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Table A.1

Spin–orbit angle values (projected in the sky plane and 3D) used in our analysis along with their sources.

Planet name Projected spin-orbit angle 3D spin–orbit angle
λ(deg) Source ψ(deg) Source
55 Cnc e 72.4−11.5+12.7$72.4_{ - 11.5}^{ + 12.7}$ Bourrier & Hébrard (2014) 72.7−12.7+12.2$72.7_{ - 12.7}^{ + 12.2}$ This work
AU Mic b −4.7−6.4+6.8$ - 4.7_{ - 6.4}^{ + 6.8}$ Hirano et al. (2020b) 9.2−5.3+4.3$9.2_{ - 5.3}^{ + 4.3}$ This work
CoRoT-1 b 77.0−11.0+11.0$77.0_{ - 11.0}^{ + 11.0}$ Pont et al. (2010) — —
CoRoT-11 b 0.1−2.6+2.6$0.1_{ - 2.6}^{ + 2.6}$ Gandolfi et al. (2012) — —
CoRoT-18 b −10.0−20.0+20.0$ - 10.0_{ - 20.0}^{ + 20.0}$ Hébrard et al. (2011b) 20.0−20.0+20.0$20.0_{ - 20.0}^{ + 20.0}$ Hébrard et al. (2011b)
CoRoT-19 b −52.0−22.0+27.0$ - 52.0_{ - 22.0}^{ + 27.0}$ Guenther et al. (2012) — —
CoRoT-2 b 7.2−4.5+4.5$7.2_{ - 4.5}^{ + 4.5}$ Bouchy et al. (2008) 10.7−5.1+4.3$10.7_{ - 5.1}^{ + 4.3}$ This work
CoRoT-3 b −37.6−10.0+22.3$ - 37.6_{ - 10.0}^{ + 22.3}$ Triaud et al. (2009) — —
DS Tuc b 2.9−0.9+0.9$2.9_{ - 0.9}^{ + 0.9}$ Zhou et al. (2020) 14.2−3.6+2.9$14.2_{ - 3.6}^{ + 2.9}$ This work
GJ 3470 b 101.0−14.0+29.0$101.0_{ - 14.0}^{ + 29.0}$ Stefànsson et al. (2022) 97.0−11.0+16.0$97.0_{ - 11.0}^{ + 16.0}$ Stefànsson et al. (2022)
GJ 436 b 114.0−17.0+23.0$114.0_{ - 17.0}^{ + 23.0}$ Bourrier et al. (2022) 103.0−12.0+13.0$103.0_{ - 12.0}^{ + 13.0}$ Bourrier et al. (2022)
HAT-P-1 b 3.7−2.1+2.1$3.7_{ - 2.1}^{ + 2.1}$ Johnson et al. (2008) — —
HAT-P-11 b 133.9−8.3+7.1$133.9_{ - 8.3}^{ + 7.1}$ Bourrier et al. (2023) 104.9−9.1+8.6$104.9_{ - 9.1}^{ + 8.6}$ Bourrier et al. (2023)
HAT-P-12 b −54.0−13.0+41.0$ - 54.0_{ - 13.0}^{ + 41.0}$ Mancini et al. (2018) — —
HAT-P-13 b 1.9−8.6+8.6$1.9_{ - 8.6}^{ + 8.6}$ Winn et al. (2010b) — —
HAT-P-14 b 189.1−5.1+5.1$189.1_{ - 5.1}^{ + 5.1}$ Winn et al. (2011) — —
HAT-P-16 b −2.0−46.0+55.0$ - 2.0_{ - 46.0}^{ + 55.0}$ Albrecht et al. (2012b) — —
HAT-P-17 b 19.0−16.0+14.0$19.0_{ - 16.0}^{ + 14.0}$ Fulton et al. (2013) — —
HAT-P-18 b 132.0−15.0+15.0$132.0_{ - 15.0}^{ + 15.0}$ Esposito et al. (2014) — —
HAT-P-2 b 0.2−12.5+12.2$0.2_{ - 12.5}^{ + 12.2}$ Loeillet et al. (2008) — —
HAT-P-20 b −8.0−6.9+6.9$ - 8.0_{ - 6.9}^{ + 6.9}$ Esposito et al. (2017) 36.0−12.0+10.0$36.0_{ - 12.0}^{ + 10.0}$ Esposito et al. (2017)
