TEPCat: Orbital obliquity observations for transiting planetary systems

This table catalogues measurements of orbital obliquity for the known (published) transiting extrasolar planetary systems. This effect is normally observed spectroscopically (usually via radial velocity measurements) but can be obtained photometrically, by analysis of starspot crossing events during transits.

The radial-velocity anomaly known as the Rossiter-McLaughlin effect was originally predicted by Holt (1893) and observed (but not definitively) in the eclipsing binary star systems δ Librae (Schlesinger 1910) and λ Tauri (Schlesinger 1916). It was subsequently described and clearly demonstrated by Rossiter (1924) for β Lyrae and McLaughlin (1924) for β Persei. The designation "Rossiter-McLaughlin effect" arose from the latter two papers.

All known orbital obliquity constraints are included. Many systems have multiple measurements, often resulting from the same data. In these cases the most recent is normally the most reliable but it is important to check the published papers to be sure. I indicate the preferred value for each object using the "Pflag" column in the ASCII and CSV files (not in the HTML table below). Pflag is set to "y" for the best value for a given object, and to "n" for all other values for this object.

The quantity most commonly observed is the sky-projected angle between the axes of the stellar rotation and the planetary orbit. This quantity is normally called the sky-projected obliquity and denoted λ. There is an alternative definition of the co-ordinate system which yields the value β instead. The two quantities are related by λ = -β i.e. one is the negative value of the other.

The orbital obliquity is more difficult to determine than the sky-projected orbital obliquity, and only a few measurements exist. This quantity is called ψ and it is always closer to 90 degrees than λ:
ψ ≥ |λ| for λ < 90 degrees
ψ ≤ |λ| for λ > 90 degrees
This means that objects with a constraint on λ also have a constraint on ψ, but this is often not given explicitly.

Click here for details of the quantities and their units
Click here for the table in machine-readable ASCII format
Click here for the table in machine-readable CSV format
Click here to return to the TEPCat main page

System	Teff (K)	λ (degrees)	ψ (degrees)	Reference
55 Cnc e	5172 ± 18	72.4 + 12.7 - 11.5 indeterminate 10 + 17 - 20	23 + 14 - 12	Bourrier & Hébrard (2014) López-Morales et al. (2014) Zhao et al. (2023)
AU Mic b	3540 + 120 − 110	−4.7 + 6.8 - 6.4 −0.1 + 5.1 - 5.0 −3.0 + 10.4 - 10.3 5 + 16 - 15		Hirano et al. (2020) Martioli et al. (2021) Palle et al. (2020) Addison et al. (2021)
CoRoT-1	5950 ± 150	77 ± 11		Pont et al. (2010)
