Next-Generation Transit Survey

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|image1=The Next-Generation Transit Survey (NGTS) at Paranal (1502d).jpg{{!}}NGST facility with the VLT (left) and VISTA (right) in the background

|image2=The Next-Generation Transit Survey (NGTS) at Paranal (1502f).jpg{{!}}Engineering rendering the facility

|image3=The Next-Generation Transit Survey (NGTS) at Paranal (1502c).jpg{{!}}NGTS observations at night

|image4=The Next-Generation Transit Survey (NGTS) at Paranal (1502b).jpg{{!}}The array of twelve 0.2-metre robotic telescopes

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Top: NGTS facility with the VLT (left) and VISTA (right) in the background
Middle: the facility (rendered) and night observations
Bottom: The array of twelve 0.2-meter robotic telescopes

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The Next-Generation Transit Survey (NGTS) is a ground-based robotic search for exoplanets. The facility is located at Paranal Observatory in the Atacama Desert in northern Chile, about 2 km from ESO's Very Large Telescope and 0.5 km from the VISTA Survey Telescope. Science operations began in early 2015. The astronomical survey is managed by a consortium of seven European universities and other academic institutions from Chile, Germany, Switzerland, and the United Kingdom. Prototypes of the array were tested in 2009 and 2010 on La Palma, and from 2012 to 2014 at Geneva Observatory.

The aim of NGTS is to discover super-Earths and exo-Neptunes transiting relatively bright and nearby stars with an apparent magnitude of up to 13. The survey uses transit photometry, which precisely measures the dimming of a star to detect the presence of a planet when it crosses in front of it. NGTS consists of an array of twelve commercial 0.2-metre telescopes (f/2.8), each equipped with a red-sensitive CCD camera operating in the visible and near-infrared at 600–900 nm. The array covers an instantaneous field of view of 96 square degrees (8 deg² per telescope) or around 0.23% of the entire sky. NGTS builds heavily on experience with SuperWASP, using more sensitive detectors, refined software, and larger optics, though having a much smaller field of view. Compared to the Kepler space telescope with its original Kepler field of 115 square degrees, the sky area covered by NGTS will be sixteen times larger, because the survey intends to scan four different fields every year over a period of four years. As a result, the sky coverage will be comparable to that of Kepler's K2 phase.

NGTS is suited to ground-based photometric follow-up of exoplanet candidates from space-based telescopes such as TESS, Gaia and PLATO. In turn, larger instruments such as HARPS, ESPRESSO and VLT-SPHERE may follow-up on NGTS discoveries with a detailed characterization to measure the mass of a large number of targets using Doppler spectroscopy (wobble method) and make it possible to determine the exoplanet's density, and hence whether it is gaseous or rocky. This detailed characterization allows to fill the gap between Earth-sized planets and gas giants as other ground-based surveys can only detect Jupiter-sized exoplanets, and Kepler{{'}}s Earth-sized planets are often too far away or orbit stars too dim to allow for the planet's mass determination. NGTS's wider field of view also enables it to detect a larger number of more-massive planets around brighter stars.

Science mission

File:The Next-Generation Transit Survey (NGTS) at Paranal - Vid.ogg

Ground-based surveys for extrasolar planets such as WASP and the HATNet Project have discovered many large exoplanets, mainly Saturn- and Jupiter-sized gas giants. Space-based missions such as CoRoT and the Kepler survey have extended the results to smaller objects, including rocky super-Earth- and Neptune-sized exoplanets. Orbiting space missions have a higher accuracy of stellar brightness measurement than is possible via ground-based measurements, but they have probed a relatively small region of sky. Unfortunately, most of the smaller candidates orbit stars that are too faint for confirmation by radial-velocity measurements. The masses of these smaller candidate planets are hence either unknown or poorly constrained, such that their bulk composition cannot be estimated.

By focusing on super-Earth- to Neptune-sized targets orbiting cool, small, but bright stars of K and early-M spectral type, over an area considerably larger than that covered by space missions, NGTS is intended to provide prime targets for further scrutiny by telescopes such as the Very Large Telescope (VLT), Extremely Large Telescope (ELT), and the James Webb Space Telescope (JWST). Such targets are more readily characterized in terms of their atmospheric composition, planetary structure, and evolution than smaller targets orbiting larger stars.

In follow-up observations by larger telescopes, powerful means will be available to probe the atmospheric composition of exoplanets discovered by NGTS. For example, during secondary eclipse, when the star occults the planet, a comparison between the in-transit and out-of-transit flux allows computation of a difference spectrum representing the thermal emission of the planet. Calculation of the transmission spectrum of the planet's atmosphere can be obtained by measuring the small spectral changes in the spectrum of the star that arise during the planet's transit. This technique requires an extremely high signal-to-noise ratio, and has thus far been successfully applied to only a few planets orbiting small, nearby, relatively bright stars, such as HD 189733 b and GJ 1214 b. NGTS is intended to greatly increase the number of planets that area analyzable using such techniques. Simulations of expected NGTS performance reveal the potential of discovering approximately 231 Neptune- and 39 super-Earth-sized planets amenable to detailed spectrographic analysis by the VLT, compared to only 21 Neptune- and 1 super-Earth-sized planets from the Kepler data.

Instrument

= Development =

The scientific goals of the NGTS require being able to detect transits with a precision of 1 mmag at 13th magnitude. Although at ground level this level of accuracy was routinely achievable in narrow-field observations of individual objects, it was unprecedented for a wide-field survey. To achieve this goal, the designers of the NGTS instruments drew upon an extensive hardware and software heritage from the WASP project, in addition to developing many refinements in prototype systems operating on La Palma during 2009 and 2010, and at the Geneva Observatory from 2012 to 2014.

= Telescope array =

NGTS employs an automated array of twelve 20-centimeter f/2.8 telescopes on independent equatorial mounts and operating at orange to near-infrared wavelengths (600–900 nm). It is located at the European Southern Observatory's Paranal Observatory in Chile, a location noted for low water-vapor and excellent photometric conditions.

= Combined search =

The NGTS telescope project cooperates closely with ESO's large telescopes. ESO facilities available for follow-up studies include the High Accuracy Radial Velocity Planet Searcher (HARPS) at La Silla Observatory; ESPRESSO for radial-velocity measurements at the VLT; SPHERE, an adaptive optics system and coronagraphic facility at the VLT that directly images extrasolar planets; and a variety of other VLT and planned ELT instruments for atmospheric characterization.