HAT-P-22 b −2.1−3.0+3.0$ - 2.1_{ - 3.0}^{ + 3.0}$ Mancini et al. (2018) 24.0−18.0+18.0$24.0_{ - 18.0}^{ + 18.0}$ Mancini et al. (2018)
HAT-P-23 b 15.0−22.0+22.0$15.0_{ - 22.0}^{ + 22.0}$ Moutou et al. (2011) — —
HAT-P-24 b 20.0−16.0+16.0$20.0_{ - 16.0}^{ + 16.0}$ Albrecht et al. (2012b) — —
HAT-P-27 b 24.2−44.5+76.0$24.2_{ - 44.5}^{ + 76.0}$ Brown et al. (2012b) — —
HAT-P-3 b −25.3−22.8+29.4$ - 25.3_{ - 22.8}^{ + 29.4}$ Bourrier et al. (2023) 75.7−7.9+8.5$75.7_{ - 7.9}^{ + 8.5}$ Bourrier et al. (2023)
HAT-P-30 b 73.5−9.0+9.0$73.5_{ - 9.0}^{ + 9.0}$ Johnson et al. (2011) — —
HAT-P-32 b 85.0−1.5+1.5$85.0_{ - 1.5}^{ + 1.5}$ Albrecht et al. (2012b) — —
HAT-P-33 b −5.9−4.1+4.1$ - 5.9_{ - 4.1}^{ + 4.1}$ Bourrier et al. (2023) — —
HAT-P-34 b 0.0−14.0+14.0$0.0_{ - 14.0}^{ + 14.0}$ Albrecht et al. (2012b) — —
HAT-P-36 b −14.0−18.0+18.0$ - 14.0_{ - 18.0}^{ + 18.0}$ Mancini et al. (2015) 0.0−63.0+63.0$0.0_{ - 63.0}^{ + 63.0}$ Mancini et al. (2015)
HAT-P-4 b −4.9−11.9+11.9$ - 4.9_{ - 11.9}^{ + 11.9}$ Winn et al. (2011) — —
HAT-P-41 b −22.1−6.0+0.8$ - 22.1_{ - 6.0}^{ + 0.8}$ Johnson et al. (2017) — —
HAT-P-49 b −97.7−1.8+1.8$ - 97.7_{ - 1.8}^{ + 1.8}$ Bourrier et al. (2023) — —
HAT-P-56 b 8.0−2.0+2.0$8.0_{ - 2.0}^{ + 2.0}$ Zhou et al. (2016a) — —
HAT-P-6 b 165.0−6.0+6.0$165.0_{ - 6.0}^{ + 6.0}$ Albrecht et al. (2012b) — —
HAT-P-69 b 30.3−7.3+6.1$30.3_{ - 7.3}^{ + 6.1}$ Zhou et al. (2019b) — —
HAT-P-7 b 220.3−9.3+8.2$220.3_{ - 9.3}^{ + 8.2}$ Benomar et al. (2014) 115.0−16.0+19.0$115.0_{ - 16.0}^{ + 19.0}$ Benomar et al. (2014)
HAT-P-70 b 107.9−1.7+2.0$107.9_{ - 1.7}^{ + 2.0}$ Bello-Arufe et al. (2022) — —
HAT-P-8 b −17.0−11.5+9.2$ - 17.0_{ - 11.5}^{ + 9.2}$ Moutou et al. (2011) — —
HAT-P-9 b −16.0−8.0+8.0$ - 16.0_{ - 8.0}^{ + 8.0}$ Moutou et al. (2011) — —
HATS-14 b 76.0−5.0+4.0$76.0_{ - 5.0}^{ + 4.0}$ Zhou et al. (2015) — —
HATS-2 b 8.0−8.0+8.0$8.0_{ - 8.0}^{ + 8.0}$ Mohler-Fischer et al. (2013) 28.5−18.0+14.0$28.5_{ - 18.0}^{ + 14.0}$ This work
HATS-3 b 3.0−25.0+25.0$3.0_{ - 25.0}^{ + 25.0}$ Addison et al. (2014) — —
HATS-70 b 8.9−4.5+5.6$8.9_{ - 4.5}^{ + 5.6}$ Zhou et al. (2019a) 13.2−5.9+6.4$13.2_{ - 5.9}^{ + 6.4}$ Zhou et al. (2019a)
HD 106315 c −2.7−2.6+2.7$ - 2.7_{ - 2.6}^{ + 2.7}$ Bourrier et al. (2023) — —
HD 149026 b 12.0−7.0+7.0$12.0_{ - 7.0}^{ + 7.0}$ Albrecht et al. (2012b) — —
