheol |last2=Do |first2=Hee-Jin |last3=Park |first3=Myeong-Gu |last4=Lim |first4=Beomdu |last5=Choi |first5=Yeon-Ho |last6=Koo |first6=Jae-Rim |last7=Bang |first7=Tae-Yang |last8=Oh |first8=Hyeong-Ill |last9=Han |first9=Inwoo |last10=Chang |first10=Heon-Young |date=2023 |title=Long-period radial velocity variations of nine M red giants: The detection of sub-stellar companions around HD 6860 and HD 112300 |journal=Astronomy and Astrophysics |volume=678 |doi=10.1051/0004-6361/202243725 |arxiv=2307.15897|bibcode=2023A&A...678A.106L |s2cid=260334453 }}

|0.0340{{±|0.0085}}

|0.219{{±|0.008}}

|5.254467{{±|0.000009}}

|0.059{{±|0.001}}

|1194{{±|28}}

| style="background:#FFFF00" |transit

|220.548{{±|0.670|0.665}}

|1.00{{±|0.06}}

|5920{{±|110}}

|Also known as TOI-1473 b{{cite journal|last=Akana Murphy|first=Joseph M.|collaboration=48|date=8 September 2023|title=The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight Systems|journal=The Astronomical Journal|volume=166|issue=4|page=153|doi=10.3847/1538-3881/ace2ca|doi-access=free |arxiv=2306.16587 |bibcode=2023AJ....166..153A }}

|

|0.200 ±0.007

|10.924709 ±0.000032

|0.200 ±0.007

|668 ±13

| style="background:#FFFF00" |transit

|148.6035{{+-|0.2880|0.2870}}

|0.790{{+-|0.020|0.036}}

|4757 ±89

|{{Cite journal |last1=Tuson |first1=Amy |last2=Queloz |first2=Didier |last3=Osborn |first3=Hugh P. |last4=Wilson |first4=Thomas G. |last5=Hooton |first5=Matthew J. |last6=Beck |first6=Mathias |last7=Lendl |first7=Monika |last8=Olofsson |first8=Göran |last9=Fortier |first9=Andrea |last10=Bonfanti |first10=Andrea |last11=Brandeker |first11=Alexis |last12=Buchhave |first12=Lars A. |last13=Cameron |first13=Andrew Collier |last14=Ciardi |first14=David R. |last15=Collins |first15=Karen A. |date=2023 |title=TESS and CHEOPS discover two warm sub-Neptunes transiting the bright K-dwarf HD 15906 |journal=Monthly Notices of the Royal Astronomical Society |volume=523 |issue=2 |pages=3090–3118 |doi=10.1093/mnras/stad1369 |doi-access=free |arxiv=2306.04511}}

|

|0.261{{+-|0.006|0.005}}

|21.583298{{+-|0.000052|0.000055}}

|0.141{{+-|0.002|0.001}}

|532 ±10

| style="background:#FFFF00" |transit

|148.6035{{+-|0.2880|0.2870}}

|0.790{{+-|0.020|0.036}}

|4757 ±89

|

|21 ±1

|

|803 ±5

|2.1 ±0.1

|

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

|731.066{{+-|29.409|27.254}}

|1.84 ±0.09

|3860 ±100

|{{cite journal |last1=Lee |first1=Byeong-Cheol |last2=Koo |first2=Jae-Rim |last3=Jeong |first3=Gwanghui |last4=Park |first4=Myeong-Gu |last5=Han |first5=Inwoo |last6=Choi |first6=Yeon-Ho |title=A Search for Exoplanets around Northern Circumpolar Stars VII. Detection of Planetary Companion Orbiting the Largest Host Star HD 18438 |journal=Journal of Korean Astronomical Society |date=1 March 2023 |volume=56 |issue=1 |pages=35–40 |doi=10.5303/JKAS.2023.56.1.35 |arxiv=2303.08357 |bibcode=2023JKAS...56...35L |s2cid=257532879 |url=https://ui.adsabs.harvard.edu/abs/2023JKAS...56...35L/abstract |issn=1225-4614 |access-date=10 September 2023 |archive-date=6 October 2023 |archive-url=https://web.archive.org/web/20231006045920/https://ui.adsabs.harvard.edu/abs/2023JKAS...56...35L/abstract |url-status=live }}

|<0.08360

|0.2326 ±0.0054

|47.42489{{+-|0.00010|0.00011}}

|0.2958{{+-|0.0044|0.0042}}

|546 ±6

| style="background:#FFFF00" |transit

|204.7581{{+-|0.3787|0.3370}}

|1.098{{+-|0.040|0.039}}

|6169 ±64

|{{Cite journal |last1=Garai |first1=Z. |last2=Osborn |first2=H. P. |last3=Gandolfi |first3=D. |last4=Brandeker |first4=A. |last5=Sousa |first5=S. G. |last6=Lendl |first6=M. |last7=Bekkelien |first7=A. |last8=Broeg |first8=C. |last9=Cameron |first9=A. Collier |last10=Egger |first10=J. A. |last11=Hooton |first11=M. J. |last12=Alibert |first12=Y. |last13=Delrez |first13=L. |last14=Fossati |first14=L. |last15=Salmon |first15=S. |date=2023-06-01 |title=Refined parameters of the HD 22946 planetary system and the true orbital period of planet d★ |url=https://ui.adsabs.harvard.edu/abs/2023A%26A...674A..44G |journal=Astronomy and Astrophysics |volume=674 |pages=A44 |doi=10.1051/0004-6361/202345943 |arxiv=2306.04468 |bibcode=2023A&A...674A..44G |s2cid=259095617 |issn=0004-6361 |access-date=1 January 2024 |archive-date=16 December 2023 |archive-url=https://web.archive.org/web/20231216013133/https://ui.adsabs.harvard.edu/abs/2023A%26A...674A..44G |url-status=live }}

|0.0267{{±|0.0098}}

|0.234{{±|0.014}}

|7.049144{{±|0.000009}}

|0.076{{±|0.002}}

|1290{{±|41}}

| style="background:#FFFF00" |transit

|148.786{{±|0.409|0.407}}

|1.19{{±|0.07}}

|6220{{±|110}}

|Also known as TOI-554 b.

|<0.013

|0.134{{±|0.011}}

|3.044050{{±|0.000008}}

|0.0435{{±|0.0009}}

|1707{{±|54}}

| style="background:#FFFF00" |transit

|148.786{{±|0.409|0.407}}

|1.19{{±|0.07}}

|6220{{±|110}}

|Also known as TOI-554 c.

|6.6 ±0.5

|

|490 ±3

|1.3 ±0.1

|

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

|682.674{{+-|11.588|11.210}}

|1.14 ±0.15

|3940 ±40

|{{Cite journal |last1=Lee |first1=Byeong-Cheol |last2=Han |first2=Inwoo |last3=Jeong |first3=Gwanghui |last4=Koo |first4=Jae-Rim |last5=Lim |first5=Beomdu |last6=Park |first6=Myeong-Gu |last7=Bang |first7=Tae-Yang |last8=Choi |first8=Yeon-Ho |last9=Choi |first9=Yeon-Ho |last10=Oh |first10=Hyeong-Ill |date=2023-08-22 |title=A Search for Exoplanets around Northern Circumpolar Stars. VIII. Filtering Out a Planet Cycle from the Multi-Period Radial Velocity Variations in M Giant HD 36384 |url=https://doi.org/10.5303/JKAS.2023.56.2.195 |journal=Journal of the Korean Astronomical Society |volume=56 |issue=2 |pages=195–199 |arxiv=2308.05994 |bibcode=2023JKAS...56..195L |doi=10.5303/JKAS.2023.56.2.195}}

|16 ±1

|

|2690{{+-|60|102}}

|3.8 ±0.1

|

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

|119.7253{{+-|0.1833|0.1823}}

|1.00 ±0.05

|

|

|0.07 ±0.01

|

|15.017 ±0.002

|0.121 ±0.001

|

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

|169.8125{{+-|0.2479|0.2472}}

|1.039 ±0.025

|5873 ±19

|

|0.40 ±0.06

|

|3449{{+-|189|210}}

|4.5 ±0.2

|

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

|169.8125{{+-|0.2479|0.2472}}

|1.039 ±0.025

|5873 ±19

|

|5.4{{+-|0.5|0.4}}

|

|4356{{+-|173|112}}

|5.3{{+-|0.2|0.1}}

|

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

|98.9192{{+-|0.1973|0.1970}}

|1.06 ±0.05

|

|

|5.01{{+-|0.79|0.76}}

|

|3441{{+-|18|17}}

|4.761 ±0.042

|

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

|186.9079{{+-|0.3584|0.3568}}

|1.21 ±0.03

|6314 ±65

|{{Cite journal |last1=Xiao |first1=Guang-Yao |last2=Liu |first2=Yu-Juan |last3=Teng |first3=Huan-Yu |last4=Wang |first4=Wei |last5=Brandt |first5=Timothy D. |last6=Zhao |first6=Gang |last7=Zhao |first7=Fei |last8=Zhai |first8=Meng |last9=Gao |first9=Qi |date=2023-05-01 |title=The Masses of a Sample of Radial-velocity Exoplanets with Astrometric Measurements |url=https://iopscience.iop.org/article/10.1088/1674-4527/accb7e |journal=Research in Astronomy and Astrophysics |volume=23 |issue=5 |pages=055022 |doi=10.1088/1674-4527/accb7e |arxiv=2303.12409 |bibcode=2023RAA....23e5022X |s2cid=257663647 |issn=1674-4527}}

|0.53 ±0.03

|

|2164{{+-|21|20}}

|3.48 ±0.03

|

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

|188.4552{{+-|0.3930|0.3911}}

|1.200 ±0.024

|5631 ±21

|

|17.9 ±1.3

|

|95.233{{+-|0.098|0.096}}

|

|

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

|59.3728{{+-|0.1895|0.1882}}

|0.85 ±0.02

|4929 ±44

|Host star also known as 83 Leonis{{Cite journal |last1=Stalport |first1=M. |last2=Cretignier |first2=M. |last3=Udry |first3=S. |last4=John |first4=A. Anna |last5=Wilson |first5=T. G. |last6=Delisle |first6=J. -B. |last7=Bonomo |first7=A. S. |last8=Buchhave |first8=L. A. |last9=Charbonneau |first9=D. |last10=Dalal |first10=S. |last11=Damasso |first11=M. |last12=Di Fabrizio |first12=L. |last13=Dumusque |first13=X. |last14=Fiorenzano |first14=A. |last15=Harutyunyan |first15=A. |date=2023 |title=A review of planetary systems around HD 99492, HD 147379, and HD 190007 with HARPS-N |journal=Astronomy & Astrophysics |volume=678 |pages=A90 |doi=10.1051/0004-6361/202346887 |arxiv=2308.05669|bibcode=2023A&A...678A..90S |s2cid=260775534 }}

|3.0{{±|0.7|0.5}}

|

|2990{{+-|54|51}}

|3.7 ±0.1

|

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

|126.1689{{+-|0.2202|0.2195}}

|0.74 ±0.04

|

|{{Cite journal |last1=Philipot |first1=F. |last2=Lagrange |first2=A. -M. |last3=Kiefer |first3=F. |last4=Rubini |first4=P. |last5=Delorme |first5=P. |last6=Chomez |first6=A. |date=2023 |title=A multi-technique approach to identifying and/Or constraining radial-velocity substellar companions |journal=Astronomy & Astrophysics |volume=678 |pages=A107 |doi=10.1051/0004-6361/202346612 |arxiv=2308.05417|bibcode=2023A&A...678A.107P |s2cid=260775968 }}

|15.83{{±|2.33|2.74}}

|

|466.63{{±|2.33|2.74}}

|1.33{{±|0.08|0.11}}

|

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

|202.45560 ±11.05904

|1.4 ±0.3

|3657

|{{Cite journal|last1=Lee |first1=Byeong-Cheol |last2=Do |first2=Hee-Jin |last3=Park |first3=Myeong-Gu |last4=Lim |first4=Beomdu |last5=Choi |first5=Yeon-Ho |last6=Koo |first6=Jae-Rim |last7=Bang |first7=Tae-Yang |last8=Oh |first8=Hyeong-Ill |last9=Han |first9=Inwoo |last10=Chang |first10=Heon-Young |date=2023 |title=Long-period radial velocity variations of nine M red giants: The detection of sub-stellar companions around HD 6860 and HD 112300 |journal=Astronomy and Astrophysics |volume=678 |doi=10.1051/0004-6361/202243725 |arxiv=2307.15897|bibcode=2023A&A...678A.106L |s2cid=260334453 }} Host star also known as Minelauva or Auva

|2.3{{+-|0.8|0.3}}

|

|4055{{+-|45|44}}

|5.4 ±0.1

|

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

|184.3368{{+-|0.3803|0.3734}}

|1.28 ±0.06

|

|

|0.018{{±|0.007}}

|0.224{{±|0.012}}

|15.92346{{±|0.00002}}

|0.120{{±|0.003}}

|815{{±|27}}

| style="background:#FFFF00" |transit

|240.936{{±|0.469|0.468}}

|0.90{{±|0.06}}

|5710{{±|110}}

|Also known as TOI-1247 b.

|0.267

|

|

|46

|

|style="background:#ba9550"|disk kinematics

|rowspan="4"|330.15{{±|3.85}}

|rowspan="4"|2.041{{±|0.395}}

|rowspan="4"|8291{{±|510}}{{Cite journal |last1=Paegert |first1=M. |last2=Stassun |first2=K. G. |last3=Collins |first3=K. A. |last4=Pepper |first4=J. |last5=Torres |first5=G. |last6=Jenkins |first6=J. |last7=Twicken |first7=J. D. |last8=Latham |first8=D. W. |date=2022-02-01 |title=VizieR Online Data Catalog: TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021) |bibcode=2022yCat.4039....0P |journal=VizieR Online Data Catalog |volume=4039 |pages=IV/39}}

|{{Cite journal |last1=Garrido-Deutelmoser |first1=Juan |last2=Petrovich |first2=Cristobal |last3=Charalambous |first3=Carolina |last4=Guzmán |first4=Viviana V. |last5=Zhang |first5=Ke |date=2023-03-01 |title=A gap-sharing planet pair shaping the crescent in HD 163296: a disk sculpted by a resonant chain |arxiv=2301.13260 |journal=The Astrophysical Journal Letters |volume=945 |issue=2 |pages=L37 |doi=10.3847/2041-8213/acbea8 |doi-access=free |issn=2041-8205}}

|0.189

|

|

|54

|

|style="background:#ba9550"|disk kinematics

|

|0.40

|

|

|84.5

|

|style="background:#ba9550"|disk kinematics

|

|1

|

|

|137

|

|style="background:#ba9550"|disk kinematics

|

|19{{+-|2|1}}

|

|2343 ±2

|3.59{{+-|0.06|0.07}}

|

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

|187.2993{{±|0.0689|0.0684}}

|1.10 ±0.06

|

|

|3.7{{+-|1.6|1.1}}

|

|1804 ±73

|2.9 ±0.1

|

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

|177.1869{{+-|0.9031|0.8940}}

|1.00 ±0.05

|

|

|3 ±2

|

|

|37.2 ±1.5

|

| style="background:#FF6CDA" |imaging

|435.744{{+-|2.717|2.674}}

|1.85

|

|{{Cite journal |last1=Hammond |first1=Iain |last2=Christiaens |first2=Valentin |last3=Price |first3=Daniel J. |last4=Toci |first4=Claudia |last5=Pinte |first5=Christophe |last6=Juillard |first6=Sandrine |last7=Garg |first7=Himanshi |date=2023-06-01 |title=Confirmation and Keplerian motion of the gap-carving protoplanet HD 169142 b |journal=Monthly Notices of the Royal Astronomical Society |volume=522 |issue=1 |pages=L51–L55 |doi=10.1093/mnrasl/slad027 |doi-access=free |arxiv=2302.11302 |bibcode=2023MNRAS.522L..51H |issn=0035-8711 }}

|1.3{{+-|0.3|0.1}}

|

|4060{{+-|148|112}}

|4.6{{+-|0.2|0.1}}

|

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

|102.3967{{+-|0.1778|0.1768}}

|0.80 ±0.04

|

|

|0.0192 ±0.0050

|0.201 ±0.010

|6.441008 ±0.000011

|0.0629 ±0.0011

|743 ±26

| style="background:#FFFF00" |transit

|77.11 ±0.04

|0.80 ±0.04

|4819 ±94

|{{cite journal|arxiv=2303.03775|year=2023|title=The young mini-Neptune HD 207496b that is either a naked core or on the verge of becoming one|last1=Barros |first1=S. C. C. |last2=Demangeon |first2=O. D. S. |last3=Armstrong |first3=D. J. |last4=Delgado Mena |first4=E. |last5=Acuña |first5=L. |author6=J. |last7=Fernández |first7=Fernández |last8=Deleuil |first8=M. |last9=Collins |first9=K. A. |last10=Howell |first10=S. B. |last11=Ziegler |first11=C. |last12=Adibekyan |first12=V. |last13=Sousa |first13=S. G. |last14=Stassun |first14=K. G. |last15=Grieves |first15=N. |last16=Lillo-Box |first16=J. |last17=Hellier |first17=C. |last18=Wheatley |first18=P. J. |last19=Briceño |first19=C. |last20=Collins |first20=K. I. |last21=Hawthorn |first21=F. |last22=Hoyer |first22=S. |last23=Jenkins |first23=J. |last24=Law |first24=N. |last25=Mann |first25=A. W. |last26=Matson |first26=R. A. |last27=Mousis |first27=O. |last28=Nielsen |first28=L. D. |last29=Osborn |first29=A. |last30=Osborn |first30=H. |journal=Astronomy & Astrophysics |volume=673 |pages=A4 |doi=10.1051/0004-6361/202245741 |bibcode=2023A&A...673A...4B |s2cid=257378182 |display-authors=1 }}

|

|0.1824 ±0.0067

|7.4341393 ±0.0000062

|0.0720 ±0.0026

|805{{+-|13|12}}

| style="background:#FFFF00" |transit

|134.2804 ±0.4612

|0.789{{+-|0.022|0.021}}

|5037 ±14

|Host star also known as TOI-1430{{Cite journal |last1=Orell-Miquel |first1=J. |last2=Lampón |first2=M. |last3=López-Puertas |first3=M. |last4=Mallorquín |first4=M. |last5=Murgas |first5=F. |last6=Peláez-Torres |first6=A. |last7=Pallé |first7=E. |last8=Esparza-Borges |first8=E. |last9=Sanz-Forcada |first9=J. |last10=Tabernero |first10=H. M. |last11=Nortmann |first11=L. |last12=Nagel |first12=E. |last13=Parviainen |first13=H. |last14=Osorio |first14=M. R. Zapatero |last15=Caballero |first15=J. A. |date=2023 |title=Confirmation of an He I evaporating atmosphere around the 650-Myr-old sub-Neptune HD 235088 b (TOI-1430 b) with CARMENES |journal=Astronomy & Astrophysics |volume=677 |pages=A56 |doi=10.1051/0004-6361/202346445 |arxiv=2307.05191|bibcode=2023A&A...677A..56O |s2cid=259766771 }}

|0.025{{±|0.006}}

|0.228{{±|0.017}}

|10.75101{{±|0.00006}}

|0.092{{±|0.002}}

|855{{±|28}}

| style="background:#FFFF00" |transit

|331.681{{±|1.373|1.360}}

|0.91{{±|0.06}}

|5530{{±|110}}

|Also known as TOI-266 b.

|0.0296{{±|0.0069}}

|0.221{{±|0.017}}

|19.6053{{±|0.0003}}

|0.138{{±|0.003}}

|699{{±|23}}

| style="background:#FFFF00" |transit

|331.681{{±|1.373|1.360}}

|0.91{{±|0.06}}

|5530{{±|110}}

|Also known as TOI-266 c.