Partnership

Although located at Paranal Observatory, NGTS is not in fact operated by ESO, but by a consortium of seven academic institutions from Chile, Germany, Switzerland, and the United Kingdom:

Results

On 31 October 2017, the discovery of NGTS-1b, a confirmed hot Jupiter-sized extrasolar planet orbiting NGTS-1, an M-dwarf star, about half the mass and radius of the Sun, every 2.65 days, was reported by the survey team. Daniel Bayliss, of the University of Warwick, and lead author of the study describing the discovery of NGTS-1b, stated, "The discovery of NGTS-1b was a complete surprise to us—such massive planets were not thought to exist around such small stars – importantly, our challenge now is to find out how common these types of planets are in the Galaxy, and with the new Next-Generation Transit Survey facility we are well-placed to do just that."
On 3 September 2018, the discovery of NGTS-4b, a sub-Neptune-sized planet transiting a 13th magnitude K-dwarf in a 1.34 day orbit. NGTS-4b has a mass 20.6 ± 3.0 {{Earth mass|link=true}} and radius 3.18 ± 0.26 {{Earth radius|link=true}}, which places it well within the so-called "Neptunian desert". The mean density of the planet (3.45 ± 0.95 g cm⁻³) is consistent with a composition of 100% H2O or a rocky core with a volatile envelope.

Discoveries

=Planets=

This is a list of planets discovered by this survey. This list is incomplete, and requires more information.

{{legend|#d5fdf4|Indicates that the planet orbits one or both stars in a binary system}}

class="toccolours sortable" border="1" cellspacing="0" cellpadding="2" style="margin:auto; text-align:center; border-collapse:collapse; margin-left:0; margin-right:0;"

style="background:#a0b0ff;"

! Star

! Distance (ly)

! Planet

! Mass
({{Jupiter mass|link=y}})

! Radius
({{Jupiter radius|link=y}})

! Orbital
period
(d)

! Semimajor
axis
(AU)

! Orbital
eccentricity

! Inclination
(°)

! Discovery
year

NGTS-1

|Columba

|{{RA|05|30|51.41}}

|{{DEC

36|37|51.53}}

|15.67

|711

|M0.5 V

|NGTS-1b

|0.812

|1.33

|2.65

|0.023

|0.016

|85.27

|2017

NGTS-2

|Centaurus

|{{RA|14|20|29.46}}

|{{DEC

31|12|07.45}}

|10.79

|1,162

|F5 V

|NGTS-2b

|0.74

|1.595

|4.51

|0.04

|83.45

|2018

style ="background:#d5fdf4;"

|NGTS-3

|Columba

|{{RA|06|17|46.74}}

|{{DEC

35|42|22.91}}

|14.669

|2,426

|G6 V + K1 V

|NGTS-3Ab

|2.38

|1.48

|1.68

|0.02

|0?

|89.56

|2018

NGTS-4

|Columba

|{{RA|05|58|23.75}}

|{{DEC

30|48|42.36}}

|13.12

|922

|K2 V

|NGTS-4b

|0.06

|0.25

|1.34

|0.02

|82.5 ± 5.8

|2018

style ="background:#d5fdf4;"

|NGTS-5

|Virgo

|{{RA|14|44|13.97}}

|{{DEC|05|36|19.42}}

|13.77

|1,009

|K2 V + M2 V

|NGTS-5Ab

|0.229

|1.136

|3.36

|0.04

|0?

|86.6 ± 0.2

|2019

style ="background:#d5fdf4;"

|NGTS-6

|Caelum

|{{RA|05|03|10.90}}

|{{DEC

30|23|57.72}}

|14.12

|1,014

|K4 V

|NGTS-6Ab

|1.339 ± 0.028

|1.326

|0.882

|0.01

|78.231

|2019

NGTS-8

|Capricornus

|{{RA|21|55|54.22}}

|{{DEC

14|04|6.38}}

|13.68

|1,399

|K0 V

|NGTS-8b

|0.93 ± 0.01

|1.09 ± 0.03

|2.50

|0.035

|0.01

|86.9 ± 0.5

|2019

NGTS-9

|Hydra

|{{RA|09|27|40.95}}

|{{DEC

19|20|51.53}}

|12.80

|1,986

|F8 V

|NGTS-9b

|2.90 ± 0.17

|1.07 ± 0.06

|4.435

|0.058

|0.06

|84.1 ± 0.4

|2019

style ="background:#d5fdf4;"

|NGTS-10

|Lepus

|{{RA|06|07|29.31}}

|{{DEC|−25|35|40.61}}

|14.34

|1,059

|K5 V + K5 V

|NGTS-10Ab

|2.162

|1.205

|0.77

|0.0143

|0?

|2019

rowspan="2"|NGTS-11

|rowspan="2"|Cetus

|rowspan="2"|{{RA|01|34|05.14}}

|rowspan="2"|{{DEC

14|25|09.16}}

|rowspan="2"|12.46

|rowspan="2"|621

|rowspan="2"|K2 V

|NGTS-11b

|0.344

|0.817

|35.455

|0.201

|0.11

|2020

NGTS-11c

|0.419

|12.77

|2022

NGTS-12

|Centaurus

|{{RA|11|44|59.99}}

|{{DEC

35|48|26.03}}

|12.38

|1,456

|G4 V

|NGTS-12b

|0.208

|1.048

|7.53

|0.0757

|0?

|88.90 ± 0.76

|2020

NGTS-13

|Centaurus

|{{RA|11|44|57.68}}

|{{DEC

38|08|22.96}}

|12.70

|2,151

|G2 IV

|NGTS-13b

|4.84

|1.142

|4.119

|0.0549

|0.086

|88.7

|2021

style ="background:#d5fdf4;"

|NGTS-14

|Grus

|{{RA|21|54|04.23}}

|{{DEC

38|22|38.79}}

|13.24

|1,060

|K1 V + M3 V

|NGTS-14Ab

|0.092

|0.44

|3.536

|0.0403

|0?