CoRoT-2	5598 ± 50	7.2 ± 4.5 4.7 ± 12.3 −1.0 + 6.0 - 7.7 4.0 + 5.9 - 6.1		Bouchy et al. (2008) Nutzmann et al. (2011) Czesla et al. (2012) Gillon et al. (2010)
CoRoT-3	6558 ± 44	−37.6 + 22.3 - 10.0		Triaud et al. (2009)
CoRoT-11	6343 ± 72	prograde 0.1 ± 2.6		Gandolfi et al. (2010) Gandolfi et al. (2012)
CoRoT-18	5440 ± 100	−10 ± 20	20 ± 20	Hébrard et al. (2011)
CoRoT-19	6090 ± 70	−52 + 27 - 22		Guenther et al. (2012)
CoRoT-36	6730 ± 140	275.8 ± 11.3		Sebastian et al. (2022)
DS Tuc	5598 + 28 − 59	2.93 + 0.88 - 0.87 12.1 + 2.6 - 2.1		Zhou et al. (2020) Benatti et al. (2021)
GJ 436	3416 ± 54	72 + 33 - 24 114 + 23 - 17	80 + 21 - 18 103 + 13 - 12	Bourrier et al. (2018) Bourrier et al. (2022)
GJ 3470	3725 ± 54	101 + 29 - 14	97 + 16 - 11	Stefánsson et al. (2022)
GPX-1	7000 ± 200	6.8 ± 1.7		Giacalone et al. (2024)
HAT-P-1	5975 ± 50	3.7 ± 2.1		Johnson et al. (2008)
HAT-P-2	6290 ± 60	1.2 ± 13.4 0.2 + 12.2 - 12.5 9 ± 10		Winn et al. (2007) Loeillet et al. (2008) Albrecht et al. (2012)
HAT-P-3	5190 ± 80	21.2 ± 8.7 −25.3 + 29.4 - 22.8	75.7 + 8.5 - 7.9	Mancini et al. (2018) Bourrier et al. (2023)
HAT-P-4	6036 ± 46	−4.9 ± 11.9		Winn et al. (2011)
HAT-P-6	6570 ± 80	166 ± 10 165 ± 6		Hébrard et al. (2011) Albrecht et al. (2012)
HAT-P-7	6310 ± 15	182.5 ± 9.4 −132.6 + 10.5 - 16.3 155 ± 37 220.3 + 8.2 - 9.3 142 + 12 - 16 136 + 16 - 22	94.6 + 5.5 - 3.0 115 + 19 - 16 97 ± 14 101 ± 2 87 ± 2 116.4 + 30.2 - 14.7	Winn et al. (2009) Narita et al. (2009) Albrecht et al. (2012) Benomar et al. (2014) Lund et al. (2014) Masuda (2015) solution 1 Masuda (2015) solution 2 Campante et al. (2016)
HAT-P-8	6200 ± 80	−9.7 + 9.0 - 7.7 −17 + 9.2 - 11.5		Simpson et al. (2011) Moutou et al. (2011)
HAT-P-9	6350 ± 150	−16 ± 8		Moutou et al. (2011)
HAT-P-11	4780 ± 50	103 + 26 - 10 103 + 22 - 18 106 + 15 - 12 121 + 24 - 21 almost polar orbit 133.9 + 7.1 - 8.3	106 + 15 - 11 97 + 8 - 4 104.9 + 8.6 - 9.1	Winn et al. (2010) Hirano et al. (2011) Sanchis-Ojeda et al. (2011) solution 1 Sanchis-Ojeda et al. (2011) solution 2 Deming et al. (2011) Bourrier et al. (2023)
HAT-P-12	4665 ± 45	−54 + 41 - 13		Mancini et al. (2018)
HAT-P-13	5653 ± 90	1.9 ± 8.6		Winn et al. (2010)
HAT-P-14	6600 ± 90	189.1 ± 5.1		Winn et al. (2011)
HAT-P-15	5620 ± 20	13 ± 6		Mancini et al. (2022)
HAT-P-16	6140 ± 72	−10 ± 16 −2 + 55 - 46		Moutou et al. (2011) Albrecht et al. (2012)
HAT-P-17	5350 ± 20	19 + 14 - 16 −27.5 ± 6.7		Fulton et al. (2013) Mancini et al. (2022)
HAT-P-18	4870 ± 50	132 ± 15		Esposito et al. (2014)
HAT-P-20	4595 ± 45	−8.0 ± 6.9	36 + 10 - 12	Esposito et al. (2017)
HAT-P-21	5695 ± 45	−0.7 ± 12.5		Mancini et al. (2022)
HAT-P-22	5314 ± 50	−2.1 ± 3.0	24 ± 18	Mancini et al. (2018)
HAT-P-23	5885 ± 72	15 ± 22		Moutou et al. (2011)
HAT-P-24	6373 ± 80	20 ± 16		Albrecht et al. (2012)
HAT-P-27	5316 ± 55	24.2 + 76.0 - 44.5		Brown et al. (2012)