|0.0315 ±0.0098

|0.348

|20.772907 ±0.000023

|0.1438{{+-|0.0025|0.0037}}

|663.4{{+-|9.1|6.3}}

| style="background:#FFFF00" |transit

|220.3112{{+-|0.5108|0.5085}}

|1.022{{+-|0.043|0.076}}

|5609.0 ±33.0

|{{Cite journal |last1=Osborn |first1=Hugh P. |last2=Nowak |first2=Grzegorz |last3=Hébrard |first3=Guillaume |last4=Masseron |first4=Thomas |last5=Lillo-Box |first5=J. |last6=Pallé |first6=Enric |last7=Bekkelien |first7=Anja |last8=Florén |first8=Hans-Gustav |last9=Guterman |first9=Pascal |last10=Simon |first10=Attila E. |last11=Adibekyan |first11=V. |last12=Bieryla |first12=Allyson |last13=Borsato |first13=Luca |last14=Brandeker |first14=Alexis |last15=Ciardi |first15=David R. |date=2023 |title=Two warm Neptunes transiting HIP 9618 revealed by TESS and Cheops |journal=Monthly Notices of the Royal Astronomical Society |volume=523 |issue=2 |pages=3069–3089 |doi=10.1093/mnras/stad1319 |doi-access=free |arxiv=2306.04450}}

|<0.0576 ±0.0053

|0.298

|52.563491 ±0.000072

|0.2669{{+-|0.0046|0.0069}}

|486.9{{+-|6.6|4.6}}

| style="background:#FFFF00" |transit

|220.3112{{+-|0.5108|0.5085}}

|1.022{{+-|0.043|0.076}}

|5609.0 ±33.0

|

|0.032 ±0.0025

|0.31

|13.63083 ±0.00003

|0.1070 ±0.0016

|777 ±18

| style="background:#FFFF00" |transit

|222.4123{{+-|0.5779|0.5750}}

|0.89 ±0.04

|5289 ±69

|Host star also known as TOI-469{{Cite journal |last1=Damasso |first1=M. |last2=Rodrigues |first2=J. |last3=Castro-González |first3=A. |last4=Lavie |first4=B. |last5=Davoult |first5=J. |last6=Osorio |first6=M. R. Zapatero |last7=Dou |first7=J. |last8=Sousa |first8=S. G. |last9=Owen |first9=J. E. |last10=Sossi |first10=P. |last11=Adibekyan |first11=V. |last12=Osborn |first12=H. |last13=Leinhardt |first13=Z. |last14=Alibert |first14=Y. |last15=Lovis |first15=C. |date=2023 |title=A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO. Radial velocities lead to the detection of transits with low signal-to-noise ratio |journal=Astronomy and Astrophysics |volume=679 |doi=10.1051/0004-6361/202347240 |arxiv=2308.13310|bibcode=2023A&A...679A..33D |s2cid=261214427 }}

|0.014 ±0.001

|1.58{{+-|0.10|0.11}}

|3.53796 ±0.00003

|0.0436{{+-|0.0006|0.0007}}

|1217 ±29

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

|222.4123{{+-|0.5779|0.5750}}

|0.89 ±0.04

|5289 ±69

|

|0.016 ±0.001

|1.37 ±0.11

|6.42975{{+-|0.00009|0.00010}}

|0.0649{{+-|0.0009|0.0010}}

|998.0 ±24.0

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

|222.4123{{+-|0.5779|0.5750}}

|0.89 ±0.04

|5289 ±69

|

|2.4{{+-|0.4|0.2}}

|

|3274{{+-|47|46}}

|4.0 ±0.1

|

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

|129.6239{{+-|0.2166|0.2162}}

|0.80 ±0.04

|

|

|14.8 ±0.4

|

|104100{{+-|107260|40934}}

|23.04{{+-|13.88|6.55}}

|2050{{+-|35|20}}

| style="background:#FF6CDA" |imaging

|481.188{{+-|4.837|4.472}}

|0.135{{+-|0.010|0.013}}

|

|{{Cite journal |last1=Chomez |first1=A. |last2=Squicciarini |first2=V. |last3=Lagrange |first3=A. -M. |last4=Delorme |first4=P. |last5=Viswanath |first5=G. |last6=Janson |first6=M. |last7=Flasseur |first7=O. |last8=Chauvin |first8=G. |last9=Langlois |first9=M. |last10=Rubini |first10=P. |last11=Bergeon |first11=S. |last12=Albert |first12=D. |last13=Bonnefoy |first13=M. |last14=Desidera |first14=S. |last15=Engler |first15=N. |date=2023 |title=An imaged 15 M _Jup companion within a hierarchical quadruple system |journal=Astronomy & Astrophysics |volume=676 |pages=L10 |doi=10.1051/0004-6361/202347044 |arxiv=2307.01195|bibcode=2023A&A...676L..10C |s2cid=259316431 }}

|

|0.163

|7.610303 ±0.000018

|0.06899{{+-|0.00029|0.00023}}

|721 ±10

| style="background:#FFFF00" |transit

|150.7239{{+-|0.2818|0.2805}}

|0.761 ±0.038

|4930 ±100

|{{Cite journal |last1=Lowson |first1=N |last2=Zhou |first2=G |last3=Huang |first3=C X |last4=Wright |first4=D J |last5=Edwards |first5=B |last6=Nabbie |first6=E |last7=Venner |first7=A |last8=Quinn |first8=S N |last9=Collins |first9=K A |last10=Gillen |first10=E |last11=Battley |first11=M |last12=Triaud |first12=A |last13=Hellier |first13=C |last14=Seager |first14=S |last15=Winn |first15=J N |date=2023-09-12 |title=Two mini-Neptunes Transiting the Adolescent K-star HIP 113103 Confirmed with TESS and CHEOPS |journal=Monthly Notices of the Royal Astronomical Society |volume=527 |pages=1146–1162 |language=en |doi=10.1093/mnras/stad2756 |issn=0035-8711|doi-access=free }}

|

|0.2141

|14.245648 ±0.000019

|0.10479{{+-|0.00045|0.00035}}

|585 ±10

| style="background:#FFFF00" |transit

|150.7239{{+-|0.2818|0.2805}}

|0.761 ±0.038

|4930 ±100

|

|0.0172 ±0.0024

|

|36.116{{+-|0.027|0.029}}

|0.1417 ±0.0023

|234.4{{+-|5.5|5.3}}

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

|20.36655 ±0.01453

|0.291 ±0.013

|3347 ±50

|Habitable zone planet. Host star also known as Gliese 555{{Cite journal |last1=González-Álvarez |first1=E. |last2=Kemmer |first2=J. |last3=Chaturvedi |first3=P. |last4=Caballero |first4=J. A. |last5=Quirrenbach |first5=A. |last6=Amado |first6=P. J. |last7=Béjar |first7=V. J. S. |last8=Cifuentes |first8=C. |last9=Herrero |first9=E. |last10=Kossakowski |first10=D. |last11=Reiners |first11=A. |last12=Ribas |first12=I. |last13=Rodríguez |first13=E. |last14=Rodríguez-López |first14=C. |last15=Sanz-Forcada |first15=J. |date=2023 |title=The CARMENES search for exoplanets around M dwarfs |journal=Astronomy & Astrophysics |volume=675 |pages=A141 |doi=10.1051/0004-6361/202346276 |arxiv=2305.19677|s2cid=265978782 }}

|5.41+{{+-|0.52|0.44}}

|

|921.2 ±10.8

|1.961 ±0.027

|

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

|358.315{{+-|2.645|2.609}}

|1.18 ±0.04

|5959 ±61

|{{Cite journal |last1=Bonomo |first1=A. S. |last2=Dumusque |first2=X. |last3=Massa |first3=A. |last4=Mortier |first4=A. |last5=Bongiolatti |first5=R. |last6=Malavolta |first6=L. |last7=Sozzetti |first7=A. |last8=Buchhave |first8=L. A. |last9=Damasso |first9=M. |last10=Haywood |first10=R. D. |last11=Morbidelli |first11=A. |last12=Latham |first12=D. W. |last13=Molinari |first13=E. |last14=Pepe |first14=F. |last15=Poretti |first15=E. |date=2023 |title=Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems |journal=Astronomy & Astrophysics |volume=677 |doi=10.1051/0004-6361/202346211 |arxiv=2304.05773|bibcode=2023A&A...677A..33B |s2cid=258078829 }}

|0.0094 ±0.0085

|0.091 ±0.005

|4.0179694 ±0.0000027

|0.0270 ±0.0002

|412 ±9

| style="background:#FFFF00" |transit

|71.126 ±0.030

|0.1635 ±0.0041

|3173 ±53

|{{cite journal|arxiv=2302.00699|year=2023|title=An Earth-sized Planet around an M5 Dwarf Star at 22 pc|last1=Hirano |first1=Teruyuki |last2=Dai |first2=Fei |last3=Livingston |first3=John H. |last4=Kasagi |first4=Yui |last5=Narita |first5=Norio |author6=Hiroyuki Tako Ishikawa |last7=Grziwa |first7=Sascha |last8=Lam |first8=Kristine W. F. |last9=Miyakawa |first9=Kohei |last10=Serrano |first10=Luisa M. |last11=Matsumoto |first11=Yuji |last12=Kokubo |first12=Eiichiro |last13=Kimura |first13=Tadahiro |last14=Ikoma |first14=Masahiro |last15=Winn |first15=Joshua N. |last16=Wisniewski |first16=John P. |last17=Harakawa |first17=Hiroki |last18=Teng |first18=Huan-Yu |last19=Cochran |first19=William D. |last20=Fukui |first20=Akihiko |last21=Gandolfi |first21=Davide |last22=Guenther |first22=Eike W. |last23=Hori |first23=Yasunori |last24=Ikuta |first24=Kai |last25=Kawauchi |first25=Kiyoe |last26=Knudstrup |first26=Emil |last27=Korth |first27=Judith |last28=Kotani |first28=Takayuki |last29=Krishnamurthy |first29=Vigneshwaran |last30=Kudo |first30=Tomoyuki |journal=The Astronomical Journal |volume=165 |issue=3 |page=131 |doi=10.3847/1538-3881/acb7e1 |bibcode=2023AJ....165..131H |s2cid=256503980 |display-authors=1 |doi-access=free }}

|<5.2

|0.241{{+-|0.027|0.0152}}

|13.1020{{+-|0.0026|0.0024}}

|0.0880{{+-|0.0100|0.0210}}

|447 ±49

| style="background:#FFFF00" |transit

|392.402{{+-|1.973|1.954}}

|0.548 ±0.012

|3746 ±72

|{{Cite journal |last1=Incha |first1=Elyse |last2=Vanderburg |first2=Andrew |last3=Jacobs |first3=Tom |last4=LaCourse |first4=Daryll |last5=Bieryla |first5=Allyson |last6=Pass |first6=Emily |last7=Howell |first7=Steve B |last8=Berlind |first8=Perry |last9=Calkins |first9=Michael |last10=Esquerdo |first10=Gilbert |last11=Latham |first11=David W |last12=Mann |first12=Andrew W |date=2023-05-23 |title=Kepler 's last planet discoveries: two new planets and one single-transit candidate from K2 campaign 19 |url=https://academic.oup.com/mnras/article/523/1/474/7178009 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=523 |issue=1 |pages=474–487 |doi=10.1093/mnras/stad1049 |issn=0035-8711 |doi-access=free |access-date=6 October 2023 |archive-date=1 December 2023 |archive-url=https://web.archive.org/web/20231201103215/https://academic.oup.com/mnras/article/523/1/474/7178009 |url-status=live |arxiv=2305.18516 }}

|<2.2

|0.295{{+-|0.012|0.011}}

|6.5350 ±0.0014

|0.063{{+-|0.006|0.014}}

|558 ±55

| style="background:#FFFF00" |transit

|306.7249{{+-|0.9860|0.9794}}

|0.569 ±0.012

|3861 ±77

|

|1.16 ±0.09

|1.23

|4700 {{+-|3000|700}}

|4.11 ±0.32

|

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

|16960

|0.574 ±0.037

|

|Gas giant.{{Cite journal |last1=Specht |first1=D |last2=Poleski |first2=R |last3=Penny |first3=M T |last4=Kerins |first4=E |last5=McDonald |first5=I |last6=Lee |first6=Chung-Uk |last7=Udalski |first7=A |last8=Bond |first8=I A |last9=Shvartzvald |first9=Y |last10=Zang |first10=Weicheng |last11=Street |first11=R A |last12=Hogg |first12=D W |last13=Gaudi |first13=B S |last14=Barclay |first14=T |last15=Barentsen |first15=G |date=2023-02-22 |title=Kepler K2 Campaign 9 – II. First space-based discovery of an exoplanet using microlensing |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=520 |issue=4 |pages=6350–6366 |doi=10.1093/mnras/stad212 |doi-access=free |arxiv=2203.16959 |issn=0035-8711}}{{Cite web |title=K2-2016-BLG-005L b - Exoplanet-catalog |url=https://exoplanets.nasa.gov/exoplanet-catalog/8836/k2-2016-blg-0005l-b/ |access-date=2023-12-03 |website=Exoplanet Exploration: Planets Beyond our Solar System |language=en |archive-date=3 December 2023 |archive-url=https://web.archive.org/web/20231203200006/https://exoplanets.nasa.gov/exoplanet-catalog/8836/k2-2016-blg-0005l-b/ |url-status=live }}

|0.03990 ±0.00705

|

|151.04 ±0.45

|0.5379 ±0.0044

|

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

|605.039{{+-|2.645|2.626}}

|0.910 ±0.021

|5708 ±28

|

|0.272 ±0.032

|

|3455 {{+-|348|169}}

|4.60 {{+-|0.32|0.16}}

|

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

|

|1.057 {{+-|0.022|0.020}}

|5847 ±75

|{{Cite journal |last1=Bonomo |first1=A. S. |last2=Dumusque |first2=X. |last3=Massa |first3=A. |last4=Mortier |first4=A. |last5=Bongiolatti |first5=R. |last6=Malavolta |first6=L. |last7=Sozzetti |first7=A. |last8=Buchhave |first8=L. A. |last9=Damasso |first9=M. |last10=Haywood |first10=R. D. |last11=Morbidelli |first11=A. |last12=Latham |first12=D. W. |last13=Molinari |first13=E. |last14=Pepe |first14=F. |last15=Poretti |first15=E. |date=September 2023 |title=Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities: No excess of cold Jupiters in small planet systems |url=https://www.aanda.org/articles/aa/pdf/2023/09/aa46211-23.pdf |journal=Astronomy & Astrophysics |volume=677 |issue=A33 |pages=18 |doi=10.1051/0004-6361/202346211 |arxiv=2304.05773 |bibcode=2023A&A...677A..33B |s2cid=261556620 |issn=0004-6361 |access-date=7 December 2023 |archive-date=3 December 2023 |archive-url=https://web.archive.org/web/20231203174310/https://www.aanda.org/articles/aa/pdf/2023/09/aa46211-23.pdf |url-status=live }}

|

|0.1509503920

|4.458169937

|

|

| style="background:#FFFF00" |transit

|

|1.017 {{+-|0.167|0.125}}

|6100{{+-|193|214}}

|

|

|0.3570351276

|94.8864975

|

|

| style="background:#FFFF00" |transit

|

|0.966 {{+-|0.075|0.068}}

|5888 {{+-|106|117}}

|

|

|0.0794273806

|0.764007986

|

|

| style="background:#FFFF00" |transit

|

|0.84 {{+-|0.065|0.09}}

|5142 ±153

|

|

|0.6351157298

|150.0209961

|

|

| style="background:#FFFF00" |transit

|

|0.846 {{+-|0.059|0.049}}

|5618 ±112

|

|

|0.1849409870

|232.0469971

|

|

| style="background:#FFFF00" |transit

|

|0.974 {{+-|0.082|0.062}}

|5903 {{+-|106|117}}

|

|

|0.2346332985

|85.51660156

|

|

| style="background:#FFFF00" |transit

|

|1 ±0.072

|5592 ±75

|

|

|0.1543405297

|3.076410055

|

|

| style="background:#FFFF00" |transit

|

|0.949 {{+-|0.067|0.055}}

|5670 ±114

|

|

|0.4055676538

|24.6147995

|

|

| style="background:#FFFF00" |transit

|

|0.859 {{+-|0.06|0.033}}

|5312 ±79

|

|

|0.3911149410

|11.67889977

|

|

| style="background:#FFFF00" |transit

|

|1.041 ±0.139

|6122 {{+-|169|190}}

|

|

|0.1360516194

|5.254559994

|

|

| style="background:#FFFF00" |transit

|

|1.05{{+-|0.075|0.113}}

|5550 {{+-|166|183}}

|

|

|0.1464004690

|4.096680164

|

|

| style="background:#FFFF00" |transit

|

|0.8 {{+-|0.048|0.028}}

|4999 ±79

|

|

|0.1754842890

|6.503270149

|

|

| style="background:#FFFF00" |transit

|

|0.8 {{+-|0.048|0.028}}

|4999 ±79

|

|

|0.1583551639

|17.15699959

|

|

| style="background:#FFFF00" |transit

|

|1.016 {{+-|0.093|0.084}}

|5676 {{+-|115|104}}

|

|

|0.157641449

|2.421489954

|

|

| style="background:#FFFF00" |transit

|

|1.27 {{+-|0.142|0.156}}

|6213 {{+-|173|259}}

|

|

|0.09474546031

|6.209179878

|

|

| style="background:#FFFF00" |transit

|

|0.782 {{+-|0.116|0.062}}

|5440 ±162

|

|

|0.2816491659

|11.80609989

|

|

| style="background:#FFFF00" |transit

|

|1.714 {{+-|0.17|0.316}}

|6900 {{+-|184|204}}

|

|

|0.2770100246

|29.54210091

|

|

| style="background:#FFFF00" |transit

|

|0.877 {{+-|0.083|0.092}}

|5510 {{+-|166|149}}

|

|

|0.4607912263

|20.99720001

|

|

| style="background:#FFFF00" |transit

|

|0.813 {{+-|0.104|0.064}}

|5211 {{+-|181|163}}

|

|

|0.5035248257

|5.05821991

|

|

| style="background:#FFFF00" |transit

|

|0.951 {{+-|0.198|0.144}}

|4883 {{+-|146|132}}

|

|

|0.2112591764

|180.9259949

|

|

| style="background:#FFFF00" |transit

|

|0.937 {{+-|0.09|0.121}}

|5818 {{+-|139|157}}

|{{Cite journal |last1=Valizadegan |first1=Hamed |last2=Martinho |first2=Miguel J. S. |last3=Jenkins |first3=Jon M. |last4=Caldwell |first4=Douglas A. |last5=Twicken |first5=Joseph D. |last6=Bryson |first6=Stephen T. |date=2023-07-01 |title=Multiplicity Boost of Transit Signal Classifiers: Validation of 69 New Exoplanets using the Multiplicity Boost of ExoMiner |journal=The Astronomical Journal |volume=166 |issue=1 |pages=28 |doi=10.3847/1538-3881/acd344 |arxiv=2305.02470 |bibcode=2023AJ....166...28V |issn=0004-6256 |doi-access=free }}

|

|0.1500582511

|199.6679993

|

|

| style="background:#FFFF00" |transit

|

|0.794 {{+-|0.071|0.03}}

|5678 {{+-|113|102}}

|

|

|0.1675442283

|59.28409958

|

|

| style="background:#FFFF00" |transit

|

|0.861 {{+-|0.05|0.041}}

|5225 {{+-|83|73}}

|

|

|0.1555895228

|8.934909821

|

|

| style="background:#FFFF00" |transit

|

|1.336 ±0.2

|6688 {{+-|187|281}}

|

|

|0.2001966118

|11.60449982

|

|

| style="background:#FFFF00" |transit

|

|0.934 {{+-|0.063|0.045}}

|5533 {{+-|83|74}}

|

|

|0.7992697886

|35.79949951

|

|

| style="background:#FFFF00" |transit

|

|1.801 {{+-|0.193|0.359}}

|5745 {{+-|86|77}}

|

|

|0.2788835142

|61.5685997

|

|

| style="background:#FFFF00" |transit

|

|0.991 {{+-|0.079|0.065}}

|5626 ±77

|

|0.266 {{+-|0.098|0.063}}

|

|841.4{{+-|8.1|5.3}}

|

|

| style="background:#FFFF00" |transit

|

|0.943 ±0.037

|5491 ±100

|{{Cite journal |last1=Yahalomi |first1=Daniel A |last2=Kipping |first2=David |last3=Nesvorný |first3=David |last4=Dalba |first4=Paul A |last5=Benni |first5=Paul |last6=Cacho-Negrete |first6=Ceiligh |last7=Collins |first7=Karen |last8=Earwicker |first8=Joel T |last9=Lewis |first9=John Arban |last10=McLeod |first10=Kim K |last11=Schwarz |first11=Richard P |last12=Wang |first12=Gavin |date=2023-10-28 |title=Not-so-fast Kepler-1513: a perturbing planetary interloper in the exomoon corridor |url=https://academic.oup.com/mnras/article/527/1/620/7303293 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=527 |issue=1 |pages=620–639 |doi=10.1093/mnras/stad3070 |issn=0035-8711 |doi-access=free |arxiv=2310.03802 |bibcode=2024MNRAS.527..620Y |access-date=6 December 2023 |archive-date=9 December 2023 |archive-url=https://web.archive.org/web/20231209114430/https://academic.oup.com/mnras/article/527/1/620/7303293 |url-status=live }}

|

|0.212775814

|9.630929947

|

|

| style="background:#FFFF00" |transit

|

|1.06 {{+-|0.177|0.133}}

|6432{{+-|155|214}}

|

|

|0.196806485

|44.98529816

|

|

| style="background:#FFFF00" |transit

|

|0.825 {{+-|0.096|0.078}}

|5295 ±185

|

|

|0.1427426870

|4.729469776

|

|

| style="background:#FFFF00" |transit

|

|0.609 ±0.033

|4224 ±84

|

|

|0.3621203501

|116.5849991

|

|

| style="background:#FFFF00" |transit

|

|0.936 {{+-|0.114|0.093}}

|5738 {{+-|156|173}}

|

|

|0.1476494621

|0.626281977

|

|

| style="background:#FFFF00" |transit

|

|0.79 {{+-|0.073|0.064}}

|4922 ±169

|

|

|0.129895841

|0.766691983

|

|

| style="background:#FFFF00" |transit

|

|0.765 {{+-|0.051|0.028}}

|4821 ±76

|

|

|0.1531807444

|3.596430063

|

|

| style="background:#FFFF00" |transit

|

|1.09 {{+-|0.07|0.078}}

|5887 {{+-|70|79}}

|

|

|0.1417613278

|5.053750038

|

|

| style="background:#FFFF00" |transit

|

|0.999 {{+-|0.114|0.125}}

|5772 {{+-|156|173}}

|

|

|0.1505043216

|3.157219887

|

|

| style="background:#FFFF00" |transit

|

|1.251 {{+-|0.19|0.233}}

|6120 {{+-|195|217}}

|

|

|1.043

|4.96

|

|

| style="background:#FFFF00" |transit

|

|1.097 {{+-|0.21|0.135}}

|6117 {{+-|156|210}}

|{{Cite journal |last1=Wu |first1=Dong-Hong |last2=Rice |first2=Malena |last3=Wang |first3=Songhu |date=2023-04-01 |title=Evidence for Hidden Nearby Companions to Hot Jupiters |journal=The Astronomical Journal |volume=165 |issue=4 |pages=171 |doi=10.3847/1538-3881/acbf3f |arxiv=2302.12778 |bibcode=2023AJ....165..171W |issn=0004-6256 |doi-access=free }}