|86.7

|2021

NGTS-15

|Eridanus

|{{RA|04|53|25.27}}

|{{DEC

32|48|01.25}}

|14.67

|2,626

|G6 V

|NGTS-15b

|0.751

|1.10 ± 0.10

|3.276

|0.0441

|2021

NGTS-16

|Fornax

|{{RA|03|53|03.34}}

|{{DEC

30|48|16.71}}

|14.36

|3,008

|G7 V

|NGTS-16b

|0.667

|1.30

|4.845

|0.0523

|2021

NGTS-17

|Caelum

|{{RA|04|51|36.14}}

|{{DEC

34|13|34.18}}

|14.31

|3,366

|G4 V

|NGTS-17b

|0.764

|1.24 ± 0.11

|3.242

|0.0391

|2021

NGTS-18

|Hydra

|{{RA|12|02|11.09}}

|{{DEC

35|32|54.99}}

|14.54

|3,689

|G5 V

|NGTS-18b

|0.409

|1.21 ± 0.18

|3.051

|0.0448

|2021

NGTS-20

|Eridanus

|{{RA|46|17|33.43}}

|{{DEC

21|56|01.1}}

|11.79

|1,248

|G1 IV

|NGTS-20b

|2.98

|1.07±0.04

|54.189

|0.313

|0.432 ± 0.023

|88.4 ± 0.6

|2022

NGTS-21

|Sculptor

|{{RA|20|45|01.99}}

|{{DEC

35|25|40.23}}

|14.82

|2,090

|K3 V

|NGTS-21b

|2.36 ± 0.21

|1.33 ± 0.03

|1.543

|0.0236

|83.85 ± 0.44

|2022

HATS-54 (NGTS-22)Discovered by HATNet, updated parameters by NGTS.

|Phoenix

|{{RA|13|22|32.4}}

|{{DEC

44|41|20.0}}

|13.914

|2,348

|G6 V

|HATS-54b (NGTS-22b)

|1.015 ± 0.024

|0.753 ± 0.057

|2.544

|0.0370

|83.67 ± 0.34

|2018

NGTS-23

|Horologium

|{{RA|04|41|43.6}}

|{{DEC

40|02|41.0}}

|14.010

|3,232

|F9 V

|NGTS-23b

|0.613 ± 0.097

|1.267 ± 0.030

|4.076

|0.0504

|89.12

|2022

NGTS-24

|Antlia

|{{RA|11|14|15.3}}

|{{DEC

37|54|36.5}}

|13.192

|2,364

|G2 IV

|NGTS-24b

|0.520

|1.214

|3.467

|0.0479

|82.61

|2022

NGTS-25

|Sagittarius

|{{RA|20|29|40.3}}

|{{DEC

39|01|55.5}}

|14.266

|1,686

|K0 V

|NGTS-25b

|0.639

|1.023

|2.823

|0.0388

|89.34

|2022

NGTS-26

|Centaurus

|{{RA|14|30|43.99}}

|{{DEC

31|43|56.83}}

|14.90

|3,611

|G6 V

|NGTS-26b

|0.292

|1.328

|4.520

|0.0490

|86.43

|2024

NGTS-27

|Centaurus

|{{RA|13|44|06.37}}

|{{DEC

32|31|22.71}}

|13.50

|3,187

|G3

|NGTS-27b

|0.593

|1.396

|3.370

|0.0446

|86.2

|2024

=Brown dwarfs=

In addition, the survey has discovered three brown dwarfs.

class="toccolours sortable" border="1" cellspacing="0" cellpadding="2" style="margin:auto; text-align:center; border-collapse:collapse; margin-left:0; margin-right:0;"

style="background:#a0b0ff;"

! Star

! Distance (ly)

! Planet

! Mass
({{Jupiter mass|link=y}})

! Radius
({{Jupiter radius|link=y}})

! Orbital
period
(d)

! Semimajor
axis
(AU)

! Orbital
eccentricity

! Inclination
(°)

! Discovery
year

style="background:#d5fdf4;"

|NGTS-7 A

|Sculptor

|{{RA|23|30|05.26}}

|{{DEC

38|58|11.70}}

|14.34

|449

|M3/4 V + M3/4 V

|NGTS-7Ab

|75.5

|1.349

|16.22 h

|0.0139

|0?

|88.43520

|2019

NGTS-19

|Libra

|{{RA|15|16|31.6}}

|{{DEC

25|42|17.24}}

|14.12

|1,223

|K3 V

|NGTS-19b

|69.5

|1.034

|17.84

|0.1296

|0.3767

|88.72

|2021

style="background:#d5fdf4;"

|NGTS-28 A

|Hydra

|{{RA|14|11|43.0}}

|{{DEC

29|58|28.39}}

|402

|M1 V

|NGTS-28Ab

|69.0

|0.95

|1.254

|0.0202

|0.0404

|85.36

|2024

= Other exoplanet search projects =

{{hatnote|For a complete list see footer "Exoplanet search projects"}}

HATNet Project (HAT)
Miniature Exoplanet Radial Velocity Array (MINERVA)
Kilodegree Extremely Little Telescope (KELT)
Trans-Atlantic Exoplanet Survey (TrES)
Wide Angle Search for Planets (WASP and SuperWASP)
XO Telescope
Microlensing Observations in Astrophysics (MOA)
Optical Gravitational Lensing Experiment (OGLE)
Anglo-Australian Planet Search (AAPS)
Cool Companions on Ultrawide Orbits (COCONUTS)
Transiting Planets and Planetesimals Small Telescope (TRAPPIST)
Search for Habitable Planets Eclipsing Ultra-cool Stars (SPECULOOS)

Notes

References

{{reflist

|refs=

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{{cite web |title=About NGTS |publisher=Next Generation Transit Survey |url=http://www.ngtransits.org/ |access-date=22 May 2015 |archive-url=https://web.archive.org/web/20150531140608/http://www.ngtransits.org/ |archive-date=31 May 2015 |url-status=dead }}

{{cite journal |doi=10.1051/epjconf/20134713002 |title=The Next Generation Transit Survey (NGTS) |url=http://www.epj-conferences.org/articles/epjconf/pdf/2013/08/epjconf_hpcs2012_13002.pdf |journal=EPJ Web of Conferences |volume=47 |pages=13002 |year=2013 |last1=Wheatley |first1=P. J. |last2=Pollacco |first2=D. L. |last3=Queloz |first3=D. |last4=Rauer |first4=H. |last5=Watson |first5=C. A. |last6=West |first6=R. G. |last7=Chazelas |first7=B. |last8=Louden |first8=T. M. |last9=Walker |first9=S. |last10=Bannister |first10=N. |last11=Bento |first11=J. |last12=Burleigh |first12=M. |last13=Cabrera |first13=J. |last14=Eigmüller |first14=P. |last15=Erikson |first15=A. |last16=Genolet |first16=L. |last17=Goad |first17=M. |last18=Grange |first18= A. |last19=Jordán |first19=A. S. |last20=Lawrie |first20=K. |last21=McCormac |first21=J. |last22=Neveu |first22=M. |bibcode = 2013EPJWC..4713002W|arxiv = 1302.6592 |s2cid=51743906 }}