HAT-P-29	6140 ± 30	−26 ± 16		Mancini et al. (2022)
HAT-P-30	6338 ± 42	73.5 ± 9.0 70.5 + 2.9 - 2.8		Johnson et al. (2011) Cegla et al. (2023)
HAT-P-32	6269 ± 64	85 ± 1.5		Albrecht et al. (2012)
HAT-P-33	6446 ± 88	−5.9 ± 4.1		Bourrier et al. (2023)
HAT-P-34	6442 ± 88	0 ± 14		Albrecht et al. (2012)
HAT-P-36	5620 ± 40	−14 ± 18	0 + 63 - 0	Mancini et al. (2015)
HAT-P-41	6390 ± 100	−22.1 + 0.8 - 6.0		Johnson et al. (2017)
HAT-P-49	6820 ± 52	−97.7 ± 1.8		Bourrier et al. (2023)
HAT-P-56	6566 ± 50	8 ± 2		Zhou et al. (2016)
HAT-P-67	6406 + 65 − 61	2.2 ± 0.4		Sicilia et al. (2024)
HAT-P-69	7724 + 250 − 360	30.3 + 6.1 - 7.3		Zhou et al. (2019)
HAT-P-70	8450 ± 195	113.1 + 5.1 - 3.4 107.9 + 2.0 - 1.7		Zhou et al. (2019) Bello-Arufe et al. (2022)
HATS-2	5227 ± 95	8 ± 8 3 ± 18	38 ± 27	Mohler-Fischer et al. (2013) Biagiotti et al. (2024)
HATS-3	6351 ± 76	3 ± 25		Addison et al. (2014)
HATS-14	5346 ± 60	76 + 4 - 5		Zhou et al. (2015)
HATS-38	5662 ± 80	−108 + 11 - 16		Espinoza-Retamal et al. (2024)
HATS-70	7930 ± 180	8.9 + 5.6 - 4.5		Zhou et al. (2019)
HD 3167b	5300 ± 73	−6.6 + 6.6 - 7.9	29.5 + 7.2 - 9.4	Bourrier et al. (2021)
HD 3167c	5300 ± 73	−98 ± 23 −108.9 + 5.4 - 5.5	107.7 + 5.1 - 4.9	Dalal et al. (2019) Bourrier et al. (2021)
HD 17156	6046 + 76 − 72	62 ± 25 9.4 ± 9.3 −4.8 ± 5.3 10.0 ± 5.1		Narita et al. (2008) Cochran et al. (2008) Barbieri et al. (2009) Narita et al. (2009)
HD 63433b	5700 + 76 − 75	8.0 + 33.0 - 45.0		Mann et al. (2020)
HD 80606	5584 ± 13	prograde 50 + 61 - 36 53 + 34 - 21 42 ± 8		Moutou et al. (2009) Pont et al. (2009) Winn et al. (2009) Hébrard et al. (2010)
HD 106315c	6364 ± 87	−10.9 + 3.6 - 3.8 −2.7 + 2.7 - 2.6		Zhou et al. (2018) Bourrier et al. (2023)
HD 110067c	5266 ± 64	6 + 24 - 26		Zak et al. (2024)
HD 118203	5788 ± 51	−12 + 8 - 10	0 + 33.5 - 0	Zhang et al. (2024)
HD 149026	6147 ± 50	−12 ± 15 12 ± 7		Wolf et al. (2007) Albrecht et al. (2012)
HD 189733	4969 ± 43	−1.4 ± 1.1 0.85 + 0.28 - 0.32 −0.50 ± 0.30 −0.4 ± 0.2 −0.31 + 0.18 - 0.17 −1.00 + 0.22 - 0.23	4 + 18 - 4 7 + 12 - 4 13.6 ± 6.9	Winn et al. (2006) Triaud et al. (2009) Collier Cameron et al. (2010) Dumusque (2014) Cegla et al. (2016) Casasayas-Barris et al. (2017) Cristo et al. (2023)
HD 191939b	5427 ± 50	3.7 ± 5.0		Lubin et al. (2024)
HD 209458	6117 ± 50	3.9 + 18 - 21 −4.4 ± 1.4 −5 ± 7 0.6 ± 0.4 1.58 ± 0.08		Queloz et al. (2000) Winn et al. (2005) Albrecht et al. (2012) Santos et al. (2020) Casasayas-Barris et al. (2021)
HD 332231	6089 + 97 − 96	−42 ± 11 −2 ± 6		Sedaghati et al. (2022) Knudstrup & Albrecht (2022)
HIP 67522b	5675 ± 75	−5.8 + 2.8 - 5.7	20.2 + 10.3 - 8.7	Heitzmann et al. (2021)
K2-25b	3207 ± 58	1.7 + 5.8 - 3.7 3 ± 16	17 + 11 - 8	Gaidos et al. (2020) Stefansson et al. (2020)
K2-29	5358 ± 38	1.5 ± 8.7		Santerne et al. (2016)
K2-33	3540 ± 70	−10 + 22 - 24		Hirano et al. (2024)