|

|0.1625482348

|4.537000179

|

|

| style="background:#FFFF00" |transit

|

|0.769 {{+-|0.053|0.079}}

|4805 ±144

|

|

|0.2683562384

|10.849699997

|

|

| style="background:#FFFF00" |transit

|

|0.869 {{+-|0.06|0.095}}

|5251 ±158

|

|

|0.2538143392

|33.0257988

|

|

| style="background:#FFFF00" |transit

|

|1.049 {{+-|0.059|0.073}}

|5819 {{+-|69|87}}

|

|

|0.8396838173

|453.5429993

|

|

| style="background:#FFFF00" |transit

|

|1.519 {{+-|0.15|0.376}}

|5874 {{+-|87|79}}

|

|

|0.773130047

|3.823159933

|

|

| style="background:#FFFF00" |transit

|

|1.213 {{+-|0.076|0.093}}

|6202 {{+-|99|149}}

|

|

|0.1465788952

|7.328519821

|

|

| style="background:#FFFF00" |transit

|

|0.812 {{+-|0.058|0.029}}

|5135 {{+-|84|75}}

|

|

|0.718709408

|1.99285996

|

|

| style="background:#FFFF00" |transit

|

|0.42 {{+-|0.046|0.056}}

|3638 {{+-|72|87}}

|

|

|0.1981446855

|3.420650005

|

|

| style="background:#FFFF00" |transit

|

|0.877 {{+-|0.064|0.037}}

|3638 {{+-|72|87}}

|

|

|0.2631818295

|19.54929924

|

|

| style="background:#FFFF00" |transit

|

|0.776 {{+-|0.089|0.065}}

|5549 ±163

|

|

|0.134713408

|2.345860004

|

|

| style="background:#FFFF00" |transit

|

|0.799 {{+-|0.041|0.081}}

|4769 ±172

|

|

|0.151307244

|3.648269892

|

|

| style="background:#FFFF00" |transit

|

|0.799 {{+-|0.041|0.081}}

|4769 ±172

|

|

|0.2912843007

|5.644889832

|

|

| style="background:#FFFF00" |transit

|

|0.799 {{+-|0.041|0.081}}

|4769 ±172

|

|

|0.2188423849

|8.742970467

|

|

| style="background:#FFFF00" |transit

|

|0.799 {{+-|0.041|0.081}}

|4769 ±172

|

|

|0.1382819717

|1.549999952

|

|

| style="background:#FFFF00" |transit

|

|1.127 {{+-|0.189|0.172}}

|6033 ±183

|

|

|0.4247487156

|10.16100025

|

|

| style="background:#FFFF00" |transit

|

|0.999 {{+-|0.153|0.126}}

|6032 {{+-|189|232}}

|

|

|0.3491842959

|1.735129952

|

|

| style="background:#FFFF00" |transit

|

|1.028 {{+-|0.074|0.067}}

|5751 {{+-|103|114}}

|

|

|0.1058972326

|1.187000036

|

|

| style="background:#FFFF00" |transit

|

|1.028 {{+-|0.074|0.067}}

|5751 {{+-|103|114}}

|

|

|0.1646893688

|13.26080036

|

|

| style="background:#FFFF00" |transit

|

|0.914 {{+-|0.061|0.042}}

|5478 {{+-|82|74}}

|

|

|0.2594348291

|22.79019928

|

|

| style="background:#FFFF00" |transit

|

|0.914 {{+-|0.061|0.042}}

|5478 {{+-|82|74}}

|

|

|0.0916229564

|15.61120033

|

|

| style="background:#FFFF00" |transit

|

|0.874 {{+-|0.048|0.054}}

|5383 ±107

|

|

|0.3949511704

|26.65660095

|

|

| style="background:#FFFF00" |transit

|

|1.373 {{+-|0.205|0.512}}

|5159 {{+-|171|155}}

|

|

|0.0555001398

|4.612319946

|

|

| style="background:#FFFF00" |transit

|

|0.932 {{+-|0.052|0.047}}

|5495 {{+-|74|82}}

|

|

|0.4119018693

|73.75779724

|

|

| style="background:#FFFF00" |transit

|

|0.847 {{+-|0.068|0.049}}

|5029 {{+-|192|174}}

|

|

|0.204657316

|32.37609863

|

|

| style="background:#FFFF00" |transit

|

|0.748 {{+-|0.027|0.043}}

|4580 ±92

|

|

|0.2509594797

|92.72949982

|

|

| style="background:#FFFF00" |transit

|

|0.748 {{+-|0.027|0.043}}

|4580 ±92

|

|

|0.2179502440

|26.75749969

|

|

| style="background:#FFFF00" |transit

|

|1.111 ±0.153

|6215 {{+-|194|259}}

|

|

|0.0619324805

|3.03263998

|

|

| style="background:#FFFF00" |transit

|

|0.962 {{+-|0.054|0.068}}

|5640 {{+-|101|113}}

|

|

|0.3169779722

|8.739450455

|

|

| style="background:#FFFF00" |transit

|

|0.632 {{+-|0.063|0.057}}

|4406 {{+-|154|170}}

|

|

|0.2961910652

|6.383150101

|

|

| style="background:#FFFF00" |transit

|

|0.581 ±0.029

|3757 {{+-|74|82}}

|

|

|0.1963604037

|20.6182003

|

|

| style="background:#FFFF00" |transit

|

|0.581 ±0.029

|3757 {{+-|74|82}}

|

|

|0.1062540847

|1.190999985

|

|

| style="background:#FFFF00" |transit

|

|0.864 {{+-|0.049|0.085}}

|5081 {{+-|166|136}}

|

|

|0.3639938397

|14.09449959

|

|

| style="background:#FFFF00" |transit

|

|0.864 {{+-|0.049|0.085}}

|5081 {{+-|166|136}}

|

|0.05 ±0.04

|

|

|1.40 ±0.17

|

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

|21000 ±2000

|0.25 ±0.14

|

|

|0.00415 ±0.00176

|

|

|2.26{{+-|0.51|0.69}}

|

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

|10665{{+-|4175|3751}}

|0.43 ±0.18

|

|{{Cite journal |last1=Zang |first1=Weicheng |last2=Jung |first2=Youn Kil |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 |date=2023-03-01 |title=Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10 −4 Planets from the First 4 yr Survey |journal=The Astronomical Journal |volume=165 |issue=3 |pages=103 |doi=10.3847/1538-3881/acb34b |arxiv=2210.12344 |bibcode=2023AJ....165..103Z |issn=0004-6256 |doi-access=free }}

|1.20 ±1.21

|

|

|1.39 ±0.50

|

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

|23000 ±4000

|0.18 ±0.18

|

|

|0.0175{{+-|0.0111|0.0088}}

|

|

|1.85{{+-|0.55|0.60}}

|

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

|17612{{+-|5936|8480}}

|0.34{{+-|0.22|0.17}}

|

|

|0.0117{{+-|0.0117|0.0057}}

|

|

|1.25{{+-|0.27|0.25}}

|

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

|23353{{+-|1990|2120}}

|0.27{{+-|0.26|0.13}}

|

|

|0.0111{{+-|0.0061|0.0051}}

|

|

|1.78{{+-|0.45|0.46}}

|

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

|13829{{+-|7045|5577}}

|0.41{{+-|0.23|0.19}}

|

|

|1.81 ±0.96

|

|

|5.67 ±2.70

|

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

|22000 ±5000

|0.70 ±0.37

|

|{{cite journal|arxiv=2302.13544|year=2023|title=Systematic KMTNet Planetary Anomaly Search. VIII. Complete Sample of 2019 Subprime Field Planets|author1=Youn Kil Jung |last2=Zang |first2=Weicheng |last3=Wang |first3=Hanyue |last4=Han |first4=Cheongho |last5=Gould |first5=Andrew |last6=Udalski |first6=Andrzej |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Hwang |first9=Kyu-Ha |last10=Ryu |first10=Yoon-Hyun |last11=Shin |first11=In-Gu |last12=Shvartzvald |first12=Yossi |last13=Yang |first13=Hongjing |last14=Yee |first14=Jennifer C. |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=165 |issue=6 |page=226 |doi=10.3847/1538-3881/accb8f |bibcode=2023AJ....165..226J |s2cid=258505742 |display-authors=1 |doi-access=free }}

|0.094 ±0.050

|

|

|2.44 ±1.12

|

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

|9000 ±3000

|0.39 ±0.21

|

|

|0.0128{{+-|0.0081|0.0065}}

|

|

|1.70{{+-|0.50|0.56}}

|

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

|15231{{+-|7990|6849}}

|0.25{{+-|0.16|0.13}}

|

|

|0.0147 ±0.0048

|

|

|2.87{{+-|0.64|0.66}}

|

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

|21592{{+-|2348|6295}}

|0.75{{+-|0.24|0.25}}

|

|

|1.16 ±0.77

|

|

|1.85 ±0.93

|

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

|19000 ±5000

|0.34 ±0.25

|

|

|0.1255{{+-|0.0648|0.0374}}

|

|

|2.29{{+-|0.64|0.42}}

|

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

|10437{{+-|2968|2188}}

|0.23{{+-|0.12|0.07}}

|

|{{Cite journal |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 |last9=Kil Jung |first9=Youn |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 |date=2023-03-01 |title=Mass Production of 2021 KMTNet Microlensing Planets II |journal=The Astronomical Journal |volume=165 |issue=3 |pages=83 |doi=10.3847/1538-3881/acab6b |arxiv=2207.07295 |bibcode=2023AJ....165...83R |issn=0004-6256 |doi-access=free }}

|1.26{{+-|1.01|0.66}}

|

|

|1.75 ±0.42

|

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

|21134{{+-|3262|4501}}

|0.38{{+-|0.30|0.20}}

|

|

|1.30 ±0.68

|

|

|3.54 ±1.06

|

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

|14807 ±5447

|0.63 ±0.33

|

|

|1.07{{±|1.15|0.68}}

|

|

|1.79{{±|0.30|0.38}}

|

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

|23000{{±|4000|5000}}

|0.37{{±|0.4|0.23}}

|

|Multiple orbital solutions{{cite journal|arxiv=2304.03871|year=2023|title=KMT-2021-BLG-2010Lb, KMT-2022-BLG-0371Lb, and KMT-2022-BLG-1013Lb: Three microlensing planets detected via partially covered signals |last1=Han |first1=Cheongho |last2=Lee |first2=Chung-Uk |last3=Zang |first3=Weicheng |author4=Youn Kil Jung |last5=Christie |first5=Grant W. |last6=Zhang |first6=Jiyuan |last7=Albrow |first7=Michael D. |last8=Chung |first8=Sun-Ju |last9=Gould |first9=Andrew |last10=Hwang |first10=Kyu-Ha |last11=Kim |first11=Doeon |last12=Ryu |first12=Yoon-Hyun |last13=Shin |first13=In-Gu |last14=Shvartzvald |first14=Yossi |last15=Yang |first15=Hongjing |last16=Yee |first16=Jennifer C. |last17=Cha |first17=Sang-Mok |last18=Kim |first18=Dong-Jin |last19=Kim |first19=Seung-Lee |last20=Lee |first20=Dong-Joo |last21=Lee |first21=Yongseok |last22=Park |first22=Byeong-Gon |last23=Pogge |first23=Richard W. |last24=Natusch |first24=Tim |last25=Mao |first25=Shude |last26=Maoz |first26=Dan |last27=Penny |first27=Matthew T. |last28=Zhu |first28=Wei |journal=Astronomy & Astrophysics |volume=674 |pages=A90 |doi=10.1051/0004-6361/202346298 |bibcode=2023A&A...674A..90H |s2cid=258048865 }}

|0.900{{+-|0.420|0.240}}

|

|

|1.85 ±0.31

|

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

|9687 ±2348

|0.20{{+-|0.10|0.05}}

|

|

|0.26{{±|0.13|0.11}}

|

|

|3.02{{±|0.45|0.56}}

|

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

|23000{{±|3000|4000}}

|0.63{{±|0.32|0.28}}

|

|Multiple orbital solutions

|0.0485{{±|0.0302|0.0233}}

|

|

|1.9 ±0.7

|

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

|11000 ±5000

|0.53{{±|0.31|0.26}}

|

|{{Cite encyclopedia |title=The Extrasolar Planet Encyclopaedia — KMT-2022-BLG-0440L b |url=https://exoplanet.eu/catalog/kmt_2022_blg_0440l_b--8582/ |access-date=2023-01-19 |encyclopedia=Extrasolar Planets Encyclopaedia |date=23 October 1995 }}{{cite journal|arxiv=2301.06779|year=2023|title=KMT-2022-BLG-0440Lb: A new q < 10−4 microlensing planet with the central-resonant caustic degeneracy broken|last1=Zhang |first1=Jiyuan |last2=Zang |first2=Weicheng |author3=Youn Kil Jung |last4=Yang |first4=Hongjing |last5=Gould |first5=Andrew |last6=Sumi |first6=Takahiro |last7=Mao |first7=Shude |last8=Dong |first8=Subo |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=Yee |first16=Jennifer C. |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=Qian |first26=Qiyue |last27=Liu |first27=Zhuokai |last28=Maoz |first28=Dan |last29=Penny |first29=Matthew T. |last30=Zhu |first30=Wei |journal=Monthly Notices of the Royal Astronomical Society |volume=522 |issue=4 |pages=6055–6069 |doi=10.1093/mnras/stad1398 |doi-access=free |display-authors=1 }}

|0.31{{±|0.46|0.16}}

|

|

|1.38{{±|0.18|0.20}}

|

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

|25000 ±3000

|0.18{{±|0.28|0.10}}

|

|

|0.0147 ±0.0014

|

|8.781 ±0.006

|0.048 ±0.006

|330

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

|33.372 ±0.014

|0.210 ±77

|3129 ±6

|{{Cite journal |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=Andreas |last9=Gubler |first9=Jonas L. |last10=Quanz |first10=Sascha P. |date=February 2023 |title=L 363-38 b: A planet newly discovered with ESPRESSO orbiting a nearby M dwarf star |url=https://www.aanda.org/10.1051/0004-6361/202244347 |journal=Astronomy & Astrophysics |volume=670 |issue=A42 |pages=12 |doi=10.1051/0004-6361/202244347 |arxiv=2210.12710 |bibcode=2023A&A...670A..42S |s2cid=253098575 |issn=0004-6361}}

|0.0414 ±0.0026

|

|3.71778{{±|0.00080|0.00081}}

|0.02262 ±0.00018

|

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

|51.43 ±0.03

|0.1118 ±0.0027

|2861 ±77

|{{cite arXiv|eprint=2303.13321|year=2023|title=An extreme test case for planet formation: a close-in Neptune orbiting an ultracool star|last1=Stefansson |first1=Gudmundur |last2=Mahadevan |first2=Suvrath |last3=Miguel |first3=Yamila |last4=Robertson |first4=Paul |last5=Delamer |first5=Megan |last6=Kanodia |first6=Shubham |last7=Cañas |first7=Caleb |last8=Winn |first8=Joshua |last9=Ninan |first9=Joe |last10=Terrien |first10=Ryan |last11=Holcomb |first11=Rae |last12=Ford |first12=Eric |last13=Zawadzki |first13=Brianna |last14=Bowler |first14=Brendan P. |last15=Bender |first15=Chad |last16=Cochran |first16=William |last17=Diddams |first17=Scott |last18=Endl |first18=Michael |last19=Fredrick |first19=Connor |last20=Halverson |first20=Samuel |last21=Hearty |first21=Fred |last22=Hill |first22=Gary J. |last23=Lin |first23=Andrea |last24=Metcalf |first24=Andrew |last25=Monson |first25=Andrew |last26=Ramsey |first26=Lawrence |last27=Roy |first27=Arpita |last28=Schwab |first28=Christian |last29=Wright |first29=Jason |last30=Zeimann |first30=Gregory |class=astro-ph.EP }}

|0.002876 ±0.000588

|0.0883 ±0.0045

|2.029088 ±0.000006

|0.0206

|586.0

| style="background:#FFFF00" |transit

|40.704

|0.262

|3312.0

|{{cite journal |last1=Lustig-Yaeger |first1=J. |last2=Fu |first2=G. |display-authors=etal |date=January 2023 |title=A JWST transmission spectrum of the nearby Earth-sized exoplanet LHS 475 B |journal=Nature Astronomy |volume=7 |issue=11 |pages=1317–1328 |doi=10.1038/s41550-023-02064-z |arxiv=2301.04191|bibcode=2023NatAs...7.1317L |s2cid=261439142 }}{{Cite encyclopedia |title=The Extrasolar Planet Encyclopaedia — LHS 475 b |url=https://exoplanet.eu/catalog/lhs_475_b--8580/ |access-date=2023-01-12 |encyclopedia=Extrasolar Planets Encyclopaedia |date=23 October 1995 |archive-date=20 December 2023 |archive-url=https://web.archive.org/web/20231220142928/https://exoplanet.eu/catalog/lhs_475_b--8580/ |url-status=live }} Host star also known as TOI-910{{cite arXiv |eprint=2304.01920|year=2023|title=LHS 475 b: A Venus-sized Planet Orbiting a Nearby M Dwarf |last1=Ment |first1=Kristo |last2=Charbonneau |first2=David |last3=Irwin |first3=Jonathan |last4=Winters |first4=Jennifer G. |last5=Pass |first5=Emily |last6=Shporer |first6=Avi |last7=Essack |first7=Zahra |last8=Kostov |first8=Veselin B. |last9=Kunimoto |first9=Michelle |last10=Levine |first10=Alan |last11=Seager |first11=Sara |last12=Vanderspek |first12=Roland |last13=Winn |first13=Joshua N. |class=astro-ph.EP }} Also the first exoplanet confirmed by the James Webb Space Telescope.{{cite web | url=https://astrobiology.com/2023/01/webb-discovers-lhs-475-b-an-earth-sized-rocky-planet.html | title=Webb Discovers LHS 475 b, an Earth-Sized, Rocky Planet | date=12 January 2023 }}

|0.0028 {{±|0.0016|0.0013}}

|0.09207{{±|0.00393|0.00384}}

|2.753436 ±0.000013

|0.01992 ±0.00024

|395.5{{±|2.6|2.3}}

| style="background:#FFFF00" |transit

|86.4077{{±|0.20874|0.20809}}

|0.139 ±0.005

|2960 ±55

|{{Cite journal |last1=Peterson |first1=Merrin S. |last2=Benneke |first2=Björn |last3=Collins |first3=Karen |last4=Piaulet |first4=Caroline |last5=Crossfield |first5=Ian J. M. |last6=Ali-Dib |first6=Mohamad |last7=Christiansen |first7=Jessie L. |last8=Gagné |first8=Jonathan |last9=Faherty |first9=Jackie |last10=Kite |first10=Edwin |last11=Dressing |first11=Courtney |last12=Charbonneau |first12=David |last13=Murgas |first13=Felipe |last14=Cointepas |first14=Marion |last15=Almenara |first15=Jose Manuel |date=2023-05-25 |title=A temperate Earth-sized planet with tidal heating transiting an M6 star |url=https://www.nature.com/articles/s41586-023-05934-8 |journal=Nature |language=en |volume=617 |issue=7962 |pages=701–705 |doi=10.1038/s41586-023-05934-8 |pmid=37198481 |bibcode=2023Natur.617..701P |hdl=11603/28165 |s2cid=258764768 |issn=0028-0836 |hdl-access=free |access-date=7 December 2023 |archive-date=29 December 2023 |archive-url=https://web.archive.org/web/20231229081916/https://www.nature.com/articles/s41586-023-05934-8 |url-status=live }}

|0.39 ±0.31

|

|

|1.09 ±0.17

|

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

|24000 ±2000

|0.09 ±0.07

|

|

|0.14{{±|0.13|0.08}}

|

|

|2.74{{±|0.43|0.47}}

|

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

|24400 {{±|3200|3700}}

|0.43 {{±|0.39|0.23}}

|

|{{Cite journal |last1=Olmschenk |first1=Greg |last2=Bennett |first2=David P. |last3=Bond |first3=Ian A. |last4=Zang |first4=Weicheng |last5=Jung |first5=Youn Kil |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 |last14=Silva |first14=Stela Ishitani |last15=Itow |first15=Yoshitaka |date=2023-04-01 |title=MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert |journal=The Astronomical Journal |volume=165 |issue=4 |pages=175 |doi=10.3847/1538-3881/acbcc8 |arxiv=2210.02436 |bibcode=2023AJ....165..175O |issn=0004-6256 |doi-access=free }}

|0.015 ±0.005

|

|

|1.63 ±0.35

|

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

|6500 ±1400

|0.18 ±0.05

|

|{{cite journal|arxiv=2304.02815|year=2023|title=MOA-2022-BLG-249Lb: Nearby microlensing super-Earth planet detected from high-cadence surveys |last1=Han |first1=Cheongho |last2=Gould |first2=Andrew |author3=Youn Kil Jung |last4=Bond |first4=Ian A. |last5=Zang |first5=Weicheng |last6=Chung |first6=Sun-Ju |last7=Albrow |first7=Michael D. |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=Doeon |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=Mao |first23=Shude |last24=Zhu |first24=Wei |last25=Abe |first25=Fumio |last26=Barry |first26=Richard |last27=Bennett |first27=David P. |last28=Bhattacharya |first28=Aparna |last29=Fujii |first29=Hirosame |last30=Fukui |first30=Akihiko |journal=Astronomy & Astrophysics |volume=674 |pages=A89 |doi=10.1051/0004-6361/202346166 |bibcode=2023A&A...674A..89H |s2cid=257985492 |display-authors=1 }}

|

|

|

|100

|500 ±100

| style="background:#FF6CDA" |imaging

|159.537 {{±|1.742|1.706}}

|1.5

|

|{{Cite journal |last1=Wagner |first1=Kevin |last2=Stone |first2=Jordan |last3=Skemer |first3=Andrew |last4=Ertel |first4=Steve |last5=Dong |first5=Ruobing |last6=Apai |first6=Dániel |last7=Spalding |first7=Eckhart |last8=Leisenring |first8=Jarron |last9=Sitko |first9=Michael |last10=Kratter |first10=Kaitlin |last11=Barman |first11=Travis |last12=Marley |first12=Mark |last13=Miles |first13=Brittany |last14=Boccaletti |first14=Anthony |last15=Assani |first15=Korash |date=2023-07-06 |title=Direct images and spectroscopy of a giant protoplanet driving spiral arms in MWC 758 |url=https://www.nature.com/articles/s41550-023-02028-3 |journal=Nature Astronomy |language=en |volume=7 |issue=10 |pages=1208–1217 |doi=10.1038/s41550-023-02028-3 |arxiv=2307.04021 |bibcode=2023NatAs...7.1208W |s2cid=259501395 |issn=2397-3366 |access-date=7 December 2023 |archive-date=7 September 2023 |archive-url=https://web.archive.org/web/20230907203208/https://www.nature.com/articles/s41550-023-02028-3 |url-status=live }}

|11.49 ±7.96

|

|

|1.34 ±0.47

|

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

|22000 ±5000

|0.43 ±0.29

|

|{{cite journal|arxiv=2303.16881|year=2023|title=Systematic KMTNet Planetary Anomaly Search. IX. Complete Sample of 2016 Prime-Field Planets|last1=Shin |first1=In-Gu |last2=Yee |first2=Jennifer C. |last3=Zang |first3=Weicheng |last4=Yang |first4=Hongjing |last5=Hwang |first5=Kyu-Ha |last6=Han |first6=Cheongho |last7=Gould |first7=Andrew |last8=Udalski |first8=Andrzej |last9=Bond |first9=Ian A. |last10=Albrow |first10=Michael D. |last11=Chung |first11=Sun-Ju |author12=Youn Kil Jung |last13=Ryu |first13=Yoon-Hyun |last14=Shvartzvald |first14=Yossi |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=Radosław |last27=Soszyński |first27=Igor |last28=Pietrukowicz |first28=Paweł |last29=Kozłowski |first29=Szymon |last30=Rybicki |first30=Krzysztof A. |journal=The Astronomical Journal |volume=166 |issue=3 |page=104 |doi=10.3847/1538-3881/ace96d |bibcode=2023AJ....166..104S |display-authors=1 |doi-access=free }}

|0.03 ±0.01

|

|

|1.46 ±0.16

|

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

|7000 ±2000

|0.26 ±0.11

|

|

|0.0166 {{±|0.0148|0.0086}}

|

|

|1.75{{±|0.46|0.47}}

|

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

|20870{{±|2510|4920}}

|0.38{{±|0.34|0.20}}

|

|

|7.12 ±1.47

|

|

|1.84 ±0.44

|

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

|21000 ±3000

|0.91 ±0.19

|

|

|3.34 ±1.90

|

|

|6.99 ±3.21

|

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

|18000 ±6000

|0.66 ±0.38

|

|

|0.0680 ±0.0079

|

|282.2{{±|2.2|3.7}}

|0.827 ±0.011

|

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

|56.7901{{±|0.0786|0.0783}}

|0.95 ±0.01

|5817 ±24

|{{Cite journal |last1=Brewer |first1=John M. |last2=Zhao |first2=Lily L. |last3=Fischer |first3=Debra A. |last4=Roettenbacher |first4=Rachael M. |last5=Henry |first5=Gregory W. |last6=Llama |first6=Joe |last7=Szymkowiak |first7=Andrew E. |last8=Cabot |first8=Samuel H. C. |last9=Weiss |first9=Sam A. |last10=McCarthy |first10=Chris |date=2023-08-01 |title=EXPRES. IV. Two Additional Planets Orbiting ρ Coronae Borealis Reveal Uncommon System Architecture |journal=The Astronomical Journal |volume=166 |issue=2 |pages=46 |doi=10.3847/1538-3881/acdd6f |arxiv=2306.06888 |bibcode=2023AJ....166...46B |issn=0004-6256 |doi-access=free }}