{{cite web |url=https://star.pst.qub.ac.uk/webdav/public/stfc2014/posters/a1/NGTS%20-%20Watson%20v2%20FINAL.pdf |title=Searching for Super-Earths |work=Queen's University |date=2014 |access-date=2 September 2015}}

{{cite web |last1=McCormac |first1=J. |last2=Pollacco |first2=D. |last3=The NGTS Consortium |title=The Next Generation Transit Survey Prototyping Phase |url=http://www.astroscu.unam.mx/rmaa/RMxAC..45/PDF/RMxAC..45_file6-02.pdf |access-date=22 May 2015}}

{{cite web |url=https://www.science.org/content/article/new-exoplanet-hunter-opens-its-eyes-search-super-earths |title=New exoplanet hunter opens its eyes to search for super-Earths |author=Daniel Clery |publisher=Science |date=14 January 2015}}

{{cite web |title=NGTS Science Programme |url=http://www.ngtransits.org/science.shtml |publisher=Next Generation Transit Survey |access-date=22 May 2015 |archive-url=https://web.archive.org/web/20171216003138/http://www.ngtransits.org/science.shtml |archive-date=16 December 2017 |url-status=dead }}

{{cite web |title=SPHERE - Spectro-Polarimetric High-contrast Exoplanet REsearch |url=http://www.eso.org/sci/facilities/paranal/instruments/sphere.html |publisher=European Southern Observatory |access-date=23 May 2015}}

{{Cite journal

|display-authors=6

|title=NGTS-1b: A hot Jupiter transiting an M-dwarf

|journal=Monthly Notices of the Royal Astronomical Society

|volume=475

|issue=4

|pages=4467

|year=2017

|doi=10.1093/mnras/stx2778

|doi-access=free |arxiv=1710.11099 |bibcode=2018MNRAS.475.4467B |s2cid=39357327}}

{{cite web |last=Lewin |first=Sarah |title=Monster Planet, Tiny Star: Record-Breaking Duo Puzzles Astronomers |url=https://www.space.com/38625-monster-planet-circles-tiny-star.html |date=31 October 2017 |work=Space.com |access-date=1 November 2017 }}

{{cite web |author=Staff |title='Monster' planet discovery challenges formation theory |url=https://phys.org/news/2017-10-monster-planet-discovery-formation-theory.html |date=31 October 2017 |work=Phys.org |access-date=1 November 2017 }}

{{Cite journal

|first1 = Peter J |last1 =Wheatley

|first2 = Richard G |last2 =West

|first3 = Michael R |last3 = Goad

|first4 = James S |last4 = Jenkins

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|first6 = Didier |last6 = Queloz

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|first8 = Stéphane |last8 =Udry

|first9 = Christopher A |last9 =Watson

|first10 = Bruno |last10 =Chazelas

|first11 = Philipp |last11 =Eigmüller

|date = 2017

|title = The Next Generation Transit Survey (NGTS)

|journal = Monthly Notices of the Royal Astronomical Society

|volume = 475

|issue = 4

|pages = 4476–4493

|doi = 10.1093/mnras/stx2836

|doi-access= free

|hdl= 1885/204054

|hdl-access= free

}}

{{cite journal |arxiv=1805.10449|doi=10.1093/mnras/sty2581 |title=NGTS-2b: An inflated hot-Jupiter transiting a bright F-dwarf |year=2018 |last1=Raynard |first1=Liam |last2=Goad |first2=Michael R. |last3=Gillen |first3=Edward |last4=Nielsen |first4=Louise D. |last5=Watson |first5=Christopher A. |last6=Thompson |first6=Andrew P G. |last7=McCormac |first7=James |last8=Bayliss |first8=Daniel |last9=Soto |first9=Maritza |last10=Csizmadia |first10=Szilard |last11=Chaushev |first11=Alexander |last12=Burleigh |first12=Matthew R. |last13=Alexander |first13=Richard |last14=Armstrong |first14=David J. |last15=Bouchy |first15=François |last16=Briegal |first16=Joshua T. |last17=Cabrera |first17=Juan |last18=Casewell |first18=Sarah L. |last19=Chazelas |first19=Bruno |last20=Cooke |first20=Benjamin F. |last21=Eigmüller |first21=Philipp |last22=Erikson |first22=Anders |last23=Gänsicke |first23=Boris T. |last24=Grange |first24=Andrew |last25=Günther |first25=Maximilian N. |last26=Hodgkin |first26=Simon T. |last27=Hooton |first27=Matthew J. |last28=Jenkins |first28=James S. |last29=Lambert |first29=Gregory |last30=Louden |first30=Tom |journal=Monthly Notices of the Royal Astronomical Society |volume=481 |issue=4 |pages=4960–4970 |doi-access=free |bibcode=2018MNRAS.481.4960R |display-authors=1 }}

{{cite journal |arxiv=1805.01378|doi=10.1093/mnras/sty1193 |title=Unmasking the hidden NGTS-3Ab: A hot Jupiter in an unresolved binary system |year=2018 |last1=Günther |first1=Maximilian N. |last2=Queloz |first2=Didier |last3=Gillen |first3=Edward |last4=Delrez |first4=Laetitia |last5=Bouchy |first5=François |last6=McCormac |first6=James |last7=Smalley |first7=Barry |last8=Almleaky |first8=Yaseen |last9=Armstrong |first9=David J. |last10=Bayliss |first10=Daniel |last11=Burdanov |first11=Artem |last12=Burleigh |first12=Matthew |last13=Cabrera |first13=Juan |last14=Casewell |first14=Sarah L. |last15=Cooke |first15=Benjamin F. |last16=Csizmadia |first16=Szilárd |last17=Ducrot |first17=Elsa |last18=Eigmüller |first18=Philipp |last19=Erikson |first19=Anders |last20=Gänsicke |first20=Boris T. |last21=Gibson |first21=Neale P. |last22=Gillon |first22=Michaël |last23=Goad |first23=Michael R. |last24=Jehin |first24=Emmanuël |last25=Jenkins |first25=James S. |last26=Louden |first26=Tom |last27=Moyano |first27=Maximiliano |last28=Murray |first28=Catriona |last29=Pollacco |first29=Don |last30=Poppenhaeger |first30=Katja |journal=Monthly Notices of the Royal Astronomical Society |volume=478 |issue=4 |pages=4720–4737 |doi-access=free |bibcode=2018MNRAS.478.4720G |display-authors=1 }}