K2-34	6131 ± 47	−1 + 10 - 9		Hirano et al. (2016)
K2-93d	6320 + 60 − 30	57 + 26 - 18		Grouffal et al. (2022)
K2-105	5430 ± 70	−81 + 50 - 47		Bourrier et al. (2023)
K2-139	5245 + 73 − 33	−17 ± 7		Prinoth et al. (2024)
K2-140	5654 ± 55	0.5 ± 9.7		Rice et al. (2021)
K2-232	6154 ± 60	−11.1 ± 6.6		Wang et al. (2021)
K2-234	5622 + 70 − 71	74 + 34 - 33	80 + 22 - 23	Bourrier et al. (2023)
K2-267	6189 + 47 − 52	−1.48 ± 0.85	3.4 + 3.5 - 1.6	Yu et al. (2018)
K2-290b	6302 ± 120	173 + 45 - 53		Hjorth et al.(2021)
K2-290c	6302 ± 120	153 ± 8	124 ± 6	Hjorth et al.(2021)
K2-329	5282 + 40 − 39	24 + 13 - 9		Prinoth et al. (2024)
KELT-1	6471 + 50 − 49	2 ± 16		Siverd et al. (2012)
KELT-6	6246 ± 88	−36 ± 11		Damasso et al. (2015)
KELT-7	6699 ± 24	9.7 ± 5.2 2.7 ± 0.6 −10.55 ± 0.27	12.4 ± 11.7	Bieryla et al. (2015) Zhou et al. (2016) Tabernero et al. (2022)
KELT-9	9329 ± 118	−84.8 ± 1.4 −85.78 ± 0.46 −85.01 ± 0.23 −88 ± 15 −84.8 ± 0.3	87 + 10 - 11 87.47 + 0.18 - 0.19	Gaudi et al. (2017) Borsa et al. (2019) Wyttenbach et al. (2020) Ahlers et al. (2020) Stephen et al. (2022)
KELT-10	5948 ± 74	−5.2 ± 3.4		Steiner et al. (2023)
KELT-11	5375 ± 25	−77.9 + 2.4 - 2.3		Mounzer et al. (2022)
KELT-17	7454 ± 49	−115.9 ± 4.1	116 ± 4	Zhou et al. (2016)
KELT-18	6670 ± 120	−94.8 ± 0.7	91.7 + 2.2 - 1.8	Rubenzahl et al. (2024)
KELT-19	7500 ± 110	−179.7 + 3.7 - 3.8 −179.7 + 3.7 - 3.8	155 + 17 - 21	Siverd et al. (2018) Kawai et al. (2024)
KELT-20	8652 ± 160	3.4 ± 2.1 0.6 ± 4 1.6 ± 3.1 3.9 ± 1.1	5 ± 11	Lund et al. (2017) Talens et al. (2018) Hoeijmakers et al. (2020) Singh et al. (2024)
KELT-21	7598 + 81 − 84	−5.6 + 1.7 - 1.9		Johnson et al. (2018)
KELT-24	6426 + 91 − 93	2.6 + 5.1 - 3.6 1.2 + 8.2 - 7.4 1.4 + 4.9 - 4.7		Rodriguez et al. (2019) Hjorth et al. (2019) Giovinazzi et al. (2024)
Kepler-8	6213 ± 150	−26.4 ± 10.1 5 ± 7		Jenkins et al. (2010) Albrecht et al. (2012)
Kepler-9b	5774 ± 60	−13 ± 16		Wang et al. (2018)
Kepler-13	7650 ± 250	23 ± 4 58.6 ± 2 58.6 ± 2 59.20 ± 0.05 −27.9 ± 1.1	60 ± 2 60.25 ± 0.05	Barnes et al. (2011) Johnson et al. (2014) Masuda (2015) Howarth & Morello (2017) Herman et al. (2018)
Kepler-17	5781 ± 85	0 ± 15	0 ± 15	Désert et al. (2011)
Kepler-25c	6270 ± 79	−0.5 ± 5.7 9.4 ± 7.1 −0.9 + 7.7 - 6.4	26.9 + 7.0 - 9.2 12.6 + 6.7 - 11.0 24.1 + 9.29 - 9.3	Albrecht et al. (2013) Benomar et al. (2014) Campante et al. (2016) Bourrier et al. (2023)
Kepler-30b	5498 ± 54	4 ± 10 −1 ± 10		Sanchis-Ojeda et al. (2012) method 1 Sanchis-Ojeda et al. (2012) method 2
Kepler-50b	6225 ± 66	aligned		Chaplin et al. (2013)
Kepler-50c	6225 ± 66	aligned		Chaplin et al. (2013)
Kepler-56b	4840 ± 97	misaligned		Huber et al.(2013)
Kepler-56c	4840 ± 97	misaligned		Huber et al.(2013)
Kepler-63	5576 ± 50	−110 + 22 - 14 −135 + 21 - 27	104 + 9 - 14 115 + 17 - 13	Sanchis-Ojeda et al. (2013) Bourrier et al. (2023)