|0.0119{{±|0.0017|0.0017}}

|

|12.949 ±0.014

|0.1061 ±0.0011

|

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

|56.7901{{±|0.0786|0.0783}}

|0.95 ±0.01

|5817 ±24

|

|6.14{{±|0.39|0.42}}

|1.00 ±0.04

|76.80 ±0.06

|0.369 ±0.003

|

| style="background:#FFFF00" |transit

|937 ±6

|1.13{{±|0.02|0.03}}

|5951 ±80

|{{cite journal|arxiv=2302.10838|year=2023|title=A 2:1 Mean-motion Resonance Super-Jovian Pair Revealed by TESS, FEROS, and HARPS|last1=Bozhilov |first1=Vladimir |last2=Antonova |first2=Desislava |last3=Hobson |first3=Melissa J. |last4=Brahm |first4=Rafael |last5=Jordan |first5=Andres |last6=Henning |first6=Thomas |last7=Eberhardt |first7=Jan |last8=Rojas |first8=Felipe I. |last9=Batygin |first9=Konstantin |last10=Torres-Miranda |first10=Pascal |last11=Stassun |first11=Keivan G. |last12=Millholland |first12=Sarah C. |last13=Stoeva |first13=Denitza |last14=Minev |first14=Milen |last15=Espinoza |first15=Nestor |last16=Ricker |first16=George R. |last17=Latham |first17=David W. |last18=Dragomir |first18=Diana |last19=Kunimoto |first19=Michelle |last20=Jenkins |first20=Jon M. |last21=Ting |first21=Eric B. |last22=Seager |first22=Sara |last23=Winn |first23=Joshua N. |author24=Jesus Noel Villasenor |last25=Bouma |first25=Luke G. |last26=Medina |first26=Jennifer |last27=Trifonov |first27=Trifon |journal=The Astrophysical Journal Letters |volume=946 |issue=2 |pages=L36 |doi=10.3847/2041-8213/acbd4f |bibcode=2023ApJ...946L..36B |s2cid=257050718 |doi-access=free }}

|8.02 ±0.18

|

|155.3 ±0.7

|0.591{{±|0.005|0.006}}

|

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

|937 ±6

|1.13{{±|0.02|0.03}}

|5951 ±80

|

|0.06

|0.55

|4.21285

|0.0622 ±0.0049

|

| style="background:#FFFF00" |transit

|1810 ±20

|1.21{{±|0.06|0.05}}

|4694{{±|27|20}}

|Still have an atmosphere despite high temperatures and low mass{{cite arXiv|eprint=2303.06728|year=2023|title=An unlikely survivor: a low-density hot Neptune orbiting a red giant star|last1=Grunblatt |first1=Samuel |last2=Saunders |first2=Nicholas |last3=Huber |first3=Daniel |last4=Thorngren |first4=Daniel |last5=Vissapragada |first5=Shreyas |last6=Yoshida |first6=Stephanie |last7=Schlaufman |first7=Kevin |last8=Giacalone |first8=Steven |last9=MacDougall |first9=Mason |last10=Chontos |first10=Ashley |last11=Turtelboom |first11=Emma |last12=Beard |first12=Corey |last13=Akana Murphy |first13=Joseph M. |last14=Rice |first14=Malena |last15=Isaacson |first15=Howard |last16=Angus |first16=Ruth |last17=Howard |first17=Andrew W. |class=astro-ph.EP }}

|0.0208

|0.219{{±|0.019|0.011}}

|11.070850{{±|0.000024|0.000030}}

|

|561.17

| style="background:#FFFF00" |transit

|138.4

|0.6900 ±0.0852

|4570 ±50

|{{cite journal|arxiv=2301.09865|year=2023|title=VaTEST. II. Statistical Validation of 11 TESS-detected Exoplanets Orbiting K-type Stars|last1=Mistry |first1=Priyashkumar |last2=Pathak |first2=Kamlesh |last3=Prasad |first3=Aniket |last4=Lekkas |first4=Georgios |last5=Bhattarai |first5=Surendra |last6=Gharat |first6=Sarvesh |last7=Maity |first7=Mousam |last8=Kumar |first8=Dhruv |last9=Furan |first9=Elise |last10=Howell |first10=Steve |last11=Ciardi |first11=David |last12=Bieryla |first12=Allyson |last13=Matthews |first13=Elisabeth |last14=Gonzales |first14=Erica |last15=Ziegler |first15=Carl |last16=Crossfield |first16=Ian |last17=Eastman |first17=Jason |last18=Giacalone |first18=Steven |last19=Dressing |first19=Courtney |last20=Beichman |first20=Charles |last21=Soubkiou |first21=Abderahmane |last22=Benkhaldoun |first22=Zouhair |last23=Schlieder |first23=Joshua |last24=Goliguzova |first24=Maria V. |last25=Strakhov |first25=Ivan A. |last26=Everett |first26=Mark |last27=Gnilka |first27=Crystal |last28=Lester |first28=Katie |last29=Littlefield |first29=Colin |last30=Scott |first30=Nic |journal=The Astronomical Journal |volume=166 |issue=1 |page=9 |doi=10.3847/1538-3881/acd548 |bibcode=2023AJ....166....9M |s2cid=258685555 |display-authors=1 |doi-access=free }}

|0.1452{{±|0.0085|0.0240}}

|0.6339{{±|0.0079|0.0092}}

|4.532000 ±0.000002

|0.0539{{±|0.0043|0.0036}}

|895.10{{±|32.14|33.86}}

| style="background:#FFFF00" |transit

|313.873{{±|1.886|1.864}}

|0.822 ±0.040

|4994 ±50

|{{Cite journal |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=Bieryla |first10=Allyson |last11=Eastman |first11=Jason D |last12=Esquerdo |first12=Gilbert A |last13=Lucero |first13=Jennifer P |date=2023-03-02 |title=VaTEST I: validation of sub-Saturn exoplanet TOI-181b in narrow orbit from its host star |url=https://academic.oup.com/mnras/article/521/1/1066/7049116 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=521 |issue=1 |pages=1066–1078 |doi=10.1093/mnras/stad543 |doi-access=free |issn=0035-8711|arxiv=2211.07957 }}

|

|0.128 ±0.007

|10.21520 ±0.00006

|0.100 ±0.006

|368 ±26

| style="background:#FFFF00" |transit

|77.38461 ±0.08659

|0.467 ±0.023

|3650 ±75

|

|0.17 ±0.02

|0.810 ±0.005

|104.854{{±|0.001|0.002}}

|0.4254 ±0.0020

|

| style="background:#FFFF00" |transit

|333.561{{±|0.623|0.620}}

|0.936{{±|0.003|0.005}}

|5255{{±|12|10}}

|{{Cite journal |last1=Hobson |first1=Melissa J. |last2=Trifonov |first2=Trifon |last3=Henning |first3=Thomas |last4=Jordán |first4=Andrés |last5=Rojas |first5=Felipe |last6=Espinoza |first6=Nestor |last7=Brahm |first7=Rafael |last8=Eberhardt |first8=Jan |last9=Jones |first9=Matías I. |last10=Mekarnia |first10=Djamel |last11=Kossakowski |first11=Diana |last12=Schlecker |first12=Martin |last13=Tala Pinto |first13=Marcelo |last14=Torres Miranda |first14=Pascal José |last15=Abe |first15=Lyu |date=2023-11-01 |title=TOI-199 b: A Well-characterized 100 day Transiting Warm Giant Planet with TTVs Seen from Antarctica |journal=The Astronomical Journal |volume=166 |issue=5 |pages=201 |doi=10.3847/1538-3881/acfc1d |arxiv=2309.14915 |bibcode=2023AJ....166..201H |issn=0004-6256 |doi-access=free }}

|0.28{{±|0.02|0.01}}

|

|273.69{{±|0.26|0.22}}

|0.807 ±0.003

|

| style="background:#FFFF00" |transit

|333.561{{±|0.623|0.620}}

|0.936{{±|0.003|0.005}}

|5255{{±|12|10}}

|

|0.0107{{±|0.00145|0.00142}}

|0.1278{{±|0.00765|0.00784}}

|1.2730988 ±0.0000029

|0.02118 ±0.00038

|1311 ±28

|style="background:#FFFF00"|transit

|261.328 ±0.312

|0.79 ±0.022

|5059 ±89

|{{cite arXiv |last1=Priyashkumar |first1=Mistry |title=VaTEST III: Validation of 8 Potential Super-Earths from TESS Data |date=2023-11-01 |eprint=2311.00688 |last2=Prasad |first2=Aniket |last3=Maity |first3=Mousam |last4=Pathak |first4=Kamlesh |last5=Gharat |first5=Sarvesh |last6=Lekkas |first6=Georgios |last7=Bhattarai |first7=Surendra |last8=Kumar |first8=Dhruv |last9=Lissauer |first9=Jack J. |last10=Twicken |first10=Joseph D. |last11=Soubkiou |first11=Abderahmane |last12=Pozuelos |first12=Francisco J. |last13=Jenkins |first13=Jon |last14=Horne |first14=Keith |last15=Giacalone |first15=Steven |last16=Barkaoui |first16=Khalid |last17=Timmermans |first17=Mathilde |last18=Watkins |first18=Cristilyn N. |last19=Sefako |first19=Ramotholo |last20=Collins |first20=Karen A. |last21=Shporer |first21=Avi |last22=Benkhaldoun |first22=Zouhair |last23=Stockdale |first23=Chris |last24=Jehin |first24=Emmanuël |last25=Murgas |first25=Felipe |last26=Paegert |first26=Martin |last27=Lund |first27=Michael B. |last28=Narita |first28=Norio |last29=Schwarz |first29=Richard P. |last30=Goeke |first30=Robert F. |last31=Tan |first31=Thiam-Guan |last32=Kawai |first32=Yugo |class=astro-ph.EP }}

|0.00843 ±0.00094

|0.136 ±0.011

|7.397225{{±|0.000026|0.000023}}

|0.0559 ±0.0013

|458 ±20

| style="background:#FFFF00" |transit

|71.8644{{±|0.0334|0.0333}}

|0.428 ±0.029

|3433 ±100

|{{Cite journal |last1=Castro-González |first1=A. |last2=Demangeon |first2=O. D. S. |last3=Lillo-Box |first3=J. |last4=Lovis |first4=C. |last5=Lavie |first5=B. |last6=Adibekyan |first6=V. |last7=Acuña |first7=L. |last8=Deleuil |first8=M. |last9=Aguichine |first9=A. |last10=Zapatero Osorio |first10=M. R. |last11=Tabernero |first11=H. M. |last12=Davoult |first12=J. |last13=Alibert |first13=Y. |last14=Santos |first14=N. |last15=Sousa |first15=S. G. |date=July 2023 |title=An unusually low-density super-Earth transiting the bright early-type M-dwarf GJ 1018 (TOI-244) |url=https://www.aanda.org/10.1051/0004-6361/202346550 |journal=Astronomy & Astrophysics |volume=675 |pages=A52 |doi=10.1051/0004-6361/202346550 |arxiv=2305.04922 |bibcode=2023A&A...675A..52C |s2cid=258556864 |issn=0004-6361}}

|

|0.185 ±0.013

|11.14529 ±0.00003

|0.163 ±0.002

|584 ±45

| style="background:#FFFF00" |transit

|143.287{{±|0.383|0.381}}

|0.913 ±0.029

|5310 ±124

|

|0.0308

|0.276{{±|0.026|0.013}}

|3.994086{{±|0.000008|0.000009}}

|

|739.9

| style="background:#FFFF00" |transit

|211.7

|0.5204 ±0.0203

|3748 ±64

|

|0.180 ±0.005

|0.285{{±|0.014|0.010}}

|0.777038 ±0.000001

|0.0159 ±0.0001

|1871{{±|30|25}}

| style="background:#FFFF00" |transit

|726.847{{±|12.231|11.836}}

|0.88 ±0.02

|5251 ±71

|{{Cite journal |last1=Osborn |first1=Ares |last2=Armstrong |first2=David J |last3=Fernández Fernández |first3=Jorge |last4=Knierim |first4=Henrik |last5=Adibekyan |first5=Vardan |last6=Collins |first6=Karen A |last7=Delgado Mena |first7=Elisa |last8=Fridlund |first8=Malcolm |last9=Gomes da Silva |first9=João |last10=Hellier |first10=Coel |last11=Jackson |first11=David G |last12=King |first12=George W |last13=Lillo-Box |first13=Jorge |last14=Matson |first14=Rachel A |last15=Matthews |first15=Elisabeth C |date=2023-09-21 |title=TOI-332 b: a super dense Neptune found deep within the Neptunian desert |url=https://academic.oup.com/mnras/article/526/1/548/7257597 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=526 |issue=1 |pages=548–566 |doi=10.1093/mnras/stad2575 |issn=0035-8711 |doi-access=free |access-date=9 December 2023 |archive-date=9 December 2023 |archive-url=https://web.archive.org/web/20231209125358/https://academic.oup.com/mnras/article/526/1/548/7257597 |url-status=live |arxiv=2308.12137 }}

|

|0.247 ±0.018

|17.96360 ±0.00004

|0.133 ±0.006

|609 ±61

| style="background:#FFFF00" |transit

|187.205{{±|0.270|0.269}}

|0.960 ±0.130

|5225 ±70

|{{Cite journal |last1=Oddo |first1=Dominic |last2=Dragomir |first2=Diana |last3=Brandeker |first3=Alexis |last4=Osborn |first4=Hugh P. |last5=Collins |first5=Karen |last6=Stassun |first6=Keivan G. |last7=Astudillo-Defru |first7=Nicola |last8=Bieryla |first8=Allyson |last9=Howell |first9=Steve B. |last10=Ciardi |first10=David R. |last11=Quinn |first11=Samuel |last12=Almenara |first12=Jose M. |last13=Briceño |first13=César |last14=Collins |first14=Kevin I. |last15=Colón |first15=Knicole D. |date=2023-03-01 |title=Characterization of a Set of Small Planets with TESS and CHEOPS and an Analysis of Photometric Performance |journal=The Astronomical Journal |volume=165 |issue=3 |pages=134 |doi=10.3847/1538-3881/acb4e3 |arxiv=2301.08162 |bibcode=2023AJ....165..134O |issn=0004-6256 |doi-access=free }}

|

|0.387 ±0.026

|12.19148 ±0.00003

|0.119 ±0.008

|660 ±70

| style="background:#FFFF00" |transit

|425.50{{±|1.31|1.30}}

|0.87 ±0.09

|5190 ±90

|

|0.435{{±|0.086|0.082}}

|1.693{{±|0.052|0.057}}

|4.6615983{{±|0.0000025|0.0000016}}

|0.0678{{±|0.0031|0.0026}}

|1666 ±24

| style="background:#FFFF00" |transit

|1155 ±6

|1.449 ±0.087

|6850 ±100

|{{cite journal|arxiv=2303.15080|year=2023|title=Three Saturn-mass planets transiting F-type stars revealed with TESS and HARPS|last1=Psaridi |first1=Angelica |last2=Bouchy |first2=François |last3=Lendl |first3=Monika |last4=Akinsanmi |first4=Babatunde |last5=Stassun |first5=Keivan G. |last6=Smalley |first6=Barry |last7=Armstrong |first7=David J. |last8=Howard |first8=Saburo |last9=Ulmer-Moll |first9=Solène |last10=Grieves |first10=Nolan |last11=Barkaoui |first11=Khalid |last12=Rodriguez |first12=Joseph E. |last13=Bryant |first13=Edward M. |last14=Suárez |first14=Olga |last15=Guillot |first15=Tristan |last16=Evans |first16=Phil |last17=Attia |first17=Omar |last18=Wittenmyer |first18=Robert A. |last19=Yee |first19=Samuel W. |last20=Collins |first20=Karen A. |last21=Zhou |first21=George |last22=Galland |first22=Franck |last23=Parc |first23=Léna |last24=Udry |first24=Stéphane |last25=Figueira |first25=Pedro |last26=Ziegler |first26=Carl |last27=Mordasini |first27=Christoph |last28=Winn |first28=Joshua N. |last29=Seager |first29=Sara |last30=Jenkins |first30=Jon M. |journal=Astronomy & Astrophysics |volume=675 |pages=A39 |doi=10.1051/0004-6361/202346406 |s2cid=257766828 |display-authors=1 }}

|0.303{{±|0.069|0.072}}

|0.824{{±|0.028|0.029}}

|6.402513{{±|0.000031|0.000054}}

|0.0708{{±|0.0052|0.0059}}

|1388 ±22

| style="background:#FFFF00" |transit

|400.2 ±0.6

|1.313 ±0.079

|6400 ±100

|

|0.0308{{±|0.0047}}

|0.232{{±|0.015}}

|3.94515{{±|0.00002}}

|0.047{{±|0.001}}

|1235{{±|37}}

| style="background:#FFFF00" |transit

|465.970{{±|2.789|2.759}}

|0.90{{±|0.06}}

|5600{{±|110}}

|

|0.0760

|0.470{{±|0.008|0.009}}

|3.633575 ±0.000001

|

|676.15

| style="background:#FFFF00" |transit

|

|0.5399 ±0.0204

|3765 ±65

|

|0.0025730809{{Cite web |title=Exoplanet-catalog |url=https://exoplanets.nasa.gov/exoplanet-catalog/8729/toi-700-e/ |access-date=2023-11-09 |website=Exoplanet Exploration: Planets Beyond our Solar System |language=en |archive-date=1 October 2023 |archive-url=https://web.archive.org/web/20231001052205/https://exoplanets.nasa.gov/exoplanet-catalog/8729/toi-700-e/ |url-status=live }}

|0.08502{{±|0.00794|0.00669}}

|27.80978{{±|0.00046|0.0004}}

|0.134 ±0.0022

|350{{Cite web |date=2023-02-15 |title=TOI-700 e: NASA Discovers New Earth-Like World Around Distant Star |url=https://www.azoquantum.com/Article.aspx?ArticleID=407 |access-date=2023-11-09 |website=AZoQuantum.com |language=en |archive-date=9 November 2023 |archive-url=https://web.archive.org/web/20231109051117/https://www.azoquantum.com/Article.aspx?ArticleID=407 |url-status=live }}

| style="background:#FFFF00" |transit

|101.52

|0.416 ±0.01

|3480 ±135

|Habitable zone planet{{cite journal|arxiv=2301.03617|year=2023|title=A Second Earth-sized Planet in the Habitable Zone of the M Dwarf, TOI-700|last1=Gilbert |first1=Emily A. |last2=Vanderburg |first2=Andrew |last3=Rodriguez |first3=Joseph E. |last4=Hord |first4=Benjamin J. |last5=Clement |first5=Matthew S. |last6=Barclay |first6=Thomas |last7=Quintana |first7=Elisa V. |last8=Schlieder |first8=Joshua E. |last9=Kane |first9=Stephen R. |last10=Jenkins |first10=Jon M. |last11=Twicken |first11=Joseph D. |last12=Kunimoto |first12=Michelle |last13=Vanderspek |first13=Roland |last14=Arney |first14=Giada N. |last15=Charbonneau |first15=David |last16=Günther |first16=Maximilian N. |last17=Huang |first17=Chelsea X. |last18=Isopi |first18=Giovanni |last19=Kostov |first19=Veselin B. |last20=Kristiansen |first20=Martti H. |last21=Latham |first21=David W. |last22=Mallia |first22=Franco |last23=Mamajek |first23=Eric E. |last24=Mireles |first24=Ismael |last25=Quinn |first25=Samuel N. |last26=Ricker |first26=George R. |last27=Schulte |first27=Jack |last28=Seager |first28=S. |last29=Suissa |first29=Gabrielle |last30=Winn |first30=Joshua N. |journal=The Astrophysical Journal Letters |volume=944 |issue=2 |pages=L35 |doi=10.3847/2041-8213/acb599 |bibcode=2023ApJ...944L..35G |s2cid=255570018 |display-authors=1 |doi-access=free }}{{Cite encyclopedia |title=The Extrasolar Planet Encyclopaedia — TOI-700 e |url=https://exoplanet.eu/catalog/toi_700_e--8579/ |access-date=2023-01-12 |encyclopedia=Extrasolar Planets Encyclopaedia |date=23 October 1995 }}

|

|0.1383 ±0.0057

|19.288004{{±|0.000027|0.000024}}

|0.0830 ±0.0027

|234 ±12

| style="background:#FFFF00" |transit

|138.306{{±|0.280|0.279}}

|0.240 ±0.012

|3075 ±75

|{{Cite journal |last1=Dransfield |first1=Georgina |last2=Timmermans |first2=Mathilde |last3=Triaud |first3=Amaury H M J |last4=Dévora-Pajares |first4=Martín |last5=Aganze |first5=Christian |last6=Barkaoui |first6=Khalid |last7=Burgasser |first7=Adam J |last8=Collins |first8=Karen A |last9=Cointepas |first9=Marion |last10=Ducrot |first10=Elsa |last11=Günther |first11=Maximilian N |last12=Howell |first12=Steve B |last13=Murray |first13=Catriona A |last14=Niraula |first14=Prajwal |last15=Rackham |first15=Benjamin V |date=2023-10-28 |title=A 1.55 R⊕ habitable-zone planet hosted by TOI-715, an M4 star near the ecliptic South Pole |url=https://academic.oup.com/mnras/article/527/1/35/7172075 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=527 |issue=1 |pages=35–52 |doi=10.1093/mnras/stad1439 |issn=0035-8711 |doi-access=free |access-date=9 December 2023 |archive-date=9 December 2023 |archive-url=https://web.archive.org/web/20231209182321/https://academic.oup.com/mnras/article/527/1/35/7172075 |url-status=live |arxiv=2305.06206 }}