{{cite journal |arxiv=1809.00678 |title=NGTS-4b: A sub-Neptune transiting in the desert|year=2019 |doi=10.1093/mnras/stz1084 |last1=West |first1=Richard G. |last2=Gillen |first2=Edward |last3=Bayliss |first3=Daniel |last4=Burleigh |first4=Matthew R. |last5=Delrez |first5=Laetitia |last6=Günther |first6=Maximilian N. |last7=Hodgkin |first7=Simon T. |last8=Jackman |first8=James A G. |last9=Jenkins |first9=James S. |last10=King |first10=George |last11=McCormac |first11=James |last12=Nielsen |first12=Louise D. |last13=Raynard |first13=Liam |last14=Smith |first14=Alexis M S. |last15=Soto |first15=Maritza |last16=Turner |first16=Oliver |last17=Wheatley |first17=Peter J. |last18=Almleaky |first18=Yaseen |last19=Armstrong |first19=David J. |last20=Belardi |first20=Claudia |last21=Bouchy |first21=François |last22=Briegal |first22=Joshua T. |last23=Burdanov |first23=Artem |last24=Cabrera |first24=Juan |last25=Casewell |first25=Sarah L. |last26=Chaushev |first26=Alexander |last27=Chazelas |first27=Bruno |last28=Chote |first28=Paul |last29=Cooke |first29=Benjamin F. |last30=Csizmadia |first30=Szilard |journal=Monthly Notices of the Royal Astronomical Society |volume=486 |issue=4 |pages=5094–5103 |doi-access=free |display-authors=1 }}

{{cite journal |arxiv=1905.02593|doi=10.1051/0004-6361/201935206 |title=NGTS-5b: A highly inflated planet offering insights into the sub-Jovian desert |year=2019 |last1=Eigmüller |first1=Philipp |last2=Chaushev |first2=Alexander |last3=Gillen |first3=Edward |last4=Smith |first4=Alexis |last5=Nielsen |first5=Louise D. |last6=Turner |first6=Oliver |last7=Csizmadia |first7=Szilard |last8=Smalley |first8=Barry |last9=Bayliss |first9=Daniel |last10=Belardi |first10=Claudia |last11=Bouchy |first11=François |last12=Burleigh |first12=Matthew R. |last13=Cabrera |first13=Juan |last14=Casewell |first14=Sarah L. |last15=Chazelas |first15=Bruno |last16=Cooke |first16=Benjamin F. |last17=Erikson |first17=Anders |last18=Gänsicke |first18=Boris T. |last19=Günther |first19=Maximilian N. |last20=Goad |first20=Michael R. |last21=Grange |first21=Andrew |last22=Jackman |first22=James A. G. |last23=Jenkins |first23=James S. |last24=McCormac |first24=James |last25=Moyano |first25=Maximiliano |last26=Pollacco |first26=Don |last27=Poppenhaeger |first27=Katja |last28=Queloz |first28=Didier |last29=Raynard |first29=Liam |last30=Rauer |first30=Heike |journal=Astronomy & Astrophysics |volume=625 |pages=A142 |bibcode=2019A&A...625A.142E |s2cid=146809360 |display-authors=1 }}

{{cite journal |arxiv=1904.07997|doi=10.1093/mnras/stz2349 |title=NGTS-6b: An ultrashort period hot-Jupiter orbiting an old K dwarf |year=2019 |last1=Vines |first1=Jose I. |last2=Jenkins |first2=James S. |last3=Acton |first3=Jack S. |last4=Briegal |first4=Joshua |last5=Bayliss |first5=Daniel |last6=Bouchy |first6=François |last7=Belardi |first7=Claudia |last8=Bryant |first8=Edward M. |last9=Burleigh |first9=Matthew R. |last10=Cabrera |first10=Juan |last11=Casewell |first11=Sarah L. |last12=Chaushev |first12=Alexander |last13=Cooke |first13=Benjamin F. |last14=Csizmadia |first14=Szilárd |last15=Eigmüller |first15=Philipp |last16=Erikson |first16=Anders |last17=Foxell |first17=Emma |last18=Gill |first18=Samuel |last19=Gillen |first19=Edward |last20=Goad |first20=Michael R. |last21=Jackman |first21=James A G. |last22=King |first22=George W. |last23=Louden |first23=Tom |last24=McCormac |first24=James |last25=Moyano |first25=Maximiliano |last26=Nielsen |first26=Louise D. |last27=Pollacco |first27=Don |last28=Queloz |first28=Didier |last29=Rauer |first29=Heike |last30=Raynard |first30=Liam |journal=Monthly Notices of the Royal Astronomical Society |volume=489 |issue=3 |pages=4125–4134 |doi-access=free |display-authors=1 }}

{{cite journal |arxiv=1906.08219|doi=10.1093/mnras/stz2496 |title=NGTS-7Ab: An ultrashort-period brown dwarf transiting a tidally locked and active M dwarf |year=2019 |last1=Jackman |first1=James A G. |last2=Wheatley |first2=Peter J. |last3=Bayliss |first3=Dan |last4=Gill |first4=Samuel |last5=Hodgkin |first5=Simon T. |last6=Burleigh |first6=Matthew R. |last7=Braker |first7=Ian P. |last8=Günther |first8=Maximilian N. |last9=Louden |first9=Tom |last10=Turner |first10=Oliver |last11=Anderson |first11=David R. |last12=Belardi |first12=Claudia |last13=Bouchy |first13=François |last14=Briegal |first14=Joshua T. |last15=Bryant |first15=Edward M. |last16=Cabrera |first16=Juan |last17=Casewell |first17=Sarah L. |last18=Chaushev |first18=Alexander |last19=Costes |first19=Jean C. |last20=Csizmadia |first20=Szilard |last21=Eigmüller |first21=Philipp |last22=Erikson |first22=Anders |last23=Gänsicke |first23=Boris T. |last24=Gillen |first24=Edward |last25=Goad |first25=Michael R. |last26=Jenkins |first26=James S. |last27=McCormac |first27=James |last28=Moyano |first28=Maximiliano |last29=Nielsen |first29=Louise D. |last30=Pollacco |first30=Don |journal=Monthly Notices of the Royal Astronomical Society |volume=489 |issue=4 |pages=5146–5164 |doi-access=free |display-authors=1 }}