HD 17156 b 10.0−5.1+5.1$10.0_{ - 5.1}^{ + 5.1}$ Narita et al. (2009) 61.3−6.8+6.0$61.3_{ - 6.8}^{ + 6.0}$ This work
HD 189733 b −0.4−0.2+0.2$ - 0.4_{ - 0.2}^{ + 0.2}$ Cegla et al. (2016) 7.0−4.0+12.0$7.0_{ - 4.0}^{ + 12.0}$ Cegla et al. (2016)
HD 209458 b 1.6−0.1+0.1$1.6_{ - 0.1}^{ + 0.1}$ Casasayas-Barris et al. (2021) 37.3−5.4+8.8$37.3_{ - 5.4}^{ + 8.8}$ This work
HD 3167 b −6.6−7.9+6.6$ - 6.6_{ - 7.9}^{ + 6.6}$ Bourrier et al. (2021) 29.5−9.4+7.2$29.5_{ - 9.4}^{ + 7.2}$ Bourrier et al. (2021)
HD 3167 c −108.9−5.5+5.4$ - 108.9_{ - 5.5}^{ + 5.4}$ Bourrier et al. (2021) 107.7−4.9+5.1$107.7_{ - 4.9}^{ + 5.1}$ Bourrier et al. (2021)
HD 332231 b 2.0−6.0+6.0$2.0_{ - 6.0}^{ + 6.0}$ Knudstrup & Albrecht (2022) — —
HD 63433 b 8.0−45.0+33.0$8.0_{ - 45.0}^{ + 33.0}$ Mann et al. (2020) 33.1−26.2+17.0$33.1_{ - 26.2}^{ + 17.0}$ This work
HD 63433 c −1.0−32.0+35.0$ - 1.0_{ - 32.0}^{ + 35.0}$ Dai et al. (2020) 26.4−20.3+13.0$26.4_{ - 20.3}^{ + 13.0}$ This work
HD 80606 b 42.0−8.0+8.0$42.0_{ - 8.0}^{ + 8.0}$ Hébrard et al. (2010) — —
HD 85628 A b −115.1−3.6+2.7$ - 115.1_{ - 3.6}^{ + 2.7}$ Dorval et al. (2020) — —
HD 89345 b 74.2−32.5+33.6$74.2_{ - 32.5}^{ + 33.6}$ Bourrier et al. (2023) 80.1−23.1+22.3$80.1_{ - 23.1}^{ + 22.3}$ Bourrier et al. (2023)
HIP 67522 b 5.8−3.7+2.5$5.8_{ - 3.7}^{ + 2.5}$ Heitzmann et al. (2021) 20.2−8.7+10.3$20.2_{ - 8.7}^{ + 10.3}$ Heitzmann et al. (2021)
K2-105 b −81.0−47.0+50.0$ - 81.0_{ - 47.0}^{ + 50.0}$ Bourrier et al. (2023) — —
K2-140 b 0.5−9.7+9.7$0.5_{ - 9.7}^{ + 9.7}$ Rice et al. (2021) 24.0−18.5+10.9$24.0_{ - 18.5}^{ + 10.9}$ This work
K2-232 b −11.1−6.6+6.6$ - 11.1_{ - 6.6}^{ + 6.6}$ Wang et al. (2021) — —
K2-25 b 3.0−16.0+16.0$3.0_{ - 16.0}^{ + 16.0}$ Stefansson etal. (2020) 17.0−8.0+11.0$17.0_{ - 8.0}^{ + 11.0}$ Stefansson et al. (2020)
K2-267 b −1.5−0.8+0.8$ - 1.5_{ - 0.8}^{ + 0.8}$ Yu et al. (2018) 3.4−3.5+1.6$3.4_{ - 3.5}^{ + 1.6}$ Yu et al. (2018)
K2-29 b 1.5−8.7+8.7$1.5_{ - 8.7}^{ + 8.7}$ Santerne et al. (2016) 21.6−13.3+10.3$21.6_{ - 13.3}^{ + 10.3}$ This work
K2-290 b 173.0−53.0+45.0$173.0_{ - 53.0}^{ + 45.0}$ Hjorth et al. (2021) — —
K2-290 c 153.0−8.0+8.0$153.0_{ - 8.0}^{ + 8.0}$ Hjorth et al. (2021) 124.0−6.0+6.0$124.0_{ - 6.0}^{ + 6.0}$ Hjorth et al. (2021)
K2-34 b −1.0−10.0+9.0$ - 1.0_{ - 10.0}^{ + 9.0}$ Hirano et al. (2016) —
KELT-1 b 2.0−16.0+16.0$2.0_{ - 16.0}^{ + 16.0}$ Siverd et al. (2012) — —