|0.0180 ±0.0022

|0.178 ±0.008

|4.884765{{±|0.000019|0.000024}}

|0.0618{{±|0.0036|0.0039}}

|1055.8{{±|36.2|31.3}}

| style="background:#FFFF00" |transit

|245.5 ±0.2

|0.956{{±|0.050|0.026}}

|5585 ±60

|{{cite journal|arxiv=2304.06655|year=2023|title=TOI-733 b: A planet in the small-planet radius valley orbiting a Sun-like star |last1=Georgieva |first1=Iskra Y. |last2=Persson |first2=Carina M. |last3=Goffo |first3=Elisa |last4=Acuña |first4=Lorena |last5=Aguichine |first5=Artyom |last6=Serrano |first6=Luisa M. |last7=Lam |first7=Kristine W. F. |last8=Gandolfi |first8=Davide |last9=Collins |first9=Karen A. |last10=Howell |first10=Steven B. |last11=Dai |first11=Fei |last12=Fridlund |first12=Malcolm |last13=Korth |first13=Judith |last14=Deleuil |first14=Magali |last15=Barragán |first15=Oscar |last16=Cochran |first16=William D. |last17=Csizmadia |first17=Szilárd |last18=Deeg |first18=Hans J. |last19=Guenther |first19=Eike |last20=Hatzes |first20=Artie P. |last21=Jenkins |first21=Jon M. |last22=Livingston |first22=John |last23=Luque |first23=Rafael |last24=Mousis |first24=Olivier |last25=Osborne |first25=Hannah L. M. |last26=Palle |first26=Enric |last27=Redfield |first27=Seth |author28=Vincent Van Eylen |last29=Twicken |first29=Joseph D. |last30=Winn |first30=Joshua N. |journal=Astronomy & Astrophysics |volume=674 |pages=A117 |doi=10.1051/0004-6361/202345961 |bibcode=2023A&A...674A.117G |s2cid=258108052 |display-authors=1 }}

|0.00881{{±|0.00629|0.00283}}

|0.127{{±|0.00964|0.00767}}

|2.326021 ±0.000001

|0.0207 ±0.0008

|527.19 ±22.08

| style="background:#FFFF00" |transit

|82.452 ±0.130

|0.220{{±|0.024|0.023}}

|3201{{±|100|95}}

|

|2.8 ±0.2

|1.37 ±0.04

|4.633611 ±0.000001

|0.060 ±0.003

|1561{{±|33|32}}

| style="background:#FFFF00" |transit

|527.536{{±|3.663|3.614}}

|1.40 ±0.05

|6643 ±150

|{{Cite journal |last1=Clark |first1=Jake T. |last2=Addison |first2=Brett C. |last3=Okumura |first3=Jack |last4=Vach |first4=Sydney |last5=Errico |first5=Adriana |last6=Heitzmann |first6=Alexis |last7=Rodriguez |first7=Joseph E. |last8=Wright |first8=Duncan J. |last9=Clerté |first9=Mathieu |last10=Brown |first10=Carolyn J. |last11=Fetherolf |first11=Tara |last12=Wittenmyer |first12=Robert A. |last13=Plavchan |first13=Peter |last14=Kane |first14=Stephen R. |last15=Horner |first15=Jonathan |date=2023-05-01 |title=Spinning up a Daze: TESS Uncovers a Hot Jupiter Orbiting the Rapid Rotator TOI-778 |journal=The Astronomical Journal |volume=165 |issue=5 |pages=207 |doi=10.3847/1538-3881/acc3a0 |arxiv=2212.08242 |bibcode=2023AJ....165..207C |issn=0004-6256 |doi-access=free }}

|0.03043{{±|0.00261|0.00258}}

|0.172{{±|0.010|0.008}}

|2.7970365{{±|0.0000031|0.0000030}}

|0.038 ±0.001

|

| style="background:#FFFF00" |transit

|210.696{{±|0.360|0.359}}

|0.910 ±0.100

|5558 ±100

|Also known as HD 307842.{{Cite journal |last1=Hua |first1=Xinyan |last2=Wang |first2=Sharon Xuesong |last3=Teske |first3=Johanna K. |last4=Gan |first4=Tianjun |last5=Shporer |first5=Avi |last6=Zhou |first6=George |last7=Stassun |first7=Keivan G. |last8=Rabus |first8=Markus |last9=Howell |first9=Steve B. |last10=Ziegler |first10=Carl |last11=Lissauer |first11=Jack J. |last12=Winn |first12=Joshua N. |last13=Jenkins |first13=Jon M. |last14=Ting |first14=Eric B. |last15=Collins |first15=Karen A. |date=2023-07-01 |title=A Transiting Super-Earth in the Radius Valley and an Outer Planet Candidate Around HD 307842 |journal=The Astronomical Journal |volume=166 |issue=1 |pages=32 |doi=10.3847/1538-3881/acd751 |arxiv=2306.14655 |bibcode=2023AJ....166...32H |issn=0004-6256 |doi-access=free }}

|0.0143{{±|0.0029|0.0027}}

|0.1520 ±0.0060

|3.81673 ±0.00001

|0.04220 ±0.00093

|871 ±36

| style="background:#FFFF00" |transit

|89.7009{{±|0.0959|0.0956}}

|0.665 ±0.010

|4552 ±154

|{{Cite journal |last1=Hawthorn |first1=Faith |last2=Bayliss |first2=Daniel |last3=Wilson |first3=Thomas G |last4=Bonfanti |first4=Andrea |last5=Adibekyan |first5=Vardan |last6=Alibert |first6=Yann |last7=Sousa |first7=Sérgio G |last8=Collins |first8=Karen A |last9=Bryant |first9=Edward M |last10=Osborn |first10=Ares |last11=Armstrong |first11=David J |last12=Abe |first12=Lyu |last13=Acton |first13=Jack S |last14=Addison |first14=Brett C |last15=Agabi |first15=Karim |date=2023-02-15 |title=TOI-836: A super-Earth and mini-Neptune transiting a nearby K-dwarf |url=https://academic.oup.com/mnras/article/520/3/3649/7033445 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=520 |issue=3 |pages=3649–3668 |doi=10.1093/mnras/stad306 |doi-access=free |issn=0035-8711 |access-date=9 December 2023 |archive-date=19 May 2023 |archive-url=https://web.archive.org/web/20230519072428/https://academic.oup.com/mnras/article/520/3/3649/7033445 |url-status=live |arxiv=2208.07328 }}

|0.0302{{±|0.0085|0.0027}}

|0.2308 ±0.0079

|8.59545 ±0.00001

|0.0750 ±0.0016

|665 ±27

| style="background:#FFFF00" |transit

|89.7009{{±|0.0959|0.0956}}

|0.665 ±0.010

|4552 ±154

|

|1.10{{±|0.08|0.07}}

|1.255 ±0.039

|3.2797178 ±0.0000014

|0.04435{{±|0.00100|0.00098}}

|1529{{±|23|22}}

| style="background:#FFFF00" |transit

|816.987{{±|4.951|4.892}}

|1.081{{±|0.076|0.070}}

|5842{{±|84|79}}

|{{Cite journal |last1=Hagelberg |first1=J. |last2=Nielsen |first2=L. D. |last3=Attia |first3=O. |last4=Bourrier |first4=V. |last5=Pearce |first5=L. |last6=Venturini |first6=J. |last7=Winn |first7=J. N. |last8=Bouchy |first8=F. |last9=Bouma |first9=L. G. |last10=Briceño |first10=C. |last11=Collins |first11=K. A. |last12=Davis |first12=A. B. |last13=Eastman |first13=J. D. |last14=Evans |first14=P. |last15=Falk |first15=B. |date=November 2023 |title=TOI-858 B b: A hot Jupiter on a polar orbit in a loose binary |url=https://www.aanda.org/10.1051/0004-6361/202244940 |journal=Astronomy & Astrophysics |volume=679 |pages=A70 |doi=10.1051/0004-6361/202244940 |arxiv=2309.11390 |bibcode=2023A&A...679A..70H |s2cid=262064260 |issn=0004-6361}}

|0.0120{{±|0.00849|0.00440}}

|0.148{{±|0.0102|0.0101}}

|14.362565 ±0.00009

|0.1054 ±0.0021

|621 ±16.05

| style="background:#FFFF00" |transit

|221.917 ±0.489

|0.758{{±|0.046|0.044}}

|4929{{±|80|75}}

|

|0.050773{{±|0.012938|0.012708}}

|0.2842 ±0.0138

|3.183792 ±0.000007

|0.041657 ±0.000002

|1317 ±38

| style="background:#FFFF00" |transit

|573.214{{±|0.638|0.634}}

|0.950 ±0.010

|5626 ±61

|{{Cite journal |last1=Hawthorn |first1=Faith |last2=Bayliss |first2=Daniel |last3=Armstrong |first3=David J |last4=Fernández Fernández |first4=Jorge |last5=Osborn |first5=Ares |last6=Sousa |first6=Sérgio G |last7=Adibekyan |first7=Vardan |last8=Davoult |first8=Jeanne |last9=Collins |first9=Karen A |last10=Alibert |first10=Yann |last11=Barros |first11=Susana C C |last12=Bouchy |first12=François |last13=Brogi |first13=Matteo |last14=Ciardi |first14=David R |last15=Daylan |first15=Tansu |date=2023-07-24 |title=TOI-908: a planet at the edge of the Neptune desert transiting a G-type star |url=https://academic.oup.com/mnras/article/524/3/3877/7205300 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=524 |issue=3 |pages=3877–3893 |doi=10.1093/mnras/stad1840 |issn=0035-8711 |doi-access=free |access-date=9 December 2023 |archive-date=9 December 2023 |archive-url=https://web.archive.org/web/20231209185716/https://academic.oup.com/mnras/article/524/3/3877/7205300 |url-status=live |hdl=10023/28054 |hdl-access=free }}

|0.0208

|0.219{{±|0.011|0.009}}

|11.098644{{±|0.000587|0.000581}}

|

|712.01

| style="background:#FFFF00" |transit

|212.1

|0.8200 ±0.0973

|4969 ±129

|

|0.0532 ±0.0053

|0.256{{±|0.026|0.021}}

|9.139703{{±|0.00062|0.00063}}

|0.09103{{±|0.00062|0.00063}}

|1135

| style="background:#FFFF00" |transit

|423.365{{±|1.826|1.810}}

|1.204 ±0.025

|6146 ±62

|{{Cite journal |last1=Armstrong |first1=David J |last2=Osborn |first2=Ares |last3=Adibekyan |first3=Vardan |last4=Delgado-Mena |first4=Elisa |last5=Hojjatpanah |first5=Saeed |last6=Howell |first6=Steve B |last7=Hoyer |first7=Sergio |last8=Knierim |first8=Henrik |last9=Sousa |first9=Sérgio G |last10=Stassun |first10=Keivan G |last11=Veras |first11=Dimitri |last12=Anderson |first12=David R |last13=Bayliss |first13=Daniel |last14=Bouchy |first14=François |last15=Burke |first15=Christopher J |date=2023-07-29 |title=Discovery and characterization of two Neptune-mass planets orbiting HD 212729 with TESS |url=https://academic.oup.com/mnras/article/524/4/5804/7227347 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=524 |issue=4 |pages=5804–5816 |doi=10.1093/mnras/stad2183 |issn=0035-8711 |doi-access=free |access-date=8 December 2023 |archive-date=8 December 2023 |archive-url=https://web.archive.org/web/20231208000947/https://academic.oup.com/mnras/article/524/4/5804/7227347 |url-status=live |arxiv=2307.11566 }}

|0.108{{±|0.013|0.012}}

|

|35.806{{±|0.453|0.381}}

|0.2263{{±|0.0024|0.0023}}

|719

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

|423.365{{±|1.826|1.810}}

|1.204 ±0.025

|6146 ±62

|

|0.456{{±|0.055|0.051}}

|0.767{{±|0.045|0.041}}

|2.310644 ±0.000001

|0.03428 ±0.00055

|1391{{±|38|37}}

| style="background:#FFFF00" |transit

|488.149{{±|2.136|2.117}}

|1.007{{±|0.050|0.048}}

|5446{{±|51|48}}

|{{Cite arXiv |last1=Wang |first1=Jia-Qi |last2=Jiang |first2=Xiao-Jun |last3=Zheng |first3=Jie |last4=Kellermann |first4=Hanna |last5=Riffeser |first5=Arno |last6=Wang |first6=Liang |last7=Collins |first7=Karen A. |last8=Bieryla |first8=Allyson |last9=Buchhave |first9=Lars A. |last10=Howell |first10=Steve B. |last11=Furlan |first11=Elise |last12=Girardin |first12=Eric |last13=Gregorio |first13=Joao |last14=Jensen |first14=Eric |last15=Murgas |first15=Felipe |date=2023 |title=Confirmation of a Sub-Saturn-size transiting exoplanet orbiting a G dwarf: TOI-1194 b and a very low mass companion star: TOI-1251 B from TESS |class=astro-ph.EP |eprint=2310.12458}}

|<3.5

|0.260{{±|0.012|0.011}}

|91.68278{{±|0.00032|0.00041}}

|0.387{{±|0.026|0.023}}

|440 ±60

| style="background:#FFFF00" |transit

|451.437{{±|1.262|1.259}}

|0.930 ±0.220

|5592 ±50

|{{Cite journal |last1=Mann |first1=Christopher |last2=Lafreniére |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 |date=2023-05-01 |title=Validation of TOI-1221 b: A Warm Sub-Neptune Exhibiting Transit Timing Variations around a Sun-like Star |journal=The Astronomical Journal |volume=165 |issue=5 |pages=217 |doi=10.3847/1538-3881/acc8d4 |arxiv=2209.13651 |bibcode=2023AJ....165..217M |issn=0004-6256 |doi-access=free }}

|0.205 ±0.037

|

|215.5 ±3.3

|0.794 ±0.016

|

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

|1318 ±5

|1.13+0.31

|6160

|Circumbinary planet{{cite journal|arxiv=2301.10794|year=2023|title=Radial-velocity discovery of a second planet in the TOI-1338/BEBOP-1 circumbinary system|last1=Standing |first1=Matthew R. |last2=Sairam |first2=Lalitha |last3=Martin |first3=David V. |last4=Triaud |first4=Amaury H. M. J. |last5=Correia |first5=Alexandre C. M. |last6=Coleman |first6=Gavin A. L. |last7=Baycroft |first7=Thomas A. |last8=Kunovac |first8=Vedad |last9=Boisse |first9=Isabelle |author10=Andrew Collier Cameron |last11=Dransfield |first11=Georgina |last12=Faria |first12=João P. |last13=Gillon |first13=Michaël |last14=Hara |first14=Nathan C. |last15=Hellier |first15=Coel |last16=Howard |first16=Jonathan |last17=Lane |first17=Ellie |last18=Mardling |first18=Rosemary |last19=Maxted |first19=Pierre F. L. |last20=Miller |first20=Nicola J. |last21=Nelson |first21=Richard P. |last22=Orosz |first22=Jerome A. |last23=Pepe |first23=Franscesco |last24=Santerne |first24=Alexandre |last25=Sebastian |first25=Daniel |last26=Udry |first26=Stéphane |last27=Welsh |first27=William F. |journal=Nature Astronomy |volume=7 |issue=6 |pages=702–714 |doi=10.1038/s41550-023-01948-4 |bibcode=2023NatAs...7..702S |s2cid=259138442 }}

|1.69 ±0.20

|1.5

|4.4247110 ±0.0000016

|0.05804 ±0.00020

|

| style="background:#FFFF00" |transit

|454.937{{±|1.363|1.360}}

|1.331 ±0.014

|6306 ±32

|{{Cite journal |last1=Galazutdinov |first1=G A |last2=Baluev |first2=R V |last3=Valyavin |first3=G |last4=Aitov |first4=V |last5=Gadelshin |first5=D |last6=Valeev |first6=A |last7=Sendzikas |first7=E |last8=Sokov |first8=E |last9=Mitiani |first9=G |last10=Burlakova |first10=T |last11=Yakunin |first11=I |last12=Antonyuk |first12=K A |last13=Vlasyuk |first13=V |last14=Romanyuk |first14=I |last15=Rzaev |first15=A |date=2023-08-09 |title=Doppler confirmation of TESS planet candidate TOI−1408.01: grazing transit and likely eccentric orbit |url=https://academic.oup.com/mnrasl/article/526/1/L111/7260865 |journal=Monthly Notices of the Royal Astronomical Society: Letters |language=en |volume=526 |issue=1 |pages=L111–L115 |doi=10.1093/mnrasl/slad127 |doi-access=free |issn=1745-3925 |arxiv=2309.03009 |access-date=8 December 2023 |archive-date=8 December 2023 |archive-url=https://web.archive.org/web/20231208002505/https://academic.oup.com/mnrasl/article/526/1/L111/7260865 |url-status=live }}

|0.0334

|0.290{{±|0.014|0.010}}

|1.216901 ±0.000038

|

|1181.44

| style="background:#FFFF00" |transit

|236.8

|0.7960 ±0.0370

|4668 ±50

|

|0.0109 ±0.0015

|0.145 ±0.007

|1.0697568 ±0.0000028

|0.0190 ±0.0003

|1517 ±39

| style="background:#FFFF00" |transit

|179.430{{±|0.253|0.252}}

|0.798{{±|0.035|0.044}}

|4884 ±70

|{{Cite journal |last1=Deeg |first1=H. J. |last2=Georgieva |first2=I. Y. |last3=Nowak |first3=G. |last4=Persson |first4=C. M. |last5=Cale |first5=B. L. |last6=Murgas |first6=F. |last7=Pallé |first7=E. |last8=Godoy-Rivera |first8=D. |last9=Dai |first9=F. |last10=Ciardi |first10=D. R. |last11=Murphy |first11=J. M. Akana |last12=Beck |first12=P. G. |last13=Burke |first13=C. J. |last14=Cabrera |first14=J. |last15=Carleo |first15=I. |date=September 2023 |title=TOI-1416: A system with a super-Earth planet with a 1.07 d period |url=https://www.aanda.org/10.1051/0004-6361/202346370 |journal=Astronomy & Astrophysics |volume=677 |pages=A12 |doi=10.1051/0004-6361/202346370 |arxiv=2305.18542 |bibcode=2023A&A...677A..12D |s2cid=258967404 |issn=0004-6361}}

|0.0790 ±0.0120

|1.061 ±0.029

|6.9561063 ±0.0000017

|0.0710 ±0.0012

|957 ±17

| style="background:#FFFF00" |transit

|658.569{{±|0.918|0.911}}

|0.9870 ±0.0480

|5510 ±110

|{{Cite journal |last1=Yoshida |first1=Stephanie |last2=Vissapragada |first2=Shreyas |last3=Latham |first3=David W. |last4=Bieryla |first4=Allyson |last5=Thorngren |first5=Daniel P. |last6=Eastman |first6=Jason D. |last7=López-Morales |first7=Mercedes |last8=Barkaoui |first8=Khalid |last9=Beichman |first9=Charles |last10=Berlind |first10=Perry |last11=Buchave |first11=Lars A. |last12=Calkins |first12=Michael L. |last13=Ciardi |first13=David R. |last14=Collins |first14=Karen A. |last15=Cosentino |first15=Rosario |date=2023-11-01 |title=TESS Spots a Super-puff: The Remarkably Low Density of TOI-1420b |journal=The Astronomical Journal |volume=166 |issue=5 |pages=181 |doi=10.3847/1538-3881/acf858 |arxiv=2309.09945 |bibcode=2023AJ....166..181Y |issn=0004-6256 |doi-access=free }}

|0.0138{{±|0.0101|0.00535}}

|0.164{{±|0.0142|0.0139}}

|5.971143 ±0.000006

|0.0510 ±0.0009

|558.89 ±16.37

| style="background:#FFFF00" |transit

|122.113 ±0.196

|0.498{{±|0.026|0.025}}

|3810{{±|73|78}}

|

|0.0230{{±|0.0038|0.0039}}

|0.194 ±0.004

|2.527093{{±|0.000004|0.000003}}

|0.0285 ±0.0004

|734

| style="background:#FFFF00" |transit

|169.439 ±0.243

|0.471 ±0.011

|3709 ±11

|{{Cite journal |last1=González-Álvarez |first1=E. |last2=Zapatero Osorio |first2=M. R. |last3=Caballero |first3=J. A. |last4=Béjar |first4=V. J. S. |last5=Cifuentes |first5=C. |last6=Fukui |first6=A. |last7=Herrero |first7=E. |last8=Kawauchi |first8=K. |last9=Livingston |first9=J. H. |last10=López-González |first10=M. J. |last11=Morello |first11=G. |last12=Murgas |first12=F. |last13=Narita |first13=N. |last14=Pallé |first14=E. |last15=Passegger |first15=V. M. |date=July 2023 |title=Two sub-Neptunes around the M dwarf TOI-1470 |url=https://www.aanda.org/10.1051/0004-6361/202346292 |journal=Astronomy & Astrophysics |volume=675 |pages=A177 |doi=10.1051/0004-6361/202346292 |arxiv=2306.08516 |bibcode=2023A&A...675A.177G |s2cid=259165370 |issn=0004-6361}}

|0.02278{{±|0.00903|0.00872}}

|0.220 ±0.002

|18.08816{{±|0.00006|0.00008}}

|0.106 ±0.001

|373

| style="background:#FFFF00" |transit

|169.439 ±0.243

|0.471 ±0.011

|3709 ±11

|

|0.573 ±0.074

|

|502 ±16

|

|

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

|362.934{{±|1.210|1.200}}

|1.00 ±0.05

|5542.3 ±100.0

|{{Cite journal |last1=Van Zandt |first1=Judah |last2=Petigura |first2=Erik A. |last3=MacDougall |first3=Mason |last4=Gilbert |first4=Gregory J. |last5=Lubin |first5=Jack |last6=Barclay |first6=Thomas |last7=Batalha |first7=Natalie M. |last8=Crossfield |first8=Ian J. M. |last9=Dressing |first9=Courtney |last10=Fulton |first10=Benjamin |last11=Howard |first11=Andrew W. |last12=Huber |first12=Daniel |last13=Isaacson |first13=Howard |last14=Kane |first14=Stephen R. |last15=Robertson |first15=Paul |date=2023-02-01 |title=TESS-Keck Survey. XIV. Two Giant Exoplanets from the Distant Giants Survey |journal=The Astronomical Journal |volume=165 |issue=2 |pages=60 |doi=10.3847/1538-3881/aca6ef |arxiv=2209.06958 |bibcode=2023AJ....165...60V |issn=0004-6256 |doi-access=free }}

|0.0100 {{±|0.0035|0.0022}}

|0.131 {{±|0.00562|0.00437}}

|4.8026345{{±|0.0000040|0.0000039}}

|0.03144{{±|0.00025|0.00026}}

|404 ±14

| style="background:#FFFF00" |transit

|121.1

|1.1798 ±0.0044

|3225{{±|99|100}}

|super-Earth planet{{Cite journal |last1=Ghachoui |first1=M. |last2=Soubkiou |first2=A. |last3=Wells |first3=R. D. |last4=Rackham |first4=B. V. |last5=Triaud |first5=A. H. M. J. |last6=Sebastian |first6=D. |last7=Giacalone |first7=S. |last8=Stassun |first8=K. G. |last9=Ciardi |first9=D. R. |last10=Collins |first10=K. A. |last11=Liu |first11=A. |last12=Gómez Maqueo Chew |first12=Y. |last13=Gillon |first13=M. |last14=Benkhaldoun |first14=Z. |last15=Delrez |first15=L. |date=2023-09-01 |title=TESS discovery of a super-Earth orbiting the M-dwarf star TOI-1680 |url=https://ui.adsabs.harvard.edu/abs/2023A%26A...677A..31G |journal=Astronomy and Astrophysics |volume=677 |pages=A31 |doi=10.1051/0004-6361/202347040 |arxiv=2307.05368 |bibcode=2023A&A...677A..31G |s2cid=260278487 |issn=0004-6361 |access-date=1 January 2024 |archive-date=23 November 2023 |archive-url=https://web.archive.org/web/20231123161553/https://ui.adsabs.harvard.edu/abs/2023A%26A...677A..31G |url-status=live }}