{{cite journal |arxiv=1911.02814|doi=10.1093/mnras/stz3140 |title=NGTS-8b and NGTS-9b: Two non-inflated hot-Jupiters |year=2019 |last1=Costes |first1=Jean C. |last2=Watson |first2=Christopher A. |last3=Belardi |first3=Claudia |last4=Braker |first4=Ian P. |last5=Burleigh |first5=Matthew R. |last6=Casewell |first6=Sarah L. |last7=Eigmüller |first7=Philipp |last8=Günther |first8=Maximilian N. |last9=Jackman |first9=James A G. |last10=Nielsen |first10=Louise D. |last11=Soto |first11=Maritza G. |last12=Turner |first12=Oliver |last13=Anderson |first13=David R. |last14=Bayliss |first14=Daniel |last15=Bouchy |first15=François |last16=Briegal |first16=Joshua T. |last17=Bryant |first17=Edward M. |last18=Cabrera |first18=Juan |last19=Chaushev |first19=Alexander |last20=Csizmadia |first20=Szilard |last21=Erikson |first21=Anders |last22=Gill |first22=Samuel |last23=Gillen |first23=Edward |last24=Goad |first24=Michael R. |last25=Hodgkin |first25=Simon |last26=Hooton |first26=Matthew J. |last27=Jenkins |first27=James S. |last28=McCormac |first28=James |last29=Moyano |first29=Maximiliano |last30=Queloz |first30=Didier |journal=Monthly Notices of the Royal Astronomical Society |doi-access=free |display-authors=1 }}

{{cite journal |arxiv=1909.12424|doi=10.1093/mnras/staa115 |title=NGTS-10b: The shortest period hot Jupiter yet discovered |year=2020 |last1=West |first1=Richard G. |last2=Watson |first2=Christopher A. |last3=Walker |first3=Simon R. |last4=Vines |first4=Jose I. |last5=Udry |first5=Stéphane |last6=Turner |first6=Oliver |last7=Soto |first7=Maritza |last8=Smalley |first8=Barry |last9=Smith |first9=Alexis M S. |last10=Raynard |first10=Liam |last11=Rauer |first11=Heike |last12=Queloz |first12=Didier |last13=Pollacco |first13=Don |last14=Nielsen |first14=Louise D. |last15=Moyano |first15=Maximiliano |last16=Louden |first16=Tom |last17=Longstaff |first17=Emma |last18=Lendl |first18=Monika |last19=Lambert |first19=Gregory |last20=Jenkins |first20=James S. |last21=Hooton |first21=Matthew J. |last22=Hodgkin |first22=Simon T. |last23=Günther |first23=Maximilian N. |last24=Goad |first24=Michael R. |last25=Gänsicke |first25=Boris T. |last26=Foxell |first26=Emma |last27=Erikson |first27=Anders |last28=Eigmüller |first28=Philipp |last29=Csizmadia |first29=Szilárd |last30=Costes |first30=Jean C. |journal=Monthly Notices of the Royal Astronomical Society |volume=493 |pages=126–140 |doi-access=free |display-authors=1 }}

{{cite journal |arxiv=2005.00006|doi=10.3847/2041-8213/ab9eb9 |title=NGTS-11 b (TOI-1847 b): A Transiting Warm Saturn Recovered from a TESS Single-transit Event |year=2020 |last1=Gill |first1=Samuel |last2=Wheatley |first2=Peter J. |last3=Cooke |first3=Benjamin F. |last4=Jordán |first4=Andrés |last5=Nielsen |first5=Louise D. |last6=Bayliss |first6=Daniel |last7=Anderson |first7=David R. |last8=Vines |first8=Jose I. |last9=Lendl |first9=Monika |last10=Acton |first10=Jack S. |last11=Armstrong |first11=David J. |last12=Bouchy |first12=François |last13=Brahm |first13=Rafael |last14=Bryant |first14=Edward M. |last15=Burleigh |first15=Matthew R. |last16=Casewell |first16=Sarah L. |last17=Eigmüller |first17=Philipp |last18=Espinoza |first18=Néstor |last19=Gillen |first19=Edward |last20=r. Goad |first20=Michael |last21=Grieves |first21=Nolan |last22=Günther |first22=Maximilian N. |last23=Henning |first23=Thomas |last24=Hobson |first24=Melissa J. |last25=Hogan |first25=Aleisha |last26=Jenkins |first26=James S. |last27=McCormac |first27=James |last28=Moyano |first28=Maximiliano |last29=Osborn |first29=Hugh P. |last30=Pollacco |first30=Don |journal=The Astrophysical Journal Letters |volume=898 |issue=1 |pages=L11 |s2cid=220845943 |display-authors=1 |doi-access=free |bibcode=2020ApJ...898L..11G }}

{{cite journal |arxiv=2009.10620|doi=10.1093/mnras/staa2976 |title=NGTS-12b: A sub-Saturn mass transiting exoplanet in a 7.53 day orbit |year=2020 |last1=Bryant |first1=Edward M. |last2=Bayliss |first2=Daniel |last3=Nielsen |first3=Louise D. |last4=Veras |first4=Dimitri |last5=Acton |first5=Jack S. |last6=Anderson |first6=David R. |last7=Armstrong |first7=David J. |last8=Bouchy |first8=François |last9=Briegal |first9=Joshua T. |last10=Burleigh |first10=Matthew R. |last11=Cabrera |first11=Juan |last12=Casewell |first12=Sarah L. |last13=Chaushev |first13=Alexander |last14=Cooke |first14=Benjamin F. |last15=Csizmadia |first15=Szilárd |last16=Eigmüller |first16=Philipp |last17=Erikson |first17=Anders |last18=Gill |first18=Samuel |last19=Gillen |first19=Edward |last20=Goad |first20=Michael R. |last21=Grieves |first21=Nolan |last22=Günther |first22=Maximilian N. |last23=Henderson |first23=Beth |last24=Hogan |first24=Aleisha |last25=Jenkins |first25=James S. |last26=Lendl |first26=Monika |last27=McCormac |first27=James |last28=Moyano |first28=Maximiliano |last29=Queloz |first29=Didier |last30=Rauer |first30=Heike |journal=Monthly Notices of the Royal Astronomical Society |volume=499 |issue=3 |pages=3139–3148 |doi-access=free |display-authors=1 }}