Kepler-65b	6211 ± 66	aligned		Chaplin et al. (2013)
Kepler-65c	6211 ± 66	aligned		Chaplin et al. (2013)
Kepler-65d	6211 ± 66	aligned		Chaplin et al. (2013)
Kepler-89d	6182 ± 82	−6 + 13 - 11 −11 ± 11		Hirano et al. (2012) Albrecht et al. (2013)
Kepler-1656	5731 ± 60	35 + 15 - 22		Rubenzahl et al. (2024)
Kepler-408	6088 ± 65		48 + 4 - 5	Kamiaka et al. (2019)
Kepler-420	5520 ± 80	74 + 32 - 46		Santerne et al. (2014)
Kepler-448	6820 ± 120	12.6 + 3.0 - 2.9 −7.1 + 4.2 - 2.8		Bourrier et al. (2015) Johnson et al. (2017)
MASCARA-1	7554 ± 150	69.5 ± 3 69.2 + 3.1 - 3.4	72.1 + 2.5 - 2.4	Talens et al. (2017) Hooton et al. (2022)
MASCARA-4	7810 ± 165	247.5 + 1.5 - 1.7 244 ± 15 250.34 ± 0.14	104 + 7 - 13	Dorval et al. (2020) Ahlers et al. (2020) Zhang et al. (2022)
NGTS-2	6450 ± 50	−11.3 ± 4.8		Anderson et al. (2018)
Qatar-1	4820 ± 85	−8.4 ± 7.1		Covino et al. (2013)
Qatar-2	4645 ± 50	4.3 ± 4.5 0 ± 8 0 ± 10 15 ± 20	0 + 43 - 0	Mancini et al. (2014) Mocnik et al. (2017) Dai et al. (2017) Esposito et al. (2017)
Qatar-6	5063 ± 42	0.1 ± 2.6	22 + 9 - 18	Rice et al. (2023)
TIC 241249530	6150 ± 50	163.5 + 9.4 - 7.7		Gupta et al. (2024)
TOI-1136d	5770 ± 50	5 ± 5	0 + 28 - 0	Dai et al. (2023)
TOI-1181	5990 ± 95	−2 + 16 - 15		Saunders et al.(2024)
TOI-1268	5257 ± 40	40.0 + 7.2 - 9.9		Dong et al. (2022)
TOI-1431	7690 + 400 − 250	−155 + 20 - 10		Stangret et al. (2021)
TOI-1478	5597 + 83 − 82	6.2 + 5.9 - 5.5		Rice et al. (2022)
TOI-1518	7300 ± 100	240.34 + 0.93 - 0.98 −118.96 + 0.68 - 0.65 −117.24 + 0.64 - 0.69		Cabot et al. (2021) Watanabe et al. (2024) 2020 data Watanabe et al. (2024) 2023 data
TOI-1670c	6170 ± 61	−0.3 ± 2.2		Lubin et al. (2023)
TOI-1842	6230 ± 50	−68 + 21 - 15	73 + 16 - 13	Hixenbaugh et al. (2023)
TOI-1859	6341 + 68 − 70	38.9 + 2.8 - 2.7		Dong et al. (2023)
TOI-1937	5814 + 91 − 93	4.0 ± 3.5		Yee et al. (2023)
TOI-2025	5880 ± 53	9 + 36 - 34 −10 + 7 - 10		Knudstrup et al. (2022) Wang et al. (2024)
TOI-2031	6420 + 120 − 110	−6.1 ± 7.5		Wang et al. (2024)
TOI-2076b	5200 ± 100	−3 + 15 - 16	18 + 10 - 9	Frazier et al. (2023)
TOI-2109	6530 + 160 − 150	1.7 ± 1.7		Wong et al. (2021)
TOI-2485	5939 ± 85	−20 + 26 - 21		Wang et al. (2024)
TOI-2524	5831 ± 80	10 + 19 - 22		Wang et al. (2024)
TOI-2533	6180 ± 60	−7 ± 14		Ferreira et al. (2021)
TOI-3362	6800 ± 100	1.2 + 2.8 - 2.7 2 + 4 - 5		Espinoza-Retamal et al. (2023) Prinoth et al. (2024)
TOI-3884	3180 ± 88	75 ± 10		Libby-Roberts et al.(2023)
TOI-3972	5424 + 95 − 90	−12.1 ± 8.5		Wang et al. (2024)
TOI-4201	3937 ± 70	−3.0 + 3.7 - 3.2	21.3 + 12.5 - 12.8	Gan et al.(2024)
TOI-4379	6020 ± 100	−1 + 22 - 29		Saunders et al.(2024)
TOI-4641	6560 + 300 − 340	1.41 ± 0.76	2.4 ± 1.3	Bieryla et al.(2024)
TOI-5126b	6150 + 110 − 130	1 ± 48		Radzom et al.(2024)