|0.0809

|0.487{{±|0.042|0.071}}

|3.770179{{±|0.000058|0.000060}}

|

|1136.57

| style="background:#FFFF00" |transit

|405.7

|0.8450 ±0.1089

|5135 ±50

|

|1.05 ±0.05

|

|389.2 ±3.9

|

|

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

|405.7

|0.8450 ±0.1089

|5135 ±50

|{{Cite journal |last1=Van Zandt |first1=Judah |last2=Petigura |first2=Erik A. |last3=MacDougall |first3=Mason |last4=Gilbert |first4=Gregory J. |last5=Lubin |first5=Jack |last6=Barclay |first6=Thomas |last7=Batalha |first7=Natalie M. |last8=Crossfield |first8=Ian J. M. |last9=Dressing |first9=Courtney |last10=Fulton |first10=Benjamin |last11=Howard |first11=Andrew W. |last12=Huber |first12=Daniel |last13=Isaacson |first13=Howard |last14=Kane |first14=Stephen R. |last15=Robertson |first15=Paul |date=2023-02-01 |title=TESS-Keck Survey. XIV. Two Giant Exoplanets from the Distant Giants Survey |journal=The Astronomical Journal |volume=165 |issue=2 |pages=60 |doi=10.3847/1538-3881/aca6ef |arxiv=2209.06958 |bibcode=2023AJ....165...60V |issn=0004-6256 |doi-access=free }}

|0.040 ±0.016

|0.223 ±0.016

|7.073088 ±0.000007

|0.0740 ±0.0009

|1076 ±39

| style="background:#FFFF00" |transit

|290.111{{±|1.050|1.043}}

|1.08 ±0.04

|5807 ±46

|{{Cite journal |last1=Martioli |first1=E. |last2=Hébrard |first2=G. |last3=de Almeida |first3=L. |last4=Heidari |first4=N. |last5=Lorenzo-Oliveira |first5=D. |last6=Kiefer |first6=F. |last7=Almenara |first7=J. M. |last8=Bieryla |first8=A. |last9=Boisse |first9=I. |last10=Bonfils |first10=X. |last11=Briceño |first11=C. |last12=Collins |first12=K. A. |last13=Cortés-Zuleta |first13=P. |last14=Dalal |first14=S. |last15=Deleuil |first15=M. |date=2023 |title=TOI-1736 and TOI-2141: Two systems including sub-Neptunes around solar analogs revealed by TESS and SOPHIE |journal=Astronomy & Astrophysics |volume=680 |pages=A84 |doi=10.1051/0004-6361/202347744 |arxiv=2311.07011|bibcode=2023A&A...680A..84M |s2cid=264471812 }}

|8.70{{±|1.50|0.60}}

|

|570.1 ±0.7

|1.381 ±0.017

|249 ±9

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

|290.111{{±|1.050|1.043}}

|1.08 ±0.04

|5807 ±46

|

|0.0126{{±|0.00849|0.00472}}

|0.151{{±|0.00874|0.00758}}

|8.303342{{±|0.000011|0.000013}}

|0.0742 ±0.0014

|755.55 ±20.19

| style="background:#FFFF00" |transit

|231.506 ±0.522

|0.790{{±|0.046|0.045}}

|4922{{±|94|91}}

|

|0.0158

|0.187{{±|0.005|0.006}}

|10.643976{{±|0.000014|0.000014}}

|

|490.47

| style="background:#FFFF00" |transit

|100.8

|0.5413 ±0.0204

|3815 ±157

|

|0.9720{{±|0.0760|0.0780}}

|0.9940{{±|0.0250|0.0230}}

|3.7130765 ±0.0000017

|0.04389{{±|0.00058|0.00055}}

|962.2{{±|8.0|7.9}}

| style="background:#FFFF00" |transit

|418.231{{±|2.319|2.296}}

|0.817{{±|0.033|0.030}}

|4766{{±|52|54}}

|

|0.0406

|0.325{{±|0.020|0.016}}

|1.243702{{±|0.000121|0.000114}}

|

|1510.96

| style="background:#FFFF00" |transit

|539 ±3

|0.8200 ±0.0992

|5175 ±50

|

|

|0.87 ±0.07

|63.48347 ±0.00010

|0.337{{±|0.044|0.036}}

|

| style="background:#FFFF00" |transit

|731.847{{±|3.826|3.787}}

|1.287 ±0.061

|6341{{±|68|70}}

|{{Cite journal |last1=Dong |first1=Jiayin |last2=Wang |first2=Songhu |last3=Rice |first3=Malena |last4=Zhou |first4=George |last5=Huang |first5=Chelsea X. |last6=Dawson |first6=Rebekah I. |last7=Stefánsson |first7=Gudmundur K. |last8=Halverson |first8=Samuel |last9=Kanodia |first9=Shubham |last10=Mahadevan |first10=Suvrath |last11=McElwain |first11=Michael W. |last12=Alvarado-Montes |first12=Jaime A. |last13=Ninan |first13=Joe P. |last14=Robertson |first14=Paul |last15=Roy |first15=Arpita |date=2023-07-01 |title=TOI-1859b: A 64 Day Warm Jupiter on an Eccentric and Misaligned Orbit |journal=The Astrophysical Journal Letters |volume=951 |issue=2 |pages=L29 |doi=10.3847/2041-8213/acd93d |arxiv=2305.16495 |bibcode=2023ApJ...951L..29D |issn=2041-8205 |doi-access=free }}

|2.01{{±|0.17|0.16}}

|1.247{{±|0.059|0.062}}

|0.946679944 ±0.00000047

|0.01932{{±|0.00035|0.00039}}

|2097{{±|35|36}}

| style="background:#FFFF00" |transit

|1353.99{{±|9.55|9.42}}

|1.072{{±|0.059|0.064}}

|5814{{±|91|93}}

|{{Cite journal |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 |date=2023-03-01 |title=The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets* |journal=The Astrophysical Journal Supplement Series |volume=265 |issue=1 |pages=1 |doi=10.3847/1538-4365/aca286 |arxiv=2210.15473 |bibcode=2023ApJS..265....1Y |issn=0067-0049 |doi-access=free }}

|0.0347{{±|0.0077|0.0075}}

|0.241 ±0.014

|3.098330{{±|0.000021|0.000019}}

|0.04271{{±|0.00076|0.00067}}

|1488{{±|122|160}}

| style="background:#FFFF00" |transit

|30.3424 ±0.0685

|1.082{{±|0.059|0.050}}

|5611{{±|85|82}}

|{{Cite journal |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 |date=2023-07-04 |title=TESS spots a mini-neptune interior to a hot saturn in the TOI-2000 system |url=https://academic.oup.com/mnras/article/524/1/1113/7191273 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=524 |issue=1 |pages=1113–1138 |doi=10.1093/mnras/stad1666 |doi-access=free |issn=0035-8711|arxiv=2209.14396 }}

|0.0257{{±|0.015|0.014}}

|0.727{{±|0.028|0.027}}

|9.1270550{{±|0.0000073|0.0000072}}

|0.0878{{±|0.0016|0.0014}}

|1038{{±|84|111}}

| style="background:#FFFF00" |transit

|30.3424 ±0.0685

|1.082{{±|0.059|0.050}}

|5611{{±|85|82}}

|

|1.286{{±|0.055|0.057}}

|1.054 ±0.027

|141.834025{{±|0.000065|0.000066}}

|0.5516{{±|0.0078|0.0093}}

|400.2{{±|5.6|5.7}}

| style="background:#FFFF00" |transit

|356.131{{±|1.050|1.044}}

|1.112{{±|0.048|0.055}}

|5929 ±74

|{{Cite journal |last1=Mann |first1=Christopher R. |last2=Dalba |first2=Paul A. |last3=Lafrenière |first3=David |last4=Fulton |first4=Benjamin J. |last5=Hébrard |first5=Guillaume |last6=Boisse |first6=Isabelle |last7=Dalal |first7=Shweta |last8=Deleuil |first8=Magali |last9=Delfosse |first9=Xavier |last10=Demangeon |first10=Olivier |last11=Forveille |first11=Thierry |last12=Heidari |first12=Neda |last13=Kiefer |first13=Flavien |last14=Martioli |first14=Eder |last15=Moutou |first15=Claire |date=2023-12-01 |title=Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. III. Recovery and Confirmation of a Temperate, Mildly Eccentric, Single-transit Jupiter Orbiting TOI-2010 |journal=The Astronomical Journal |volume=166 |issue=6 |pages=239 |doi=10.3847/1538-3881/ad00bc |arxiv=2311.10232 |bibcode=2023AJ....166..239M |issn=0004-6256 |doi-access=free }}

|0.0516{{±|0.0129}}

|0.302{{±|0.012}}

|3.348968{{±|0.000004}}

|0.0301{{±|0.0013|0.0012}}

|512{{±|11}}

| style="background:#FFFF00" |transit

|154.34{{±|0.13|0.10}}

|0.342{{±|0.021|0.025}}

|3194{{±|56}}

|{{cite arXiv|last1=Jones|first1=Sinclaire E.|last2=Stefánsson|first2=Guðmundur|last3=Masuda|first3=Kento|last4=Libby-Roberts|first4=Jessica E.|last5=Gardner|first5=Cristilyn N.|last6=Holcomb|first6=Rae|last7=Beard|first7=Corey|last8=Robertson|first8=Paul|last9=Cañas|first9=Caleb I.|last10=Mahadevan|first10=Suvrath|last11=Kanodia|first11=Shubham|last12=Lin|first12=Andrea S. J.|last13=Kobulnicky|first13=Henry A.|last14=Parker|first14=Brock A.|last15=Bender|first15=Chad F.|last16=Cochran|first16=William D.|last17=Diddams|first17=Scott A.|last18=Fernandes|first18=Rachel B.|last19=Gupta|first19=Arvind F.|last20=Halverson|first20=Samuel|last21=Hawley|first21=Suzanne L.|last22=Hearty|first22=Fred R.|last23=Hebb|first23=Leslie|last24=Kowalski|first24=Adam|last25=Lubin|first25=Jack|last26=Monson|first26=Andrew|last27=Ninan|first27=Joe P.|last28=Ramsey|first28=Lawrence|last29=Roy|first29=Arpita|last30=Schwab|first30=Christian|last31=Terrien|first31=Ryan C.|last32=Wisniewski|first32=John|date=9 May 2024|title=TOI-2015b: A Warm Neptune with Transit Timing Variations Orbiting an Active mid M Dwarf |class=astro-ph.EP |eprint=2310.11775}}

|0.0185

|0.204{{±|0.009|0.007}}

|7.435588 ±0.000009

|

|652.44

| style="background:#FFFF00" |transit

|

|0.6600 ±0.0868

|4348 ±100

|

|0.0138{{±|0.0101|0.00503}}

|0.162{{±|0.0145|0.0133}}

|7.768915{{±|0.000025|0.000037}}

|0.0632 ±0.0011

|520.62 ±14.18

| style="background:#FFFF00" |transit

|172.635{{±|0.294|0.261}}

|0.559{{±|0.027|0.029}}

|3710{{±|57|58}}

|

|

|0.220 ±0.012

|6.0784247 ±0.0000096

|0.05006 ±0.00103

|527 ±8

| style="background:#FFFF00" |transit

|373.609{{±|1.115|1.106}}

|0.453{{±|0.029|0.027}}

|3551{{±|49|52}}

|{{Cite journal |last1=Barkaoui |first1=K. |last2=Timmermans |first2=M. |last3=Soubkiou |first3=A. |last4=Rackham |first4=B. V. |last5=Burgasser |first5=A. J. |last6=Chouqar |first6=J. |last7=Pozuelos |first7=F. J. |last8=Collins |first8=K. A. |last9=Howell |first9=S. B. |last10=Simcoe |first10=R. |last11=Melis |first11=C. |last12=Stassun |first12=K. G. |last13=Tregloan-Reed |first13=J. |last14=Cointepas |first14=M. |last15=Gillon |first15=M. |date=September 2023 |title=TOI-2084 b and TOI-4184 b: Two new sub-Neptunes around M dwarf stars |url=https://www.aanda.org/10.1051/0004-6361/202346838 |journal=Astronomy & Astrophysics |volume=677 |pages=A38 |doi=10.1051/0004-6361/202346838 |arxiv=2306.15095 |bibcode=2023A&A...677A..38B |s2cid=259262549 |issn=0004-6361}}

|

|0.116 ±0.009

|17.664872{{±|0.000045|0.000051}}

|0.1010{{±|0.0088|0.0084}}

|347 ±9

| style="background:#FFFF00" |transit

|136.73 ±0.08

|0.465 ±0.012

|3662 ±130

|{{cite journal|arxiv=2304.09189|year=2023|title=Two Warm Super-Earths Transiting the Nearby M Dwarf, TOI-2095 |last1=Quintana |first1=Elisa V. |last2=Gilbert |first2=Emily A. |last3=Barclay |first3=Thomas |last4=Silverstein |first4=Michele L. |last5=Schlieder |first5=Joshua E. |last6=Cloutier |first6=Ryan |last7=Quinn |first7=Samuel N. |last8=Rodriguez |first8=Joseph E. |last9=Vanderburg |first9=Andrew |last10=Hord |first10=Benjamin J. |last11=Louie |first11=Dana R. |last12=Ostberg |first12=Colby |last13=Kane |first13=Stephen R. |last14=Hoffman |first14=Kelsey |last15=Rowe |first15=Jason F. |last16=Arney |first16=Giada N. |last17=Saxena |first17=Prabal |last18=Richardson |first18=Taran |last19=Clement |first19=Matthew S. |last20=Kartvedt |first20=Nicholas M. |last21=Adams |first21=Fred C. |last22=Alfred |first22=Marcus |last23=Berger |first23=Travis |last24=Bieryla |first24=Allyson |last25=Bonney |first25=Paul |last26=Boyd |first26=Patricia |last27=Cadieux |first27=Charles |last28=Caldwell |first28=Douglas |last29=Ciardi |first29=David R. |last30=Charbonneau |first30=David |journal=The Astronomical Journal |volume=166 |issue=5 |page=195 |doi=10.3847/1538-3881/acfa9f |bibcode=2023AJ....166..195Q |display-authors=1 |doi-access=free }}{{cite journal|arxiv=2304.09220|year=2023|title=Two super-Earths at the edge of the habitable zone of the nearby M dwarf TOI-2095 |last1=Murgas |first1=F. |last2=Castro-González |first2=A. |last3=Pallé |first3=E. |last4=Pozuelos |first4=F. J. |last5=Millholland |first5=S. |last6=Foo |first6=O. |last7=Korth |first7=J. |last8=Marfil |first8=E. |last9=Amado |first9=P. J. |last10=Caballero |first10=J. A. |last11=Christiansen |first11=J. L. |last12=Ciardi |first12=D. R. |last13=Collins |first13=K. A. |last14=Di Sora |first14=M. |last15=Fukui |first15=A. |last16=Gan |first16=T. |last17=Gonzales |first17=E. J. |last18=Henning |first18=Th. |last19=Herrero |first19=E. |last20=Isopi |first20=G. |last21=Jenkins |first21=J. M. |last22=Lillo-Box |first22=J. |last23=Lodieu |first23=N. |last24=Luque |first24=R. |last25=Mallia |first25=F. |last26=Morello |first26=G. |last27=Narita |first27=N. |last28=Orell-Miquel |first28=J. |last29=Parviainen |first29=H. |last30=Pérez-Torres |first30=M. |journal=Astronomy & Astrophysics |volume=677 |pages=A182 |doi=10.1051/0004-6361/202346692 |bibcode=2023A&A...677A.182M |s2cid=258212464 |display-authors=1 }}

|

|0.124{{±|0.010|0.009}}

|28.17221{{±|0.00011|0.00014}}

|0.138{{±|0.012|0.011}}

|297 ±8

| style="background:#FFFF00" |transit

|136.73 ±0.08

|0.465 ±0.012

|3662 ±130

|

|0.0060{{±|0.0044|0.0019}}

|0.110 ±0.006

|3.1190633{{±|0.000010|0.0000093}}

|0.025 ±0.001

|445 ±13

| style="background:#FFFF00" |transit

|158.08 ±0.13

|0.231 ±0.012

|3300 ±50

|{{cite journal|arxiv=2303.08174|year=2023|title=A super-Earth and a mini-Neptune near the 2:1 MMR straddling the radius valley around the nearby mid-M dwarf TOI-2096|last1=Pozuelos |first1=F. J. |last2=Timmermans |first2=M. |last3=Rackham |first3=B. V. |last4=Garcia |first4=L. J. |last5=Burgasser |first5=A. J. |last6=Kane |first6=S. R. |last7=Günther |first7=M. N. |last8=Stassun |first8=K. G. |last9=Van Grootel |first9=V. |last10=Dévora-Pajares |first10=M. |last11=Luque |first11=R. |last12=Edwards |first12=B. |last13=Niraula |first13=P. |last14=Schanche |first14=N. |last15=Wells |first15=R. D. |last16=Ducrot |first16=E. |last17=Howell |first17=S. |last18=Sebastian |first18=D. |last19=Barkaoui |first19=K. |last20=Waalkes |first20=W. |last21=Cadieux |first21=C. |last22=Doyon |first22=R. |last23=Boyle |first23=R. P. |last24=Dietrich |first24=J. |last25=Burdanov |first25=A. |last26=Delrez |first26=L. |last27=Demory |first27=B. -O. |last28=de Wit |first28=J. |last29=Dransfield |first29=G. |last30=Gillon |first30=M. |journal=Astronomy & Astrophysics |volume=672 |pages=A70 |doi=10.1051/0004-6361/202245440 |bibcode=2023A&A...672A..70P |s2cid=256927017 |display-authors=1 }}

|0.0145{{±|0.0110|0.0057}}

|0.171 ±0.008

|6.387840 ±0.000012

|0.040 ±0.002

|349{{±|10|9}}

| style="background:#FFFF00" |transit

|158.08 ±0.13

|0.231 ±0.012

|3300 ±50

|

|0.0287{{±|0.0025|0.0024}}

|0.240 ±0.014

|9.2292005 ±0.0000063

|0.0780 ±0.0009

|666 ±8

| style="background:#FFFF00" |transit

|73.7773{{±|0.0522|0.0519}}

|0.744 ±0.027

|4580 ±50

|{{Cite journal |last1=Rescigno |first1=F |last2=Hébrard |first2=G |last3=Vanderburg |first3=A |last4=Mann |first4=A W |last5=Mortier |first5=A |last6=Morrell |first6=S |last7=Buchhave |first7=L A |last8=Collins |first8=K A |last9=Mann |first9=C R |last10=Hellier |first10=C |last11=Haywood |first11=R D |last12=West |first12=R |last13=Stalport |first13=M |last14=Heidari |first14=N |last15=Anderson |first15=D |date=2023-11-27 |title=A hot mini-Neptune and a temperate, highly eccentric sub-Saturn around the bright K-dwarf TOI-2134 |url=https://academic.oup.com/mnras/article/527/3/5385/7330172 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=527 |issue=3 |pages=5385–5407 |doi=10.1093/mnras/stad3255 |issn=0035-8711 |doi-access=free |access-date=8 December 2023 |archive-date=8 December 2023 |archive-url=https://web.archive.org/web/20231208231710/https://academic.oup.com/mnras/article/527/3/5385/7330172 |url-status=live |hdl=10023/28862 |hdl-access=free }}

|0.1318{{±|0.0242|0.0246}}

|0.649 ±0.037

|95.50{{±|0.36|0.25}}

|0.371 ±0.004

|306 ±4

| style="background:#FFFF00" |transit

|73.7773{{±|0.0522|0.0519}}

|0.744 ±0.027

|4580 ±50

|

|0.075 ±0.012

|0.278 ±0.021

|18.26157 ±0.00006

|0.1330 ±0.0009

|722 ±23

| style="background:#FFFF00" |transit

|253.365{{±|0.736|0.732}}

|0.94 ±0.02

|5659 ±48

|

|2.83{{±|0.38|0.37}}

|1.281{{±|0.050|0.046}}

|3.3773512{{±|0.0000060|0.0000061}}

|0.05064{{±|0.00093|0.00110}}

|1802{{±|60|54}}

| style="background:#FFFF00" |transit

|988.275{{±|10.143|9.945}}

|1.516{{±|0.085|0.100}}

|6630{{±|300|200}}

|{{Cite journal |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=Gonzales |first14=Erica J |last15=Scott Gaudi |first15=B |date=2023-03-14 |title=Another shipment of six short-period giant planets from TESS |url=https://academic.oup.com/mnras/article/521/2/2765/7060400 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=521 |issue=2 |pages=2765–2785 |doi=10.1093/mnras/stad595 |issn=0035-8711 |doi-access=free |access-date=8 December 2023 |archive-date=8 December 2023 |archive-url=https://web.archive.org/web/20231208012242/https://academic.oup.com/mnras/article/521/2/2765/7060400 |url-status=live |arxiv=2205.05709 }}