KELT-11 b −77.9−2.3+2.4$ - 77.9_{ - 2.3}^{ + 2.4}$ Mounzer et al. (2022) — —
KELT-17 b 115.9−4.1+4.1$115.9_{ - 4.1}^{ + 4.1}$ Zhou et al. (2016b) 116.0−4.0+4.0$116.0_{ - 4.0}^{ + 4.0}$ Zhou et al. (2016b)
KELT-19 b −179.7−3.8+3.7$ - 179.7_{ - 3.8}^{ + 3.7}$ Siverd et al. (2018) — —
KELT-20 b 3.4−2.1+2.1$3.4_{ - 2.1}^{ + 2.1}$ Lund et al. (2017) 35.6−34.0+34.2$35.6_{ - 34.0}^{ + 34.2}$ Lund et al. (2017)
KELT-21 b −5.6−1.9+1.7$ - 5.6_{ - 1.9}^{ + 1.7}$ Johnson et al. (2017) —
KELT-24 b 2.6−3.6+5.1$2.6_{ - 3.6}^{ + 5.1}$ Rodriguez et al. (2019) — —
KELT-25 b 23.4−2.3+3.2$23.4_{ - 2.3}^{ + 3.2}$ Rodríguez Martínez et al. (2020) — —
KELT-4 A b 14.0−64.0+100.0$14.0_{ - 64.0}^{ + 100.0}$ Eastman etal. (2016) — —
KELT-6 b −36.0−11.0+11.0$ - 36.0_{ - 11.0}^{ + 11.0}$ Damasso etal. (2015b) — —
KELT-7 b 2.7−0.6+0.6$2.7_{ - 0.6}^{ + 0.6}$ Zhou et al. (2016a) — —
KELT-9 b −84.8−0.3+0.3$ - 84.8_{ - 0.3}^{ + 0.3}$ Stephan et al. (2022) 87.5−0.2+0.2$87.5_{ - 0.2}^{ + 0.2}$ Stephan et al. (2022)
KOI-142 b 6.4−0.1+0.1$6.4_{ - 0.1}^{ + 0.1}$ Nesvorný et al. (2013) —
KOI-142 c −107.1−0.6+0.9$ - 107.1_{ - 0.6}^{ + 0.9}$ Nesvorný et al. (2013) — —
KOI-368 b 10.0−2.0+2.0$10.0_{ - 2.0}^{ + 2.0}$ Ahlers et al. (2014) — —
KOI-94 d −11.0−11.0+11.0$ - 11.0_{ - 11.0}^{ + 11.0}$ Albrecht et al. (2013) — —
Kepler-1115 b 1.0−13.0+13.0$1.0_{ - 13.0}^{ + 13.0}$ Barnes et al. (2015) −4.0−60.0+60.0$ - 4.0_{ - 60.0}^{ + 60.0}$ Barnes et al. (2015)
Kepler-13 b 59.2−0.1+0.1$59.2_{ - 0.1}^{ + 0.1}$ Howarth & Morello (2017) 60.2−0.1+0.1$60.2_{ - 0.1}^{ + 0.1}$ Howarth & Morello (2017)
Kepler-17 b 0.0−15.0+15.0$0.0_{ - 15.0}^{ + 15.0}$ Désert et al. (2011) 0.0−15.0+15.0$0.0_{ - 15.0}^{ + 15.0}$ Désert et al. (2011)
Kepler-25 c −0.9−6.4+7.7$ - 0.9_{ - 6.4}^{ + 7.7}$ Bourrier et al. (2023) 24.1−9.3+9.2$24.1_{ - 9.3}^{ + 9.2}$ Bourrier et al. (2023)
Kepler-30b 4.0−10.0+10.0$4.0_{ - 10.0}^{ + 10.0}$ Sanchis-Ojeda etal. (2012) — —
Kepler-420 b 74.0−46.0+32.0$74.0_{ - 46.0}^{ + 32.0}$ Santerne et al. (2014) — —
Kepler-448 b −7.1−2.8+4.2$ - 7.1_{ - 2.8}^{ + 4.2}$ Johnson et al. (2017) — —
Kepler-462 b −32.0−11.0+11.0$ - 32.0_{ - 11.0}^{ + 11.0}$ Ahlers et al. (2015) 72.0−3.0+3.0$72.0_{ - 3.0}^{ + 3.0}$ This work
Kepler-462 c −32.0−40.0+40.0$ - 32.0_{ - 40.0}^{ + 40.0}$ Ahlers et al. (2015) 72.2−9.9+7.5$ - 32.0_{ - 40.0}^{ + 40.0}$ This work