{{cite journal |arxiv=2101.04245|doi=10.1051/0004-6361/202039586 |title=NGTS-13b: A hot 4.8 Jupiter-mass planet transiting a subgiant star |year=2021 |last1=Grieves |first1=Nolan |last2=Nielsen |first2=Louise D. |last3=Vines |first3=Jose I. |last4=Bryant |first4=Edward M. |last5=Gill |first5=Samuel |last6=Bouchy |first6=François |last7=Lendl |first7=Monika |last8=Bayliss |first8=Daniel |last9=Eigmueller |first9=Philipp |last10=Segransan |first10=Damien |last11=Acton |first11=Jack S. |last12=Anderson |first12=David R. |last13=Burleigh |first13=Matthew R. |last14=Casewell |first14=Sarah L. |last15=Chaushev |first15=Alexander |last16=Cooke |first16=Benjamin F. |last17=Gillen |first17=Edward |last18=Goad |first18=Michael R. |last19=Günther |first19=Maximilian N. |last20=Henderson |first20=Beth A. |last21=Hogan |first21=Aleisha |last22=Jenkins |first22=James S. |last23=Alves |first23=Douglas R. |last24=Jordán |first24=Andrés |last25=McCormac |first25=James |last26=Moyano |first26=Maximiliano |last27=Queloz |first27=Didier |last28=Raynard |first28=Liam |last29=Seidel |first29=Julia V. |last30=Smith |first30=Alexis M. S. |journal=Astronomy & Astrophysics |volume=647 |pages=A180 |bibcode=2021A&A...647A.180G |s2cid=231582818 |display-authors=1 }}

{{cite journal |arxiv=2101.01470|doi=10.1051/0004-6361/202039712 |title=NGTS-14Ab: A Neptune-sized transiting planet in the desert |year=2021 |last1=Smith |first1=A. M. S. |last2=Acton |first2=J. S. |last3=Anderson |first3=D. R. |last4=Armstrong |first4=D. J. |last5=Bayliss |first5=D. |last6=Belardi |first6=C. |last7=Bouchy |first7=F. |last8=Brahm |first8=R. |last9=Briegal |first9=J. T. |last10=Bryant |first10=E. M. |last11=Burleigh |first11=M. R. |last12=Cabrera |first12=J. |last13=Chaushev |first13=A. |last14=Cooke |first14=B. F. |last15=Costes |first15=J. C. |last16=Csizmadia |first16=Sz. |last17=Eigmüller |first17=Ph. |last18=Erikson |first18=A. |last19=Gill |first19=S. |last20=Gillen |first20=E. |last21=Goad |first21=M. R. |last22=Günther |first22=M. N. |last23=Henderson |first23=B. A. |last24=Hogan |first24=A. |last25=Jordán |first25=A. |last26=Lendl |first26=M. |last27=McCormac |first27=J. |last28=Moyano |first28=M. |last29=Nielsen |first29=L. D. |last30=Rauer |first30=H. |journal=Astronomy & Astrophysics |volume=646 |pages=A183 |bibcode=2021A&A...646A.183S |s2cid=230524042 |display-authors=1 }}

{{cite journal |arxiv=2103.10302|doi=10.1093/mnras/stab815 |title=NGTS 15b, 16b, 17b, and 18b: Four hot Jupiters from the Next-Generation Transit Survey |year=2021 |last1=Tilbrook |first1=Rosanna H. |last2=Burleigh |first2=Matthew R. |last3=Costes |first3=Jean C. |last4=Gill |first4=Samuel |last5=Nielsen |first5=Louise D. |last6=Vines |first6=José I. |last7=Queloz |first7=Didier |last8=Hodgkin |first8=Simon T. |last9=Worters |first9=Hannah L. |last10=Goad |first10=Michael R. |last11=Acton |first11=Jack S. |last12=Henderson |first12=Beth A. |last13=Armstrong |first13=David J. |last14=Anderson |first14=David R. |last15=Bayliss |first15=Daniel |last16=Bouchy |first16=François |last17=Briegal |first17=Joshua T. |last18=Bryant |first18=Edward M. |last19=Casewell |first19=Sarah L. |last20=Chaushev |first20=Alexander |last21=Cooke |first21=Benjamin F. |last22=Eigmüller |first22=Philipp |last23=Gillen |first23=Edward |last24=Günther |first24=Maximilian N. |last25=Hogan |first25=Aleisha |last26=Jenkins |first26=James S. |last27=Lendl |first27=Monika |last28=McCormac |first28=James |last29=Moyano |first29=Maximiliano |last30=Raynard |first30=Liam |journal=Monthly Notices of the Royal Astronomical Society |volume=504 |issue=4 |pages=6018–6032 |doi-access=free |display-authors=1 }}

{{cite journal |arxiv=2105.08574|doi=10.1093/mnras/stab1459 |title=NGTS-19b: A high-mass transiting brown dwarf in a 17-d eccentric orbit |year=2021 |last1=Acton |first1=Jack S. |last2=Goad |first2=Michael R. |last3=Burleigh |first3=Matthew R. |last4=Casewell |first4=Sarah L. |last5=Breytenbach |first5=Hannes |last6=Nielsen |first6=Louise D. |last7=Smith |first7=Gareth |last8=Anderson |first8=David R. |last9=Battley |first9=Matthew P. |last10=Bayliss |first10=Daniel |last11=Bouchy |first11=François |last12=Bryant |first12=Edward M. |last13=Csizmadia |first13=Szilárd |last14=Eigmüller |first14=Philipp |last15=Gill |first15=Samuel |last16=Gillen |first16=Edward |last17=Grieves |first17=Nolan |last18=Günther |first18=Maximilian N. |last19=Henderson |first19=Beth A. |last20=Hodgkin |first20=Simon T. |last21=Jackman |first21=James A G. |last22=Jenkins |first22=James S. |last23=Lendl |first23=Monika |last24=McCormac |first24=James |last25=Moyano |first25=Maximiliano |last26=Nelson |first26=Richard P. |last27=Sefako |first27=Ramotholo R. |last28=Smith |first28=Alexis M S. |last29=Stalport |first29=Manu |last30=Thomas |first30=Jessymol K. |journal=Monthly Notices of the Royal Astronomical Society |volume=505 |issue=2 |pages=2741–2752 |doi-access=free |display-authors=1 }}