|0.920{{±|0.190|0.180}}

|1.453{{±|0.053|0.048}}

|3.8240801 ±0.0000025

|0.0513{{±|0.0011|0.0013}}

|1580 ±27

| style="background:#FFFF00" |transit

|966.924{{±|2.174|2.143}}

|1.233{{±|0.077|0.090}}

|6280 ±160

|

|0.0145

|0.178{{±|0.012|0.006}}

|15.337597{{±|0.001585|0.001616}}

|

|590.88

| style="background:#FFFF00" |transit

|63.84 ±0.12

|0.7400 ±0.0854

|4756 ±50

|

|5.98{{±|0.21|0.20}}

|1.00 ±0.02

|22.65398 ±0.00002

|0.158 ±0.03

|799{{±|10|11}}

| style="background:#FFFF00" |transit

|1032 ±7

|0.99{{±|0.03|0.02}}

|5581 ±60

|

|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

|716.286{{±|5.594|5.509}}

|0.954{{±|0.041|0.046}}

|5306{{±|76|68}}

|

|0.0256

|0.248 ±0.004

|15.669494{{±|0.000926|0.001004}}

|

|600.83

| style="background:#FFFF00" |transit

|

|0.6600 ±0.0789

|4357 ±100

|

|0.0285

|0.264{{±|0.008|0.006}}

|19.104718{{±|0.000023|0.000024}}

|

|445.01

| style="background:#FFFF00" |transit

|

|0.6600 ±0.0763

|4195 ±124

|

|4.82 ±0.41

|0.9940{{±|0.0550|0.0490}}

|10.655669 ±0.000038

|0.1166 ±0.0018

|1595{{±|45|42}}

| style="background:#FFFF00" |transit

|930.489{{±|11.624|11.347}}

|1.859{{±|0.087|0.083}}

|7360{{±|320|300}}

|

|0.1089{{±|0.0129|0.0129}}

|0.541{{±|0.026|0.024}}

|3.738252 ±0.000004

|0.0491 ±0.0030

|1443{{±|15|28}}

| style="background:#FFFF00" |transit

|897.796{{±|13.712|13.314}}

|1.12 ±0.02

|5905 ±12

|{{Cite journal |last1=Frame |first1=Ginger |last2=Armstrong |first2=David J |last3=Cegla |first3=Heather M |last4=Fernández Fernández |first4=Jorge |last5=Osborn |first5=Ares |last6=Adibekyan |first6=Vardan |last7=Collins |first7=Karen A |last8=Delgado Mena |first8=Elisa |last9=Giacalone |first9=Steven |last10=Kielkopf |first10=John F |last11=Santos |first11=Nuno C |last12=Sousa |first12=Sérgio G |last13=Stassun |first13=Keivan G |last14=Ziegler |first14=Carl |last15=Anderson |first15=David R |date=2023-05-23 |title=TOI-2498 b: a hot bloated super-Neptune within the Neptune desert |url=https://academic.oup.com/mnras/article/523/1/1163/7165762 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=523 |issue=1 |pages=1163–1174 |doi=10.1093/mnras/stad1452 |issn=0035-8711 |doi-access=free |access-date=9 December 2023 |archive-date=9 December 2023 |archive-url=https://web.archive.org/web/20231209115857/https://academic.oup.com/mnras/article/523/1/1163/7165762 |url-status=live |arxiv=2305.06950 }}

|0.088{{±|0.005|0.004}}

|0.774 ±0.010

|23.288{{±|0.001|0.002}}

|0.1511 ±0.0025

|500

| style="background:#FFFF00" |transit

|1305 ±8

|0.849{{±|0.024|0.033}}

|5096 ±80

|{{cite journal|arxiv=2302.05694|year=2023|title=TOI-2525 b and c: A Pair of Massive Warm Giant Planets with Strong Transit Timing Variations Revealed by TESS|last1=Trifonov |first1=Trifon |last2=Brahm |first2=Rafael |last3=Jordan |first3=Andres |last4=Hartogh |first4=Christian |last5=Henning |first5=Thomas |last6=Hobson |first6=Melissa J. |last7=Schlecker |first7=Martin |last8=Howard |first8=Saburo |last9=Reichardt |first9=Finja |last10=Espinoza |first10=Nestor |author11=Man Hoi Lee |last12=Nesvorny |first12=David |last13=Rojas |first13=Felipe I. |last14=Barkaoui |first14=Khalid |last15=Kossakowski |first15=Diana |last16=Boyle |first16=Gavin |last17=Dreizler |first17=Stefan |last18=Kuerster |first18=Martin |last19=Heller |first19=Rene |last20=Guillot |first20=Tristan |last21=Triaud |first21=Amaury H. M. J. |last22=Abe |first22=Lyu |last23=Agabi |first23=Abdelkrim |last24=Bendjoya |first24=Philippe |last25=Crouzet |first25=Nicolas |last26=Dransfield |first26=Georgina |last27=Gasparetto |first27=Thomas |last28=Guenther |first28=Maximilian N. |last29=Marie-Sainte |first29=Wenceslas |last30=Mekarnia |first30=Djamel |journal=The Astronomical Journal |volume=165 |issue=4 |page=179 |doi=10.3847/1538-3881/acba9b |bibcode=2023AJ....165..179T |s2cid=256827169 |display-authors=1 |doi-access=free }}

|0.709 ±0.034

|0.904 ±0.010

|49.260 ±0.001

|0.2491{{±|0.0041|0.0042}}

|390

| style="background:#FFFF00" |transit

|1305 ±8

|0.849{{±|0.024|0.033}}

|5096 ±80

|

|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

|1846.66{{±|21.10|20.64}}

|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

|1218.77{{±|5.953|5.772}}

|1.15{{±|0.14|0.07}}

|5760{{±|80|79}}

|

|3.5 ±0.1

|1.08 ±0.03

|61.6277 ±0.0002

|0.300{{±|0.006|0.005}}

|592{{±|7|8}}

| style="background:#FFFF00" |transit

|658 ±3

|0.93{{±|0.03|0.02}}

|5579 ±70

|

|0.367{{±|0.049|0.040}}

|1.615{{±|0.462|0.640}}

|4.880974{{±|0.000023|0.000037}}

|0.0607{{±|0.0042|0.0043}}

|1387{{±|22|23}}

| style="background:#FFFF00" |transit

|1131 ±7

|1.16 ±0.07

|6100 ±100

|Extremely grazing transit

|0.44{{±|0.10|0.11}}

|>1.54

|4.8084983{{±|0.0000057|0.0000056}}

|0.0569{{±|0.0010|0.0011}}

|1205{{±|18|17}}

| style="background:#FFFF00" |transit

|1142.67{{±|19.63|18.99}}

|1.063{{±|0.057|0.062}}

|5764{{±|81|78}}

|

|0.9750{{±|0.0830|0.0700}}

|1.616{{±|0.034|0.032}}

|1.96229325 ±0.00000082

|0.03185 ±0.00052

|1893{{±|29|28}}

| style="background:#FFFF00" |transit

|1613.88{{±|21.68|21.13}}

|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

|1019.81{{±|7.39|7.28}}

|0.9770{{±|0.0630|0.0490}}

|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

|1503.57{{±|25.18|24.37}}

|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

|

|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

|1271.74{{±|10.42|10.26}}

|1.12{{±|0.11|0.06}}

|5760{{±|85|88}}

|

|0.0411

|0.327 ±0.013

|1.926907{{±|0.000128|0.000134}}

|

|1032.78

| style="background:#FFFF00" |transit

|368.8 ±1.5

|0.6640 ±0.0798

|4263 ±100

|

|0.665 ±0.025

|1.017 ±0.044

|2.59261842 ±0.00000041

|0.02709 ±0.00046

|604 ±19

| style="background:#FFFF00" |transit

|236.7 ±0.5

|0.394 ±0.003

|3389 ±6

|{{cite journal|arxiv=2302.10008|year=2023|title=TOI-3235 b: A Transiting Giant Planet around an M4 Dwarf Star|last1=Hobson |first1=Melissa J. |last2=Jordán |first2=Andrés |last3=Bryant |first3=E. M. |last4=Brahm |first4=R. |last5=Bayliss |first5=D. |last6=Hartman |first6=J. D. |last7=Bakos |first7=G. Á. |last8=Henning |first8=Th. |author9=Jose Manuel Almenara |last10=Barkaoui |first10=Khalid |last11=Benkhaldoun |first11=Zouhair |last12=Bonfils |first12=Xavier |last13=Bouchy |first13=François |last14=Charbonneau |first14=David |last15=Cointepas |first15=Marion |last16=Collins |first16=Karen A. |last17=Eastman |first17=Jason D. |last18=Ghachoui |first18=Mourad |last19=Gillon |first19=Michaël |last20=Goeke |first20=Robert F. |last21=Horne |first21=Keith |last22=Irwin |first22=Jonathan M. |last23=Jehin |first23=Emmanuel |last24=Jenkins |first24=Jon M. |last25=Latham |first25=David W. |last26=Moldovan |first26=Dan |last27=Murgas |first27=Felipe |last28=Pozuelos |first28=Francisco J. |last29=Ricker |first29=George R. |last30=Schwarz |first30=Richard P. |journal=The Astrophysical Journal Letters |volume=946 |issue=1 |pages=L4 |doi=10.3847/2041-8213/acbd9a |bibcode=2023ApJ...946L...4H |s2cid=257038386 |display-authors=1 |doi-access=free }}

|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

|906.386{{±|8.170|8.027}}

|1.186{{±|0.059|0.083}}

|5706{{±|95|91}}

|

|0.980{{±|0.100|0.110}}

|1.167{{±|0.048|0.044}}

|3.246075 ±0.000012

|0.04560{{±|0.00089|0.00098}}

|1534{{±|29|28}}

| style="background:#FFFF00" |transit

|1292.81{{±|19.67|19.10}}

|1.199{{±|0.072|0.076}}

|5950 ±100

|

|0.0470 ±0.0126

|0.459 ±0.014

|4.6747373 ±0.0000038

|0.043 ±0.001

|582 ±16

| style="background:#FFFF00" |transit

|259.0 ±0.3

|0.52 ±0.02

|3576 ±88

|{{cite journal|arxiv=2304.04730|year=2023|title=TOI-3785 b: A Low-density Neptune Orbiting an M2-dwarf Star |last1=Powers |first1=Luke C. |last2=Libby-Roberts |first2=Jessica |last3=Lin |first3=Andrea S. J. |last4=Cañas |first4=Caleb I. |last5=Kanodia |first5=Shubham |last6=Mahadevan |first6=Suvrath |last7=Ninan |first7=Joe P. |last8=Stefánsson |first8=Guðmundur |last9=Gupta |first9=Arvind F. |last10=Jones |first10=Sinclaire |last11=Kobulnicky |first11=Henry A. |last12=Monson |first12=Andrew |last13=Parker |first13=Brock A. |last14=Swaby |first14=Tera N. |last15=Bender |first15=Chad F. |last16=Cochran |first16=William D. |last17=Hebb |first17=Leslie |last18=Metcalf |first18=Andrew J. |last19=Robertson |first19=Paul |last20=Schwab |first20=Christian |last21=Wisniewski |first21=John |last22=Wright |first22=Jason T. |journal=The Astronomical Journal |volume=166 |issue=2 |page=44 |doi=10.3847/1538-3881/acd8bf |bibcode=2023AJ....166...44P |s2cid=258048476 |doi-access=free }}

|1.04{{±|0.15|0.14}}

|>1.65

|2.8989727{{±|0.0000038|0.0000039}}

|0.0421{{±|0.0007|0.0011}}

|1646{{±|25|24}}

| style="background:#FFFF00" |transit

|1375.55{{±|15.20|14.88}}

|1.181{{±|0.0064|0.0092}}

|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

|1820.41{{±|42.55|40.68}}

|1.242{{±|0.057|0.076}}

|5859{{±|72|71}}

|

|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

|1519.86{{±|21.48|20.90}}

|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

|1683.25{{±|19.30|18.88}}

|1.254{{±|0.067|0.072}}

|5975{{±|70|69}}

|

|0.14 ±0.03

|0.71 ±0.02

|4.35326 ±0.000005

|0.041{{±|0.002|0.001}}

|563 ±15

| style="background:#FFFF00" |transit

|353.6{{±|1.0|0.7}}

|0.49 ±0.02

|3476 ±88

|{{cite journal|arxiv=2302.07714|year=2023|title=TOI-3984 a b and TOI-5293 a b: Two Temperate Gas Giants Transiting Mid-M Dwarfs in Wide Binary Systems|last1=Cañas |first1=Caleb I. |last2=Kanodia |first2=Shubham |last3=Libby-Roberts |first3=Jessica |last4=Lin |first4=Andrea S. J. |last5=Schutte |first5=Maria |last6=Powers |first6=Luke |last7=Jones |first7=Sinclaire |last8=Monson |first8=Andrew |last9=Wang |first9=Songhu |last10=Stefánsson |first10=Guðmundur |last11=Cochran |first11=William D. |last12=Robertson |first12=Paul |last13=Mahadevan |first13=Suvrath |last14=Kowalski |first14=Adam F. |last15=Wisniewski |first15=John |last16=Parker |first16=Brock A. |last17=Larsen |first17=Alexander |last18=Chapman |first18=Franklin A. L. |last19=Kobulnicky |first19=Henry A. |last20=Gupta |first20=Arvind F. |last21=Everett |first21=Mark E. |author22=Bryan Edward Penprase |last23=Zeimann |first23=Gregory |last24=Beard |first24=Corey |last25=Bender |first25=Chad F. |last26=Colón |first26=Knicole D. |last27=Diddams |first27=Scott A. |last28=Fredrick |first28=Connor |last29=Halverson |first29=Samuel |last30=Ninan |first30=Joe P. |journal=The Astronomical Journal |volume=166 |issue=1 |page=30 |doi=10.3847/1538-3881/acdac7 |bibcode=2023AJ....166...30C |s2cid=256868404 |display-authors=1 |doi-access=free }}

|0.03461{{±|0.00406|0.00400}}

|0.269 ±0.007

|1.348335{{±|0.000003|0.000002}}

|0.0229 ±0.0002

|1441{{±|14|13}}

| style="background:#FFFF00" |transit

|578.941{{±|3.242|3.203}}

|0.88 ±0.03

|4960 ±36

|{{Cite journal |last1=Kunimoto |first1=Michelle |last2=Vanderburg |first2=Andrew |last3=Huang |first3=Chelsea X. |last4=Davis |first4=M. Ryleigh |last5=Affer |first5=Laura |last6=Cameron |first6=Andrew Collier |last7=Charbonneau |first7=David |last8=Cosentino |first8=Rosario |last9=Damasso |first9=Mario |last10=Dumusque |first10=Xavier |last11=Fiorenzano |first11=A. F. Martnez |last12=Ghedina |first12=Adriano |last13=Haywood |first13=R. D. |last14=Lienhard |first14=Florian |last15=López-Morales |first15=Mercedes |date=2023-07-01 |title=TOI-4010: A System of Three Large Short-period Planets with a Massive Long-period Companion |journal=The Astronomical Journal |volume=166 |issue=1 |pages=7 |doi=10.3847/1538-3881/acd537 |arxiv=2306.05308 |bibcode=2023AJ....166....7K |issn=0004-6256 |doi-access=free }}

|0.06390{{±|0.00670|0.00664}}

|0.529{{±|0.010|0.011}}

|5.414654 ±0.000007

|0.058 ±0.001

|907{{±|9|8}}

| style="background:#FFFF00" |transit

|578.941{{±|3.242|3.203}}

|0.88 ±0.03

|4960 ±36

|

|0.1200{{±|0.0103|0.0101}}

|0.551{{±|0.012|0.013}}

|14.70886 ±0.00003

|0.113 ±0.001

|650 ±6

| style="background:#FFFF00" |transit

|578.941{{±|3.242|3.203}}

|0.88 ±0.03

|4960 ±36

|

|2.18{{±|0.21|0.20}}

|

|>762 ±90

|1.57{{±|0.12|0.13}}

|174{{±|8|6}}

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

|578.941{{±|3.242|3.203}}

|0.88 ±0.03

|4960 ±36

|

|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

|983.937{{±|7.257|7.153}}

|1.178{{±|0.039|0.042}}

|6060{{±|74|67}}

|

|2.30 ±0.11

|1.096{{±|0.039|0.032}}

|56.39879 ±0.00010

|0.3081{{±|0.0055|0.0058}}

|605.1{{±|9.6|8.2}}

| style="background:#FFFF00" |transit

|1060 ±20

|1.23 ±0.07

|6096 ±115

|Highly eccentric orbit{{cite journal|arxiv=2303.14570|year=2023|title=A High-Eccentricity Warm Jupiter Orbiting TOI-4127|last1=Gupta |first1=Arvind F. |last2=Jackson |first2=Jonathan M. |last3=Hebrard |first3=Guillaume |last4=Lin |first4=Andrea S. |last5=Stassun |first5=Keivan G. |last6=Dong |first6=Jiayin |last7=Villanueva |first7=Steven |last8=Dragomir |first8=Diana |last9=Mahadevan |first9=Suvrath |last10=Wright |first10=Jason T. |author11=Jose Manuel Almenara |last12=Blake |first12=Cullen H. |last13=Boisse |first13=Isabelle |last14=Cortes-Zuleta |first14=Pia |last15=Dalba |first15=Paul A. |last16=Diaz |first16=Rodrigo F. |last17=Ford |first17=Eric B. |last18=Forveille |first18=Thierry |last19=Gagliano |first19=Robert |last20=Halverson |first20=Samuel P. |last21=Heidari |first21=Neda |last22=Kanodia |first22=Shubham |last23=Kiefer |first23=Flavien |last24=Latham |first24=David W. |last25=McElwain |first25=Michael W. |last26=Mireles |first26=Ismael |last27=Pepper |first27=Joshua |last28=Ricker |first28=George R. |last29=Robertson |first29=Paul |last30=Roy |first30=Arpita |journal=The Astronomical Journal |volume=165 |issue=6 |page=234 |doi=10.3847/1538-3881/accb9b |bibcode=2023AJ....165..234G |s2cid=257766926 |display-authors=1 |doi-access=free }}

|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

|669.884{{±|3.904|3.862}}

|0.905{{±|0.043|0.044}}

|5281{{±|86|76}}

|

|

|0.217 ±0.019

|4.9019804 ±0.0000052

|0.0336 ±0.0015

|412 ±8

| style="background:#FFFF00" |transit

|226.238{{±|1.058|1.049}}

|0.2109{{±|0.0290|0.0260}}

|3238{{±|48|49}}

|

|2.589 ±0.066

|1.133 ±0.024

|3.5819111 ±1.7e-06

|0.03939 ±0.0004

|745 ±14

| style="background:#FFFF00" |transit

|611.54{{±|1.96|2.28}}

|0.63 ±0.02

|3920 ±50

|{{cite journal|last1=Delamer|first1=Megan|last2=Kanodia|first2=Shubham|last3=Cañas|first3=Caleb I.|last4=Müller|first4=Simon|last5=Helled|first5=Ravit|last6=Lin|first6=Andrea S. J.|last7=Libby-Roberts|first7=Jessica E.|last8=Gupta|first8=Arvind F.|last9=Mahadevan|first9=Suvrath|last10=Teske|first10=Johanna|last11=Butler|first11=R. Paul|last12=Yee|first12=Samuel W.|last13=Crane|first13=Jeffrey D.|last14=Shectman|first14=Stephen|last15=Osip|first15=David|last16=Beletsky|first16=Yuri|last17=Monson|first17=Andrew|last18=Alvarado-Montes|first18=Jaime A.|last19=Bender|first19=Chad F.|last20=Dong|first20=Jiayin|last21=Han|first21=Te|last22=Ninan|first22=Joe P.|last23=Robertson|first23=Paul|last24=Roy|first24=Arpita|last25=Schwab|first25=Christian|last26=Stefánsson|first26=Guðmundur|last27=Wright|first27=Jason T.|display-authors=3|title=TOI-4201: An Early M-dwarf Hosting a Massive Transiting Jupiter Stretching Theories of Core-Accretion|journal=The Astrophysical Journal |year=2024 |volume=962 |issue=2 |pages=L22 |doi=10.3847/2041-8213/ad1a19 |doi-access=free |arxiv=2307.06880|bibcode=2024ApJ...962L..22D }}{{Cite encyclopedia |title=The Extrasolar Planet Encyclopaedia — Planet TOI-4201 b|url=https://exoplanet.eu/catalog/toi_4201_b--8752/|access-date=2023-07-19|encyclopedia=Extrasolar Planets Encyclopaedia|date=23 October 1995 }}

|0.0203

|0.216 ±0.023

|9.151201{{±|0.000036|0.000037}}

|

|763.05

| style="background:#FFFF00" |transit

|

|0.9000 ±0.1133

|5243 ±126

|

|0.16 ±0.16

|0.202 ±0.003

|5.5382498{{±|0.0000057|0.0000058}}

|0.05251 ±0.00011

|633.6{{±|6.2|6.3}}

|style="background:#FFFF00"|transit

|200.73

|0.6296 ±0.0086

|3901 ±69

|{{cite journal |last1=Tey |first1=Evan |last2=Huang |first2=Chelsea X. |display-authors=etal |arxiv=2301.01370 |title=TESS Discovery of Twin Planets near 2:1 Resonance around Early M-Dwarf TOI 4342 |journal=The Astronomical Journal |date=January 2023|volume=165 |issue=3 |page=93 |doi=10.3847/1538-3881/acaf88 |bibcode=2023AJ....165...93T |s2cid=255416187 |doi-access=free }}

|0.145 ±0.145

|0.215 ±0.004

|10.688716 ±0.000015

|0.08140 ±0.00017

|508.9 ±5.0

|style="background:#FFFF00"|transit

|200.73

|0.6296 ±0.0086

|3901 ±69

|

|0.9570{{±|0.0890|0.0870}}

|1.348 ±0.081

|4.378081 ±0.000019

|0.0579{{±|0.0010|0.0011}}

|1395{{±|25|22}}

| style="background:#FFFF00" |transit

|1486.69{{±|16.01|15.68}}

|1.36{{±|0.08|0.07}}

|4974 ±57

|{{Cite journal |last1=Pereira |first1=Filipe |last2=Grunblatt |first2=Samuel K |last3=Psaridi |first3=Angelica |last4=Campante |first4=Tiago L |last5=Cunha |first5=Margarida S |last6=Santos |first6=Nuno C |last7=Bossini |first7=Diego |last8=Thorngren |first8=Daniel |last9=Hellier |first9=Coel |last10=Bouchy |first10=François |last11=Lendl |first11=Monika |last12=Mounzer |first12=Dany |last13=Udry |first13=Stéphane |last14=Beard |first14=Corey |last15=Brinkman |first15=Casey L |date=2023-11-27 |title=TESS giants transiting giants V – two hot Jupiters orbiting red giant hosts |url=https://academic.oup.com/mnras/article/527/3/6332/7382226 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=527 |issue=3 |pages=6332–6345 |doi=10.1093/mnras/stad3449 |issn=0035-8711 |doi-access=free |access-date=9 December 2023 |archive-date=9 December 2023 |archive-url=https://web.archive.org/web/20231209143000/https://academic.oup.com/mnras/article/527/3/6332/7382226 |url-status=live |arxiv=2311.06678 }}