Kepler-63 b −135.0−26.8+21.2$ - 135.0_{ - 26.8}^{ + 21.2}$ Bourrier et al. (2023) 114.6−12.5+16.6$114.6_{ - 12.5}^{ + 16.6}$ Bourrier et al. (2023)
Kepler-8 b 5.0−7.0+7.0$5.0_{ - 7.0}^{ + 7.0}$ Albrecht et al. (2012b) — —
Kepler-89 d −6.0−11.0+13.0$ - 6.0_{ - 11.0}^{ + 13.0}$ Hirano et al. (2012) — —
Kepler-9 b −13.0−16.0+16.0$ - 13.0_{ - 16.0}^{ + 16.0}$ Wang et al. (2018) — —
MASCARA-1 b 69.2−3.4+3.1$69.2_{ - 3.4}^{ + 3.1}$ Hooton et al. (2022) 72.1−2.4+2.5$72.1_{ - 2.4}^{ + 2.5}$ Hooton et al. (2022)
MASCARA-4 b 244.0−15.0+15.0$244.0_{ - 15.0}^{ + 15.0}$ Ahlers et al. (2020) 104.0−13.0+7.0$104.0_{ - 13.0}^{ + 7.0}$ Ahlers et al. (2020)
NGTS-2 b −11.3−4.8+4.8$ - 11.3_{ - 4.8}^{ + 4.8}$ Anderson etal. (2018a) — —
Qatar-1 b −8.4−7.1+7.1$ - 8.4_{ - 7.1}^{ + 7.1}$ Covino et al. (2013) 18.0−10.8+7.7$18.0_{ - 10.8}^{ + 7.7}$ This work
Qatar-2 b 0.0−8.0+8.0$0.0_{ - 8.0}^{ + 8.0}$ Močnik et al. (2017) —
TOI-1268 b 40.0−9.9+7.2$40.0_{ - 9.9}^{ + 7.2}$ Dong et al. (2022) — —
TOI-1431 b −155.0−10.0+20.0$ - 155.0_{ - 10.0}^{ + 20.0}$ Stangret et al. (2021) — —
TOI-1518 b 240.3−1.0+0.9$240.3_{ - 1.0}^{ + 0.9}$ Cabot et al. (2021) — —
TOI-2025 b 9.0−31.0+33.0$9.0_{ - 31.0}^{ + 33.0}$ Knudstrup et al. (2022) — —
TOI-2109 b 1.7−1.7+1.7$1.7_{ - 1.7}^{ + 1.7}$ Wong et al. (2021) — —
TOI-942 b 1.0−33.0+41.0$1.0_{ - 33.0}^{ + 41.0}$ Wirth et al. (2021) 2.0−23.0+27.0$2.0_{ - 23.0}^{ + 27.0}$ Wirth et al. (2021)
TRAPPIST-1 b 15.0−30.0+26.0$15.0_{ - 30.0}^{ + 26.0}$ Hirano et al. (2020a) — —
TRAPPIST-1 e 9.0−51.0+45.0$9.0_{ - 51.0}^{ + 45.0}$ Hirano et al. (2020a) — —
TRAPPIST-1 f 21.0−32.0+32.0$21.0_{ - 32.0}^{ + 32.0}$ Hirano et al. (2020a) — —
TrES-1 b 30.0−21.0+21.0$30.0_{ - 21.0}^{ + 21.0}$ Narita et al. (2007) — —
TrES-2 b −9.0−12.0+12.0$ - 9.0_{ - 12.0}^{ + 12.0}$ Winn et al. (2008) — —
TrES-4 b 6.3−4.7+4.7$6.3_{ - 4.7}^{ + 4.7}$ Narita et al. (2010b) — —
V1298 Tau b 4.0−10.0+7.0$4.0_{ - 10.0}^{ + 7.0}$ Johnson et al. (2022) 8.0−7.0+4.0$8.0_{ - 7.0}^{ + 4.0}$ Johnson et al. (2022)
V1298 Tau c 4.9−15.1+15.0$4.9_{ - 15.1}^{ + 15.0}$ Feinstein et al. (2021) 21.3−10.3+10.5$21.3_{ - 10.3}^{ + 10.5}$ This work
WASP-1 b −59.0−26.0+99.0$ - 59.0_{ - 26.0}^{ + 99.0}$ Albrecht et al. (2011) — —
WASP-100 b 79.0−10.0+19.0$79.0_{ - 10.0}^{ + 19.0}$ Addison et al. (2018) 82.0−15.3+14.9$82.0_{ - 15.3}^{ + 14.9}$ This work