TOI-5398b	6000 ± 75	3.0 + 6.8 - 4.2 −24 + 14 - 13	13.2 ± 8.2	Mantovan et al.(2024) Radzom et al.(2024)
TOI-559	5925 + 85 − 76	10 + 12 - 14		Wang et al. (2024)
TOI-6029	6223 ± 100	−14 + 17 - 13		Saunders et al.(2024)
TOI-640	6460 + 130 − 150	184 ± 3	104 ± 2	Knudstrup et al. (2023)
TOI-677	6295 ± 80	0.3 ± 1.3 3.2 + 1.6 - 1.5 0 ± 1		Sedaghati et al. (2023) Hu et al. (2024) Prinoth et al. (2024)
TOI-778	6643 ± 150	18 ± 11		Clark et al. (2023)
TOI-858B	5842 + 84 − 79	99.3 + 3.8 - 3.7		Hagelberg et al. (2023)
TOI-942b	4928 + 125 − 85	1 + 41 - 33	2 + 27 - 33	Wirth et al. (2021)
TOI-942c	4928 + 125 − 85	24 ± 14	0 + 43 - 0	Teng et al. (2024)
TRAPPIST-1b	2566 ± 26	15 + 26 - 30		Hirano et al.(2020)
TRAPPIST-1e	2566 ± 26	9 + 45 - 51		Hirano et al.(2020)
TRAPPIST-1f	2566 ± 26	21 ± 32		Hirano et al.(2020)
TrES-1	5226 ± 50	30 ± 21		Narita et al. (2007)
TrES-2	5850 ± 50	−9 ± 12		Winn et al. (2008)
TrES-4	6295 ± 65	6.3 ± 4.7		Narita et al. (2010)
V1298 Tau b	5050 ± 100	2 + 12 - 4 15 + 15 - 16 4 + 7 - 10	8 + 4 - 7	Gaidos et al. (2022) LPVs Gaidos et al. (2022) RV Johnston et al. (2021)
V1298 Tau c	5050 ± 100	4.9 + 15.0 - 15.1		Feinstein et al. (2021)
WASP-1	6160 ± 64	−79.0 + 4.5 - 4.3 −59 + 99 - 26		Simpson et al. (2011) Albrecht et al. (2011)
WASP-2	5170 ± 60	−153 + 15 - 11 indeterminate		Triaud et al. (2010) Albrecht et al. (2011)
WASP-3	6440 ± 120	15 + 10 - 9 3.3 + 2.5 - 4.4 5 + 6 - 5 20.0 ± 3.3		Simpson et al. (2010) Tripathi et al. (2010) Miller et al. (2010) Oshagh et al. (2013)
WASP-4	5540 ± 55	4 + 34 - 43 −1 + 14 - 12		Triaud et al. (2010) Sanchis-Ojeda et al. (2011)
WASP-5	5770 ± 65	12.1 + 8.0 - 10.0 7.2 ± 9.5		Triaud et al. (2010) Fukui et al. (2011)
WASP-6	5375 ± 65	−11 + 18 - 14 7.2 ± 3.7		Gillon et al. (2009) Tregloan-Reed et al. (2015)
WASP-7	6520 ± 70	86 ± 6		Albrecht et al. (2012)
WASP-8	5690 ± 36	−123.3 + 3.4 - 4.4 −143.0 + 1.6 - 1.5		Queloz et al. (2010) Bourrier et al. (2017)
WASP-11	4900 ± 65	7 ± 5		Mancini et al. (2015)
WASP-12	6265 ± 50	59 + 15 - 20		Albrecht et al. (2012)
WASP-13	6025 ± 21	8 + 13 - 12		Brothwell et al. (2014)
WASP-14	6462 ± 75	−14 + 21 - 13 −33.1 ± 7.4		Joshi et al. (2009) Johnson et al. (2009)
WASP-15	6573 ± 70	−139.6 + 4.3 - 5.2		Triaud et al. (2010)
WASP-16	5630 ± 70	−4.2 + 11.0 - 13.9 11 + 26 - 19		Brown et al. (2012) Albrecht et al. (2012)
WASP-17	6550 ± 100	−147 + 49 - 11 167.4 ± 11.2 −148.5 + 4.2 - 5.4 −148.7 + 7.7 - 6.7		Anderson et al. (2010) Bayliss et al. (2010) Triaud et al. (2010) Anderson et al. (2011)
WASP-18	6400 ± 70	4.0 ± 5.0 13 ± 7		Triaud et al. (2010) Albrecht et al. (2012)
WASP-19	5460 ± 90	4.6 ± 5.2 15 ± 11 1.0 ± 1.2 −1.9 ± 1.1	0 ± 20	Hellier et al. (2011) Albrecht et al. (2012) Tregloan-Reed et al. (2013) Sedaghati et al. (2021)
WASP-20	5987 ± 20	12.7 ± 4.2		Anderson et al. (2015)
WASP-21	5924 ± 55	8 + 26 - 27		Chen et al. (2020)