|0.30 ±0.03

|1.00 ±0.02

|30.08364 ±0.00005

|0.201 ±0.005

|904{{±|16|17}}

| style="background:#FFFF00" |transit

|861 ±7

|1.19 ±0.03

|6219 ±70

|{{cite journal|arxiv=2304.02139|year=2023|title=Three Long-period Transiting Giant Planets from TESS |last1=Brahm |first1=Rafael |last2=Ulmer-Moll |first2=Solène |last3=Hobson |first3=Melissa J. |last4=Jordán |first4=Andrés |last5=Henning |first5=Thomas |last6=Trifonov |first6=Trifon |last7=Jones |first7=Matías I. |last8=Schlecker |first8=Martin |last9=Espinoza |first9=Nestor |last10=Rojas |first10=Felipe I. |last11=Torres |first11=Pascal |last12=Sarkis |first12=Paula |last13=Tala |first13=Marcelo |last14=Eberhardt |first14=Jan |last15=Kossakowski |first15=Diana |last16=Muñoz |first16=Diego J. |last17=Hartman |first17=Joel D. |last18=Boyle |first18=Gavin |last19=Suc |first19=Vincent |last20=Bouchy |first20=François |last21=Deline |first21=Adrien |last22=Chaverot |first22=Guillaume |last23=Grieves |first23=Nolan |last24=Lendl |first24=Monika |last25=Suarez |first25=Olga |last26=Triaud |first26=Amaury H. M. J. |last27=Crouzet |first27=Nicolas |last28=Dransfield |first28=Georgina |last29=Guillot |first29=Tristan |last30=Cloutier |first30=Ryan |journal=The Astronomical Journal |volume=165 |issue=6 |page=227 |doi=10.3847/1538-3881/accadd |bibcode=2023AJ....165..227B |s2cid=257952381 |display-authors=1 |doi-access=free }}

|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

|564.633{{±|4.250|4.191}}

|1.062{{±|0.059|0.063}}

|5640{{±|89|82}}

|

|2.005 ±0.052

|1.086 ±0.039

|15.266

|0.118 ±0.001

|705 ±10

|style="background:#FFFF00"|transit

|

|0.949 ±0.020

|5433 ±70

|{{Cite journal |last1=Carleo |first1=I. |last2=Malavolta |first2=L. |last3=Desidera |first3=S. |last4=Nardiello |first4=D. |last5=Wang |first5=S. |last6=Turrini |first6=D. |last7=Lanza |first7=A. F. |last8=Baratella |first8=M. |last9=Marzari |first9=F. |last10=Benatti |first10=S. |last11=Biazzo |first11=K. |last12=Bieryla |first12=A. |last13=Brahm |first13=R. |last14=Bonavita |first14=M. |last15=Collins |first15=K. A. |date=2024-02-01 |title=The GAPS programme at TNG. L. TOI-4515 b: An eccentric warm Jupiter orbiting a 1.2 Gyr-old G-star |url=https://ui.adsabs.harvard.edu/abs/2024A&A...682A.135C |journal=Astronomy and Astrophysics |volume=682 |pages=A135 |doi=10.1051/0004-6361/202348207 |issn=0004-6361|arxiv=2311.11903 |bibcode=2024A&A...682A.135C }} Highly eccentric orbit {{nowrap|1=(e = 0.46)}}

|1.49 ±0.13

|1.058{{±|0.110|0.062}}

|9.955810{{±|0.000076|0.000078}}

|0.09940{{±|0.00300|0.00320}}

|

| style="background:#FFFF00" |transit

|704.453{{±|8.033|7.857}}

|1.31{{±|0.07|0.18}}

|4896 ±110

|

|0.00849{{±|0.00629|0.00315}}

|0.126{{±|0.0112|0.00999}}

|3.965991{{±|0.000314|0.000332}}

|0.0359 ±0.0008

|554.16 ±19.14

| style="background:#FFFF00" |transit

|90.704 ±0.0978

|0.392{{±|0.027|0.026}}

|3558{{±|73|83}}

|

|2.30{{±|0.48|0.47}}

|1.118{{±|0.014|0.013}}

|225.11781{{±|0.00025|0.00022}}

|0.768 ±0.005

|318 ±4

| style="background:#FFFF00" |transit

|1107.64{{±|8.25|8.12}}

|1.192 ±0.057

|6096 ±32

|{{Cite journal |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=L. 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 |date=2023-03-01 |title=TOI-4562b: A Highly Eccentric Temperate Jupiter Analog Orbiting a Young Field Star |journal=The Astronomical Journal |volume=165 |issue=3 |pages=121 |doi=10.3847/1538-3881/acb5a2 |arxiv=2208.10854 |bibcode=2023AJ....165..121H |issn=0004-6256 |doi-access=free }}

|0.53 ±0.05

|0.940{{±|0.090|0.120}}

|31.034 ±0.001

|

|

| style="background:#FFFF00" |transit

|1251.94{{±|11.83|11.62}}

|1.34 ±0.06

|5190 ±100

|{{Cite journal |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. |date=2023-02-01 |title=TESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period−Eccentricity Relation for Giant Planets Transiting Evolved Stars |journal=The Astronomical Journal |volume=165 |issue=2 |pages=44 |doi=10.3847/1538-3881/aca670 |arxiv=2210.17062 |bibcode=2023AJ....165...44G |issn=0004-6256 |doi-access=free }}

|~0.0976

|0.607{{±|0.026|0.028}}

|82.6869 ±0.0003

|0.349 ±0.021

|347{{±|12|11}}

| style="background:#FFFF00" |transit

|705.97 ±1.68

|0.89 ±0.05

|5170 ±120

|{{cite journal|last1=Mireles|first1=Ismael|last2=Dragomir|first2=Diana|last3=Osborn|first3=Hugh P.|last4=Hesse|first4=Katharine|last5=Collins|first5=Karen A.|last6=Villanueva|first6=Steven|last7=Bieryla|first7=Allyson|last8=Ciardi|first8=David R.|last9=Stassun|first9=Keivan G.|last10=Harris|first10=Mallory|last11=Lissauer|first11=Jack J.|last12=Schwarz|first12=Richard P.|last13=Srdoc|first13=Gregor|last14=Barkaoui|first14=Khalid|last15=Riffeser|first15=Arno|last16=McLeod|first16=Kim K.|last17=Pepper|first17=Joshua|last18=Grieves|first18=Nolan|last19=Passegger|first19=Vera Maria|last20=Ulmer-Moll|first20=Solène|last21=Rodriguez|first21=Joseph E.|last22=Feliz|first22=Dax L.|last23=Quinn|first23=Samuel|last24=Boyle|first24=Andrew W.|last25=Fausnaugh|first25=Michael|last26=Kunimoto|first26=Michelle|last27=Rowden|first27=Pamela|last28=Vanderburg|first28=Andrew|last29=Wohler|first29=Bill|last30=Jenkins|first30=Jon M.|last31=Latham|first31=David W.|last32=Ricker|first32=George R.|last33=Seager|first33=Sara|last34=Winn|first34=Joshua N. |display-authors=3|title=TOI-4600 b and c: Two Long-period Giant Planets Orbiting an Early K Dwarf|journal=The Astrophysical Journal Letters|publisher=American Astronomical Society|volume=954|issue=1|date=2023-08-30|issn=2041-8205|arxiv=2308.15572|doi=10.3847/2041-8213/aceb69|doi-access=free|page=L15|bibcode=2023ApJ...954L..15M }}

|~0.1510

|0.841 ±0.037

|482.8191{{±|0.0018|0.0017}}

|1.152 ±0.068

|191 ±6

| style="background:#FFFF00" |transit

|705.97 ±1.68

|0.89 ±0.05

|5170 ±120

|{{As of|2023|August}}, longest-period confirmed planet discovered by TESS

|12.89{{±|0.58|0.57}}

|1.042{{±|0.038|0.035}}

|7.24599{{±|0.00022|0.00021}}

|0.0888 ±0.0010

|1677 ±24

| style="background:#FFFF00" |transit

|731 ±3

|1.765 ±0.061

|6264{{±|95|94}}

|Metal enriched gas giant{{cite journal|arxiv=2303.11841|year=2023|title=Discovery of a massive giant planet with extreme density around the sub-giant star TOI-4603|last1=Khandelwal |first1=Akanksha |last2=Sharma |first2=Rishikesh |last3=Chakraborty |first3=Abhijit |last4=Chaturvedi |first4=Priyanka |last5=Ulmer-Moll |first5=Solène |last6=Ciardi |first6=David R. |last7=Boyle |first7=Andrew W. |last8=Baliwal |first8=Sanjay |last9=Bieryla |first9=Allyson |last10=Latham |first10=David W. |last11=Prasad |first11=Neelam J. S. S. V. |last12=Nayak |first12=Ashirbad |last13=Lendl |first13=Monika |last14=Mordasini |first14=Christoph |journal=Astronomy & Astrophysics |volume=672 |pages=L7 |doi=10.1051/0004-6361/202245608 |bibcode=2023A&A...672L...7K |s2cid=257637141 }}

|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

|1072.41{{±|12.05|11.79}}

|1.242{{±|0.072|0.077}}

|6058{{±|99|94}}

|

|0.67 ±0.14

|0.756 ±0.024

|1.52275959{{±|0.00000032|0.00000035}}

|0.01845 ±0.00059

|624 ±30

| style="background:#FFFF00" |transit

|261.390{{±|2.114|2.081}}

|0.3357 ±0.0081

|3390 ±120

|{{Cite journal |last1=Triaud |first1=Amaury H M J |last2=Dransfield |first2=Georgina |last3=Kagetani |first3=Taiki |last4=Timmermans |first4=Mathilde |last5=Narita |first5=Norio |last6=Barkaoui |first6=Khalid |last7=Hirano |first7=Teruyuki |last8=Rackham |first8=Benjamin V |last9=Mori |first9=Mayuko |last10=Baycroft |first10=Thomas |last11=Benkhaldoun |first11=Zouhair |last12=Burgasser |first12=Adam J |last13=Caldwell |first13=Douglas A |last14=Collins |first14=Karen A |last15=Davis |first15=Yasmin T |date=2023-07-04 |title=An M dwarf accompanied by a close-in giant orbiter with SPECULOOS |url=https://academic.oup.com/mnrasl/article/525/1/L98/7235807 |journal=Monthly Notices of the Royal Astronomical Society: Letters |language=en |volume=525 |issue=1 |pages=L98–L104 |doi=10.1093/mnrasl/slad097 |issn=1745-3925 |doi-access=free |access-date=9 December 2023 |archive-date=9 December 2023 |archive-url=https://web.archive.org/web/20231209173853/https://academic.oup.com/mnrasl/article/525/1/L98/7235807 |url-status=live |arxiv=2308.02253 }}

|

|0.423{{±|0.014|0.012}}

|5.4588385{{±|0.0000070|0.0000072}}

|0.06519{{±|0.00087|0.00082}}

|1442{{±|46|40}}

| style="background:#FFFF00" |transit

|523.201{{±|5.264|5.160}}

|1.240{{±|0.050|0.046}}

|6150{{±|110|130}}

|{{Cite journal |last1=Fairnington |first1=Tyler R |last2=Nabbie |first2=Emma |last3=Huang |first3=Chelsea X |last4=Zhou |first4=George |last5=Foo |first5=Orion |last6=Millholland |first6=Sarah |last7=Wright |first7=Duncan |last8=Belinski |first8=Alexandre A |last9=Bieryla |first9=Allyson |last10=Ciardi |first10=David R |last11=Collins |first11=Karen A |last12=Collins |first12=Kevin I |last13=Everett |first13=Mark |last14=Howell |first14=Steve B |last15=Lissauer |first15=Jack J |date=2023-10-09 |title=TOI-5126: A hot super-Neptune and warm Neptune pair discovered by TESS and CHEOPS |journal=Monthly Notices of the Royal Astronomical Society |volume=527 |issue=3 |pages=8768–8783 |language=en |doi=10.1093/mnras/stad3036 |issn=0035-8711|doi-access=free }}

|

|0.344{{±|0.015|0.014}}

|17.8999{{±|0.0018|0.0013}}

|0.1439{{±|0.0019|0.0018}}

|971.0{{±|31.0|27.0}}

| style="background:#FFFF00" |transit

|523.201{{±|5.264|5.160}}

|1.240{{±|0.050|0.046}}

|6150{{±|110|130}}

|

|1.08 ±0.06

|1.03 ±0.03

|1.630757 ±0.000001

|0.0199 ±0.0002

|

| style="background:#FFFF00" |transit

|281.960{{±|1.363|1.350}}

|0.394 ±0.011

|3430 ±54

|{{Cite journal |last1=Kanodia |first1=Shubham |last2=Mahadevan |first2=Suvrath |last3=Libby-Roberts |first3=Jessica |last4=Stefansson |first4=Gudmundur |last5=Cañas |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. |date=2023-03-01 |title=TOI-5205b: A Short-period Jovian Planet Transiting a Mid-M Dwarf |journal=The Astronomical Journal |volume=165 |issue=3 |pages=120 |doi=10.3847/1538-3881/acabce |arxiv=2209.11160 |bibcode=2023AJ....165..120K |issn=0004-6256 |doi-access=free }}

|0.54 ±0.07

|1.06 ±0.04

|2.930289 ±0.000004

|0.034{{±|0.004|0.003}}

|675{{±|42|30}}

| style="background:#FFFF00" |transit

|525 ±2

|0.54 ±0.02

|3586 ±88

|

|0.412 ±0.040

|0.946 ±0.021

|3.7926220 ±0.0000062

|0.04041 ±0.00075

|689 ±12

| style="background:#FFFF00" |transit

|451.293{{±|4.357|4.276}}

|0.612 ±0.034

|3747 ±64

|{{Cite journal |last1=Hartman |first1=J. D. |last2=Bakos |first2=G. á. |last3=Csubry |first3=Z. |last4=Howard |first4=A. W. |last5=Isaacson |first5=H. |last6=Giacalone |first6=S. |last7=Chontos |first7=A. |last8=Narita |first8=N. |last9=Fukui |first9=A. |last10=de Leon |first10=J. P. |last11=Watanabe |first11=N. |last12=Mori |first12=M. |last13=Kagetani |first13=T. |last14=Fukuda |first14=I. |last15=Kawai |first15=Y. |date=2023-10-01 |title=TOI 4201 b and TOI 5344 b: Discovery of Two Transiting Giant Planets around M-dwarf Stars and Revised Parameters for Three Others |journal=The Astronomical Journal |volume=166 |issue=4 |pages=163 |doi=10.3847/1538-3881/acf56e |arxiv=2307.06809 |bibcode=2023AJ....166..163H |issn=0004-6256 |doi-access=free }}

|0.0371{{±|0.0151|0.0148}}

|0.314 ±0.017

|4.77271{{±|0.00016|0.00014}}

|0.057 ±0.003

|1242 ±37

| style="background:#FFFF00" |transit

|426.792{{±|2.237|2.211}}

|1.146 ±0.013

|6000 ±75

|{{Cite journal |last1=Mantovan |first1=G. |last2=Malavolta |first2=L. |last3=Desidera |first3=S. |last4=Zingales |first4=T. |last5=Borsato |first5=L. |last6=Piotto |first6=G. |last7=Maggio |first7=A. |last8=Locci |first8=D. |last9=Polychroni |first9=D. |last10=Turrini |first10=D. |last11=Baratella |first11=M. |last12=Biazzo |first12=K. |last13=Nardiello |first13=D. |last14=Stassun |first14=K. |last15=Nascimbeni |first15=V. |date=2023 |title=The GAPS programme at TNG XLIX. TOI-5398, the youngest compact multi-planet system composed of an inner sub-Neptune and an outer warm Saturn |journal=Astronomy and Astrophysics |volume=682 |doi=10.1051/0004-6361/202347472 |arxiv=2310.16888|bibcode=2024A&A...682A.129M }}

|0.063 ±0.013

|0.438 ±0.007

|47.73022{{±|0.00014|0.00013}}

|0.249 ±0.005

|513{{±|8|7}}

| style="background:#FFFF00" |transit

|539.441{{±|2.293|2.277}}

|0.905{{±|0.039|0.041}}

|5485 ±63

|{{Cite journal |last1=Ulmer-Moll |first1=S. |last2=Osborn |first2=H. P. |last3=Tuson |first3=A. |last4=Egger |first4=J. A. |last5=Lendl |first5=M. |last6=Maxted |first6=P. |last7=Bekkelien |first7=A. |last8=Simon |first8=A. E. |last9=Olofsson |first9=G. |last10=Adibekyan |first10=V. |last11=Alibert |first11=Y. |last12=Bonfanti |first12=A. |last13=Bouchy |first13=F. |last14=Brandeker |first14=A. |last15=Fridlund |first15=M. |date=June 2023 |title=TOI-5678b: A 48-day transiting Neptune-mass planet characterized with CHEOPS and HARPS |url=https://www.aanda.org/10.1051/0004-6361/202245478 |journal=Astronomy & Astrophysics |volume=674 |pages=A43 |doi=10.1051/0004-6361/202245478 |arxiv=2306.04295 |bibcode=2023A&A...674A..43U |s2cid=259095853 |issn=0004-6361}}

|

|0.288

|3.7711160{{±|0.0000115|0.0000107}}

|

|949.07

| style="background:#FFFF00" |transit

|292.357{{±|0.881|0.876}}

|0.7575 ±0.0593

|4590 ±126

|

|0.0116{{±|0.00849|0.00440}}

|0.145{{±|0.0171|0.0114}}

|4.164753{{±|0.00038|0.000427}}

|0.0352 ±0.0011

|518.01 ±20.15

| style="background:#FFFF00" |transit

|90.704 ±0.0978

|0.337{{±|0.027|0.032}}

|3514{{±|95|94}}

|

|0.0339

|0.292 ±0.011

|5.383050{{±|0.000207|0.000200}}

|

|678.87

| style="background:#FFFF00" |transit

|

|0.8700 ±0.1032

|5134 ±121

|

|0.048{{±|0.014|0.013}}

|0.174 ±0.011

|1.4468849{{±|0.0000022|0.0000016}}

|0.02359 ±0.00100

|1329{{±|31|30}}

| style="background:#FFFF00" |transit

|328.075{{±|1.595|1.579}}

|0.853 ±0.038

|

|{{Cite journal |last1=Maciejewski |first1=G |last2=Golonka |first2=J |last3=Łoboda |first3=W |last4=Ohlert |first4=J |last5=Fernández |first5=M |last6=Aceituno |first6=F |date=2023-07-04 |title=A hot super-Earth planet in the WASP-84 planetary system |url=https://academic.oup.com/mnrasl/article/525/1/L43/7199781 |journal=Monthly Notices of the Royal Astronomical Society: Letters |language=en |volume=525 |issue=1 |pages=L43–L49 |doi=10.1093/mnrasl/slad078 |doi-access=free |issn=1745-3925 |arxiv=2305.09177 |access-date=9 December 2023 |archive-date=1 January 2024 |archive-url=https://web.archive.org/web/20240101025944/https://academic.oup.com/mnrasl/article-abstract/525/1/L43/7199781?redirectedFrom=fulltext |url-status=live }}

|0.139 ±0.029

|1.464{{±|0.059|0.057}}

|6.2463345 ±0.0000003

|0.0676 ±0.0015

|1254 ±31

| style="background:#FFFF00" |transit

|1180.97{{±|17.56|17.06}}

|1.059{{±|0.067|0.068}}

|6078 ±120

|{{Cite journal |last1=Barkaoui |first1=Khalid |last2=Pozuelos |first2=Francisco J. |last3=Hellier |first3=Coel |last4=Smalley |first4=Barry |last5=Nielsen |first5=Louise D. |last6=Dorn |first6=Caroline |last7=Niraula |first7=Prajwal |last8=Gillon |first8=Michaël |last9=de Wit |first9=Julien |last10=Helled |first10=Ravit |last11=Müller |first11=Simon |last12=Jehin |first12=Emmanuel |last13=Demory |first13=Brice-Olivier |last14=Van Grootel |first14=V. |last15=Soubkiou |first15=Abderahmane |date=2023 |title=WASP-193b: An extremely low-density super-Neptune |journal=Astrophysics |doi=10.1038/s41550-024-02259-y |arxiv=2307.08350}}

|8.25 ±4.25

|

|2560 ±730

|0.970 ±0.050

|325{{±|15|10}}

| style="background:#FF6CDA" |imaging

|

|0.01310 ±0.00597

|415 ±20

|{{Cite journal |last1=Calissendorff |first1=Per |last2=De Furio |first2=Matthew |last3=Meyer |first3=Michael |last4=Albert |first4=Loïc |last5=Aganze |first5=Christian |last6=Ali-Dib |first6=Mohamad |last7=Bardalez Gagliuffi |first7=Daniella C. |last8=Baron |first8=Frederique |last9=Beichman |first9=Charles A. |last10=Burgasser |first10=Adam J. |last11=Cushing |first11=Michael C. |last12=Faherty |first12=Jacqueline Kelly |last13=Fontanive |first13=Clémence |last14=Gelino |first14=Christopher R. |last15=Gizis |first15=John E. |date=2023-04-01 |title=JWST/NIRCam Discovery of the First Y+Y Brown Dwarf Binary: WISE J033605.05–014350.4 |journal=The Astrophysical Journal Letters |volume=947 |issue=2 |pages=L30 |doi=10.3847/2041-8213/acc86d |arxiv=2303.16923 |bibcode=2023ApJ...947L..30C |issn=2041-8205 |doi-access=free }}

|0.003963425 ±0.0006605

|

|15.564 ±0.015

|0.0672 ±0.0014

|250.0 ±6.6

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

|31.228

|0.167 ±0.011

|3158 ±54

|Habitable zone planet{{cite journal|arxiv=2301.02477|year=2023|title=The CARMENES search for exoplanets around M dwarfs. Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass starr|doi=10.1051/0004-6361/202245322 |last1=Kossakowski |first1=D. |last2=Kürster |first2=M. |last3=Trifonov |first3=T. |last4=Henning |first4=Th. |last5=Kemmer |first5=J. |last6=Caballero |first6=J. A. |last7=Burn |first7=R. |last8=Sabotta |first8=S. |last9=Crouse |first9=J. S. |last10=Fauchez |first10=T. J. |last11=Nagel |first11=E. |last12=Kaminski |first12=A. |last13=Herrero |first13=E. |last14=Rodríguez |first14=E. |last15=González-Álvarez |first15=E. |last16=Quirrenbach |first16=A. |last17=Amado |first17=P. J. |last18=Ribas |first18=I. |last19=Al |first19=et |last20=Aceituno |first20=J. |last21=Béjar |first21=V. J. S. |last22=Baroch |first22=D. |last23=Bastelberger |first23=S. T. |last24=Chaturvedi |first24=P. |last25=Cifuentes |first25=C. |last26=Dreizler |first26=S. |last27=Jeffers |first27=S. V. |last28=Kopparapu |first28=R. |last29=Lafarga |first29=M. |last30=López-González |first30=M. J. |display-authors=1 |journal=Astronomy & Astrophysics |volume=670 |bibcode=2023A&A...670A..84K |s2cid=265978789 }}{{Cite encyclopedia |title=The Extrasolar Planet Encyclopaedia — Wolf 1069 b |url=https://exoplanet.eu/catalog/wolf_1069_b--8577/ |access-date=2023-01-09 |encyclopedia=Extrasolar Planets Encyclopaedia |date=23 October 1995 |archive-date=1 January 2024 |archive-url=https://web.archive.org/web/20240101030019/https://exoplanet.eu/catalog/wolf_1069_b--8577/ |url-status=live }}