WASP-103 b 3.0−33.0+33.0$3.0_{ - 33.0}^{ + 33.0}$ Addison et al. (2016) — —
WASP-107 b −158.0−18.5+15.2$ - 158.0_{ - 18.5}^{ + 15.2}$ Bourrier et al. (2023) 103.5−1.8+1.7$103.5_{ - 1.8}^{ + 1.7}$ Bourrier et al. (2023)
WASP-109 b 99.0−9.0+10.0$99.0_{ - 9.0}^{ + 10.0}$ Addison et al. (2018) — —
WASP-11 b 7.0−5.0+5.0$7.0_{ - 5.0}^{ + 5.0}$ Mancini et al. (2015) — —
WASP-111 b −5.0−16.0+16.0$ - 5.0_{ - 16.0}^{ + 16.0}$ Anderson et al. (2014) — —
WASP-117 b −46.9−4.8+5.5$ - 46.9_{ - 4.8}^{ + 5.5}$ Carone et al. (2021) 69.6−4.1+4.7$69.6_{ - 4.1}^{ + 4.7}$ Carone et al. (2021)
WASP-12 b 59.0−20.0+15.0$59.0_{ - 20.0}^{ + 15.0}$ Albrecht et al. (2012b) — —
WASP-121 b 87.2−0.5+0.4$87.2_{ - 0.5}^{ + 0.4}$ Bourrier et al. (2020) 88.1−0.2+0.2$88.1_{ - 0.2}^{ + 0.2}$ Bourrier et al. (2020)
WASP-127 b −128.4−5.5+5.6$ - 128.4_{ - 5.5}^{ + 5.6}$ Allart et al. (2020) — —
WASP-13 b 8.0−12.0+13.0$8.0_{ - 12.0}^{ + 13.0}$ Brothwell et al. (2014) — —
WASP-134b −43.7−9.9+9.9$ - 43.7_{ - 9.9}^{ + 9.9}$ Anderson etal. (2018b) — —
WASP-14 b −33.1−7.4+7.4$ - 33.1_{ - 7.4}^{ + 7.4}$ Johnson et al. (2009) — —
WASP-148 b −8.2−9.7+8.7$ - 8.2_{ - 9.7}^{ + 8.7}$ Wang et al. (2022) 29.8−23.4+13.2$29.8_{ - 23.4}^{ + 13.2}$ This work
WASP-15 b −139.6−4.3+5.2$ - 139.6_{ - 4.3}^{ + 5.2}$ Triaud et al. (2010) — —
WASP-156b 105.7−14.4+14.0$105.7_{ - 14.4}^{ + 14.0}$ Bourrier et al. (2023) — —
WASP-16b −4.2−13.9+11.0$ - 4.2_{ - 13.9}^{ + 11.0}$ Brown et al. (2012a) — —
WASP-166 b −0.7−1.6+1.6$ - 0.7_{ - 1.6}^{ + 1.6}$ Bourrier et al. (2023) 14.2−12.8+6.0$14.2_{ - 12.8}^{ + 6.0}$ This work
WASP-167 b −165.0−5.0+5.0$ - 165.0_{ - 5.0}^{ + 5.0}$ Temple et al. (2017) 145.6−11.6+17.6$145.6_{ - 11.6}^{ + 17.6}$ This work
WASP-17 b −148.5−4.2+5.1$ - 148.5_{ - 4.2}^{ + 5.1}$ Triaud et al. (2010) — —
WASP-174 b 31.0−1.0+1.0$31.0_{ - 1.0}^{ + 1.0}$ Temple et al. (2018) — —
WASP-178 b 91.3−6.3+6.5$91.3_{ - 6.3}^{ + 6.5}$ Rodriguez Martinez et al. (2020) — —
WASP-18 b 4.0−5.0+5.0$4.0_{ - 5.0}^{ + 5.0}$ Triaud et al. (2010) — —
WASP-180 b −162.0−5.0+5.0$ - 162.0_{ - 5.0}^{ + 5.0}$ Temple et al. (2019b) 148.9−7.8+9.6$148.9_{ - 7.8}^{ + 9.6}$ This work
WASP-189 b 91.7−1.2+1.2$91.7_{ - 1.2}^{ + 1.2}$ Deline et al. (2022) 89.6−1.2+1.2$89.6_{ - 1.2}^{ + 1.2}$ Deline et al. (2022)
WASP-19 b −1.9−1.1+1.1$ - 1.9_{ - 1.1}^{ + 1.1}$ Sedaghati et al. (2021) 14.2−12.9+7.8$14.2_{ - 12.9}^{ + 7.8}$ This work