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

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

{{cite journal |arxiv=1812.07668|doi=10.3847/1538-3881/ab26bb |title=HATS-54b–HATS-58Ab: Five New Transiting Hot Jupiters Including One with a Possible Temperate Companion |year=2019 |last1=Espinoza |first1=N. |last2=Hartman |first2=J. D. |last3=Bakos |first3=G. Á. |last4=Henning |first4=T. |last5=Bayliss |first5=D. |last6=Bento |first6=J. |last7=Bhatti |first7=W. |last8=Brahm |first8=R. |last9=Csubry |first9=Z. |last10=Suc |first10=V. |last11=Jordán |first11=A. |last12=Mancini |first12=L. |last13=Tan |first13=T. G. |last14=Penev |first14=K. |last15=Rabus |first15=M. |last16=Sarkis |first16=P. |last17=De Val-Borro |first17=M. |last18=Durkan |first18=S. |last19=Lázár |first19=J. |last20=Papp |first20=I. |last21=Sári |first21=P. |journal=The Astronomical Journal |volume=158 |issue=2 |page=63 |s2cid=119409621 |doi-access=free |bibcode=2019AJ....158...63E }}

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

{{cite journal | last=Ivshina | first=Ekaterina S. | last2=Winn | first2=Joshua N. | title=TESS Transit Timing of Hundreds of Hot Jupiters | journal=The Astrophysical Journal Supplement Series | volume=259 | issue=2 | date=2022-04-01 | issn=0067-0049 | doi=10.3847/1538-4365/ac545b | doi-access=free | page=62}}

{{cite journal | last=Bouchy | first=F. | last2=Gillen | first2=E. | last3=Turner | first3=O. | last4=Gill | first4=S. | last5=Nielsen | first5=L. D. | last6=Lendl | first6=M. | last7=Vines | first7=J. I. | last8=Alves | first8=D. R. | last9=Anderson | first9=D. R. | last10=Armstrong | first10=D. J. | last11=Bayliss | first11=D. | last12=Jenkins | first12=J. S. | last13=Acton | first13=J. S. | last14=Belardi | first14=C. | last15=Bryant | first15=E. M. | last16=Burleigh | first16=M. R. | last17=Casewell | first17=S. L. | last18=Costes | first18=J. C. | last19=Chaushev | first19=A. | last20=Cooke | first20=B. F. | last21=Eigmüller | first21=Ph. | last22=Erikson | first22=A. | last23=Günther | first23=M. N. | last24=Goad | first24=M. R. | last25=Grieves | first25=N. | last26=McCormac | first26=J. | last27=Moyano | first27=M. | last28=Raynard | first28=L. | last29=Smith | first29=A. M. S. | last30=Tilbrook | first30=R. H. | last31=Udry | first31=S. | last32=Watson | first32=C. A. | last33=West | first33=R. G. | last34=Wheatley | first34=P. J. | title=NGTS discovery of a highly inflated Saturn-mass planet and a highly irradiated hot Jupiter: NGTS-26 b and NGTS-27 b | journal=Astronomy & Astrophysics | volume=684 | date=2024 | issn=0004-6361 | doi=10.1051/0004-6361/202347162 | doi-access=free | page=A201}}

{{cite journal | last=Henderson | first=Beth A | last2=Casewell | first2=Sarah L | last3=Goad | first3=Michael R | last4=Acton | first4=Jack S | last5=Günther | first5=Maximilian N | last6=Nielsen | first6=Louise D | last7=Burleigh | first7=Matthew R | last8=Belardi | first8=Claudia | last9=Tilbrook | first9=Rosanna H | last10=Turner | first10=Oliver | last11=Howell | first11=Steve B | last12=Clark | first12=Catherine A | last13=Littlefield | first13=Colin | last14=Barkaoui | first14=Khalid | last15=Alves | first15=Douglas R | last16=Anderson | first16=David R | last17=Bayliss | first17=Daniel | last18=Bouchy | first18=Francois | last19=Bryant | first19=Edward M | last20=Dransfield | first20=George | last21=Ducrot | first21=Elsa | last22=Eigmüller | first22=Philipp | last23=Gill | first23=Samuel | last24=Gillen | first24=Edward | last25=Gillon | first25=Michaël | last26=Hawthorn | first26=Faith | last27=Hooton | first27=Matthew J | last28=Jackman | first28=James A G | last29=Jehin | first29=Emmanuel | last30=Jenkins | first30=James S | last31=Kendall | first31=Alicia | last32=Lendl | first32=Monika | last33=McCormac | first33=James | last34=Moyano | first34=Maximiliano | last35=Pedersen | first35=Peter Pihlmann | last36=Pozuelos | first36=Francisco J | last37=Ramsay | first37=Gavin | last38=Sefako | first38=Ramotholo R | last39=Timmermans | first39=Mathilde | last40=Triaud | first40=Amaury H M J | last41=Udry | first41=Stephane | last42=Vines | first42=Jose I | last43=Watson | first43=Christopher A | last44=West | first44=Richard G | last45=Wheatley | first45=Peter J | last46=Zúñiga-Fernández | first46=Sebastián | title=NGTS-28Ab: a short period transiting brown dwarf | journal=Monthly Notices of the Royal Astronomical Society | volume=530 | issue=1 | date=2024-04-05 | issn=0035-8711 | doi=10.1093/mnras/stae508 | doi-access=free | pages=318–339 | url=https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stae508/56732879/stae508.pdf | access-date=2025-05-21}}

}}

External links

{{Official website|http://www.ngtransits.org}}
{{Commons category inline}}
[https://www.eso.org/sci/publications/messenger/archive/no.165-sep16/messenger-no165-10-12.pdf The Next Generation Transit Survey Becomes Operational at Paranal], ESO archive, The Messenger 165 – September 2016

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