WASP-22	6153 ± 46	22 ± 16		Anderson et al. (2011)
WASP-23	5046 ± 99	prograde		Triaud et al. (2011)
WASP-24	6107 ± 77	−4.7 ± 4.0 −5.8 ± 4.1		Simpson et al. (2011) Smith et al. (2012)
WASP-25	5736 ± 35	14.6 ± 6.7		Brown et al. (2012)
WASP-26	6015 ± 55	indeterminate −34 + 36 - 26		Anderson et al. (2011) Albrecht et al. (2012)
WASP-28	6084 ± 45	8 ± 18 6 ± 17		Anderson et al. (2015) Mocnik et al. (2020)
WASP-30	6208 ± 85	−7 + 27 - 19		Triaud et al. (2013)
WASP-31	6175 ± 70	2.8 ± 3.1 −6 ± 6		Brown et al. (2012) Albrecht et al. (2012)
WASP-32	6100 ± 100	10.5 + 6.4 - 6.5 −2 + 17 - 19	11 ± 14	Brown et al. (2012) Brothwell et al. (2014)
WASP-33	7430 ± 100	252 ± 2 −110.06 + 0.40 - 0.27 −112.93 + 0.23 - 0.22 −111.28 + 0.47 - 0.48 −114.01 + 0.22 - 0.20 −112.91 ± 0.24 −109.29 + 0.20 - 0.17 −111.70 ± 0.39 −111.64 ± 0.28 −94.9 ± 21.4	99 + 5 - 4 103 + 5 - 4 113.99 ± 0.22 108.19 + 0.95 - 0.97 91.3 ± 18.5	Collier Cameron et al. (2010) Johnson et al. (2015) 2008 data Johnson et al. (2015) 2014 data Iorio (2016) 2008 data Iorio (2016) 2014 data Watanabe et al. (2020) 2008 data Watanabe et al. (2020) 2011 data Watanabe et al. (2020) 2014 data Cauley et al. (2021) Borsa et al. (2021) Watanabe et al. (2022) Kálmán et al. (2022)
WASP-38	6436 ± 60	15 + 33 - 43 7.5 + 4.7 - 6.1		Simpson et al. (2011) Brown et al. (2012)
WASP-39	5485 ± 50	0 ± 11		Mancini et al. (2018)
WASP-41	5546 ± 33	29 + 10 - 14 6 ± 11		Neveu-VanMalle et al. (2016) Southworth et al. (2016)
WASP-43	4240 + 30 − 20	3.5 ± 6.8	0 + 20 - 0	Esposito et al. (2017)
WASP-47b	5576 ± 67	0 ± 24	29 + 11 - 13	Sanchis-Ojeda et al. (2015) Bourrier et al. (2023)
WASP-49	5600 ± 150	54 + 79 - 58		Wyttenbach et al. (2017)
WASP-52	5000 ± 100	24 + 17 - 9 3.8 ± 8.4 1.1 ± 1.1 0.60 + 0.93 - 0.94	20 ± 50	Hébrard et al. (2013) Mancini et al. (2017) Chen et al. (2020) Cegla et al. (2023)
WASP-53	4950 ± 60	−1 ± 12		Triaud et al. (2017)
WASP-60	6105 ± 50	−129 ± 17		Mancini et al. (2018)
WASP-61	6250 ± 150	4.0 + 17.1 - 18.4		Brown et al. (2017)
WASP-62	6230 ± 80	19.4 + 5.1 - 4.9		Brown et al. (2017)
WASP-66	6600 ± 150	−4 ± 22		Addison et al. (2016)
WASP-69	4700 ± 50	0.4 + 2.0 - 1.9		Casasayas-Barris et al. (2017)
WASP-71	6180 ± 52	20.1 ± 9.7 −1.9 + 7.1 - 7.5		Smith et al. (2013) Brown et al. (2017)
WASP-72	6250 ± 100	−7 + 11 - 12		Addison et al. (2018)
WASP-74	5984 ± 57	0.77 ± 0.99		Luque et al.(2020)
WASP-76	6329 ± 65	misaligned 61.3 + 7.6 - 5.1		Brown et al. (2017) Ehrenreich et al. (2020)
WASP-77	5605 ± 41	−8 + 19 - 18		Zak et al. (2024)
WASP-78	6100 ± 150	−6.4 ± 5.9		Brown et al. (2017)
WASP-79	6600 ± 100	−106 + 19 - 13 −95.2 + 0.9 - 1.0 −99.1 + 4.1 - 3.9		Addison et al. (2013) Brown et al. (2017) Johnson et al. (2017)
WASP-80	4145 ± 100	0 ± 20 −14 ± 14		Triaud et al. (2013) Triaud et al. (2015)