WASP-190 b 21.0−6.0+6.0$21.0_{ - 6.0}^{ + 6.0}$ Temple et al. (2019a) — —
WASP-2 b −153.0−15.0+11.0$4.0_{ - 17.1}^{ + 18.4}$ Triaud et al. (2010) — —
WASP-20 b 12.7−4.2+4.2$12.7_{ - 4.2}^{ + 4.2}$ Anderson et al. (2015a) — —
WASP-21 b 8.0−27.0+26.0$8.0_{ - 27.0}^{ + 26.0}$ Chen et al. (2020a) — —
WASP-22 b 22.0−16.0+16.0$22.0_{ - 16.0}^{ + 16.0}$ Anderson et al. (2011) 3.05−14.3+13.6$3.05_{ - 14.3}^{ + 13.6}$ This work
WASP-24 b −4.7−4.0+4.0$ - 4.7_{ - 4.0}^{ + 4.0}$ Simpson et al. (2011) — —
WASP-25 b 14.6−6.7+6.7$14.6_{ - 6.7}^{ + 6.7}$ Brown et al. (2012a) — —
WASP-26 b −34.0−26.0+36.0$ - 34.0_{ - 26.0}^{ + 36.0}$ Albrecht et al. (2012b) — —
WASP-28 b 8.0−18.0+18.0$8.0_{ - 18.0}^{ + 18.0}$ Anderson et al. (2015a) — —
WASP-3 b 5.0−5.0+6.0$5.0_{ - 5.0}^{ + 6.0}$ Miller et al. (2010) — —
WASP-31 b 2.8−3.1+3.1$2.8_{ - 3.1}^{ + 3.1}$ Brown et al. (2012a) — —
WASP-32 b 10.5−6.5+6.4$10.5_{ - 6.5}^{ + 6.4}$ Brown et al. (2012b) 2.0−16.0+16.0$2.0_{ - 16.0}^{ + 16.0}$ Brown et al. (2012b)
WASP-33 b −111.6−0.3+0.3$ - 111.6_{ - 0.3}^{ + 0.3}$ Watanabe et al. (2022) 108.2−1.0+0.9$108.2_{ - 1.0}^{ + 0.9}$ Watanabe et al. (2022)
WASP-38 b 7.5−6.1+4.7$7.5_{ - 6.1}^{ + 4.7}$ Brown et al. (2012b) — —
WASP-39 b 0.0−11.0+11.0$0.0_{ - 11.0}^{ + 11.0}$ Mancini et al. (2018) — —
WASP-4 b 4.0−34.0+43.0$4.0_{ - 34.0}^{ + 43.0}$ Triaud et al. (2010) 39.3−24.2+16.8$39.3_{ - 24.2}^{ + 16.8}$ This work
WASP-41 b 6.0−11.0+11.0$6.0_{ - 11.0}^{ + 11.0}$ Southworth et al. (2016) 16.7−9.3+7.9$16.7_{ - 9.3}^{ + 7.9}$ This work
WASP-43 b 3.5−6.8+6.8$3.5_{ - 6.8}^{ + 6.8}$ Esposito et al. (2017) — —
WASP-47 b 0.0−24.0+24.0$0.0_{ - 24.0}^{ + 24.0}$ Sanchis-Ojeda et al. (2015) 29.2−13.3+11.1$29.2_{ - 13.3}^{ + 11.1}$ Bourrier et al. (2023)
WASP-49 b 54.0−58.0+79.0$54.0_{ - 58.0}^{ + 79.0}$ Wyttenbach et al. (2017) — —
WASP-5 b 12.1−8.0+10.0$12.1_{ - 8.0}^{ + 10.0}$ Triaud et al. (2010) 26.6−14.9+12.5$26.6_{ - 14.9}^{ + 12.5}$ This work
WASP-52 b 1.1−1.1+1.1$1.1_{ - 1.1}^{ + 1.1}$ Chen et al. (2020b) — —
WASP-53 b −1.0−12.0+12.0$ - 1.0_{ - 12.0}^{ + 12.0}$ Triaud et al. (2017) — —
WASP-6 b 7.2−3.7+3.7$7.2_{ - 3.7}^{ + 3.7}$ Tregloan-Reed et al. (2015) 29.6−22.7+13.7$29.6_{ - 22.7}^{ + 13.7}$ This work
WASP-60 b −129.0−17.0+17.0$ - 129.0_{ - 17.0}^{ + 17.0}$ Mancini et al. (2018) — —
WASP-61 b 4.0−18.4+17.1$4.0_{ - 18.4}^{ + 17.1}$ Brown et al. (2017) — —