WASP-84b	5280 ± 80	−0.3 ± 1.7	17.3 ± 7.7	Anderson et al. (2015)
WASP-85	5685 ± 65	0 ± 14 −16.2 ± 2.9		Mocnik et al. (2016) Jiang et al. (2023)
WASP-87	6450 ± 120	−8 ± 11		Addison et al. (2016)
WASP-94	6170 ± 80	151 + 16 - 23 123.0 ± 3.0		Neveu-VanMalle et al. (2014) Ahrer et al. (2024)
WASP-100	6940 ± 120	79 + 19 - 10		Addison et al. (2018)
WASP-101	6380 ± 120	34 ± 3		Zak et al. (2024)
WASP-103	6110 ± 160	3 ± 33 2 + 35 - 36		Addison et al. (2016) Zak et al. (2024)
WASP-105	5070 ± 130	−14 + 28 - 24		Zak et al. (2024)
WASP-106	6265 ± 36	−1 ± 11 6 + 17 - 18 −3 + 9 - 10	26 + 12 - 17	Wright et al. (2023) Wright et al. (2023) Prinoth et al. (2024)
WASP-107	4425 ± 70	118 + 38 - 19 −158 + 15 - 19	90 ± 50 103.5 + 1.79 - 1.8	Dai et al. (2017) Rubenzahl et al. (2021) Bourrier et al. (2023)
WASP-109	6520 ± 140	99 + 10 - 9		Addison et al. (2018)
WASP-111	6400 ± 150	−5 ± 16		Anderson et al. (2014)
WASP-117	6040 ± 90	44 ± 11 −46.9 + 5.5 - 4.8	69.5 + 3.6 - 3.1	Lendl et al. (2014) Carone et al. (2021)
WASP-120	6450 ± 120	−2 ± 4		Zak et al. (2024)
WASP-121	6586 ± 59	−257.8 + 5.5 - 5.3 87.20 + 0.41 - 0.45 −87.08 + 0.29 - 0.27	88.1 ± 0.25	Delrez et al. (2016) Bourrier et al. (2020) Borsa et al. (2021)
WASP-122	5720 ± 130	0.09 + 0.88 - 0.90		Stangret et al. (2024)
WASP-127	5750 ± 100	−128.4 + 5.6 - 5.5 −150.6 + 8.1 - 8.7		Allart et al. (2020) Cristo et al. (2022)
WASP-130	5600 ± 100	−1 ± 2		Prinoth et al. (2024)
WASP-131	5990 ± 50	162.4 + 1.3 - 1.2 161 ± 5	123.7 + 12.8 - 8.0	Doyle et al. (2023) Zak et al. (2024)
WASP-134	5700 ± 100	−43.7 ± 9.9		Anderson et al. (2018)
WASP-139	5233 ± 60	−85.6 + 7.7 - 4.2		Espinoza-Retamal et al. (2024)
WASP-148	5437 ± 21	−8.2 + 8.7 - 9.7		Wang et al. (2022)
WASP-156	4910 ± 61	106 ± 14		Bourrier et al. (2023)
WASP-166	6050 ± 50	−3 ± 5 −15.5 + 2.9 - 2.8 −0.7 ± 0.6	0 + 56 - 0	Hellier et al. (2019) Doyle et al. (2022) Bourrier et al. (2023)
WASP-167	6900 ± 150	−165 ± 5		Temple et al. (2017)
WASP-174	6400 ± 100	31 ± 1		Temple et al. (2018)
WASP-178	9360 ± 150	105.7 + 3.6 - 4.2		Damasceno et al. (2024)
WASP-180	6500 ± 150	−157 ± 2		Temple et al. (2019)
WASP-189	8000 ± 80	89.3 ± 1.4 86.4 + 2.9 - 4.4 91.7 ± 1.2 90.07 ± 0.24	90.0 + 5.9 - 5.8 85.4 ± 4.3 89.6 ± 1.2	Anderson et al. (2018) Lendl et al. (2020) Deline et al. (2022) Prinoth et al. (2024)
WASP-190	6400 ± 100	21 ± 6		Temple et al. (2019)
XO-2	5332 ± 57	10 ± 72 7 ± 11	27 + 12 - 27	Narita et al. (2011) Damasso et al. (2015)
XO-3	6471 + 83 − 82	70 ± 15 37.3 ± 3.7 37.3 ± 3.0		Hébrard et al. (2008) Winn et al. (2009) Hirano et al. (2011)
XO-4	6397 ± 70	−46.7 + 8.1 - 6.1		Narita et al. (2010)
XO-6	6720 ± 100	−20.7 ± 2.3		Crouzet et al. (2017)
pi Men c	5998 ± 62	−24.0 ± 4.1	26.9 + 5.8 - 4.7	Hozdic et al. (2021)

Last modified: 2024/10/04 John Southworth (Keele University, UK)