WASP-62 b 19.4−4.9+5.1$19.4_{ - 4.9}^{ + 5.1}$ Brown et al. (2017) — —
WASP-66 b −4.0−22.0+22.0$ - 4.0_{ - 22.0}^{ + 22.0}$ Addison et al. (2016) — —
WASP-69 b 0.4−2.0+1.9$0.4_{ - 2.0}^{ + 1.9}$ Casasayas-Barris et al. (2017) 15.6−14.3+7.3$15.6_{ - 14.3}^{ + 7.3}$ This work
WASP-7 b 86.0−6.0+6.0$86.0_{ - 6.0}^{ + 6.0}$ Albrecht et al. (2012a) — —
WASP-71 b −1.9−7.5+7.1$ - 1.9_{ - 7.5}^{ + 7.1}$ Brown et al. (2017) — —
WASP-72 b −7.0−12.0+11.0$ - 7.0_{ - 12.0}^{ + 11.0}$ Addison et al. (2018) — —
WASP-74 b 0.8−1.0+1.0$0.8_{ - 1.0}^{ + 1.0}$ Luque et al. (2020) — —
WASP-76 b 61.3−5.1+7.6$61.3_{ - 5.1}^{ + 7.6}$ Ehrenreich et al. (2020) — —
WASP-78 b −6.4−5.9+5.9$ - 6.4_{ - 5.9}^{ + 5.9}$ Brown et al. (2017) — —
WASP-79 b −99.1−3.9+4.1$ - 99.1_{ - 3.9}^{ + 4.1}$ Johnson et al. (2017) — —
WASP-8 b −143.0−1.5+1.6$ - 143.0_{ - 1.5}^{ + 1.6}$ Bourrier et al. (2017) — —
WASP-80 b −14.0−14.0+14.0$ - 14.0_{ - 14.0}^{ + 14.0}$ Triaud et al. (2015) — —
WASP-84 b −0.3−1.7+1.7$ - 0.3_{ - 1.7}^{ + 1.7}$ Anderson et al. (2015b) 17.3−7.7+7.7$17.3_{ - 7.7}^{ + 7.7}$ Anderson et al. (2015b)
WASP-87 b −8.0−11.0+11.0$ - 8.0_{ - 11.0}^{ + 11.0}$ Addison et al. (2016) — —
WASP-94 b 151.0−23.0+16.0$151.0_{ - 23.0}^{ + 16.0}$ Neveu-VanMalle et al. (2014) — —
XO-2 b 7.0−11.0+11.0$7.0_{ - 11.0}^{ + 11.0}$ Damasso et al. (2015a) 27.0−27.0+12.0$27.0_{ - 27.0}^{ + 12.0}$ Damasso et al. (2015a)
XO-3 b 37.3−3.0+3.0$37.3_{ - 3.0}^{ + 3.0}$ Hirano et al. (2011) — —
XO-4 b −46.7−6.1+8.1$ - 46.7_{ - 6.1}^{ + 8.1}$ Narita et al. (2010a) — —
XO-6 b −20.7−2.3+2.3$ - 20.7_{ - 2.3}^{ + 2.3}$ Crouzet et al. (2017) — —
pi Men c −24.0−4.1+4.1$ - 24.0_{ - 4.1}^{ + 4.1}$ Kunovac Hodžić et al. (2021) 26.9−4.7+5.8$26.9_{ - 4.7}^{ + 5.8}$ Kunovac Hodžić et al. (2021)

Note: as for the 3D spin–orbit angles, we include the values coming for the literature, plus the ones we derive in our study by fitting for υeq sin i⋆ (as described in Sect. 4.1). The latter 3D obliquities are referenced as “This work” and can be readily used in future studies. We do not include the 3D obliquities we derive based on an isotropic stellar inclination distribution (Sect. 4.1) because of the underlying assumptions. We recommend using the latter approach only in ensemble studies and not for individual systems.

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