The MOPYS project: A survey of 70 planets in search of extended He I and H atmospheres - No evidence of enhanced evaporation in young planets

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Volume 689 (September 2024)

A&A, 689 (2024) A179

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Table 1

Transit and system parameters used to compute the transmission spectra for each planet analysed in this work.

	P	T₀^(a)	T₁₄^(b)	T₁₂^(b)	a_p	i_p	γ	K_★	K_p^(c)
Planet	(d)	(d)	(h)	(min)	(au)	(deg)	(km s⁻¹)	(m s⁻¹)	(km s⁻¹)
K2-100 b	1.6739035 (4)⁽²⁾	140.71941 (27)⁽²⁾	1.60 ± 0.01⁽¹⁾	2.8 ± 0.8⁽¹⁾	0.0301 (14)⁽²⁾	81.27 ± 0.37⁽²⁾	+34.393(3)⁽²⁾	10.6 ± 3.0⁽²⁾	193±9
MASCARA-2 b	3.4741070 (19)⁽¹⁾	909.5906(3)⁽²⁾	3.57 ± 0.02⁽¹⁾	29 ± 1⁽¹⁾	0.0542(21)⁽¹⁾	${86.15}_{- 0.27}^{+ 0.28}$ $86.15_{ - 0.27}^{ + 0.28}$ ⁽¹⁾	−21.07(3)⁽²⁾	322.51 ⁽³⁾	170 ± 7⁽³⁾
V1298 Tau c	8.249071 (58)⁽¹⁾	1854.3479(11)⁽¹⁾	4.66 ± 0.12⁽²⁾	12⁽²⁾	0.0841 (13)⁽³⁾	${88.5}_{- 0.7}^{+ 0.9}$ $88.5_{ - 0.7}^{ + 0.9}$ ⁽²⁾	+14.64(14)⁽⁴⁾	$4_{- 3}^{+ 5}$ $4_{ - 3}^{ + 5}$ ⁽³⁾	111 ± 2
TOI-1431 b	2.6502409(41)⁽¹⁾	1739.17728(11)⁽¹⁾	2.489 ± 0.009⁽¹⁾	0.716 ± 0.022⁽¹⁾	0.0465(17)⁽¹⁾	${88.5}_{- 0.7}^{+ 0.9}$ $88.5_{ - 0.7}^{ + 0.9}$ ⁽¹⁾	−25.154⁽¹⁾	294.1 ± 1.1 ⁽¹⁾	188.15⁽²⁾
TOI-2048 b	13.790546 (55)⁽¹⁾	1739.1123(27)⁽¹⁾	3.5 ± 0.1⁽¹⁾	${6.9}_{- 0.7}^{+ 1.2}$ $6.9_{ - 0.7}^{ + 1.2}$ ⁽¹⁾	0.1078(80)⁽¹⁾	89.41 ± 0.35⁽¹⁾	−7.6(2)⁽²⁾	~2.8⁽¹⁾	85±6
HD 63433 b	7.107789 (10)⁽²⁾	1916.45142(32)⁽²⁾	3.22 ± 0.03⁽¹⁾	9 ± 1 ⁽¹⁾	0.0719(44)⁽¹⁾	${89.4}_{- 0.6}^{+ 0.4}$ $89.4_{ - 0.6}^{ + 0.4}$ ⁽¹⁾	−15.81 (10)⁽¹⁾	${1.4}_{- 0.9}^{+ 1.4}$ $1.4_{ - 0.9}^{ + 1.4}$ ⁽³⁾	110±6
HD 63433 c	20.543888 (46)⁽²⁾	1844.05824(48)⁽²⁾	4.07 ± 0.03⁽¹⁾	8 ± 1 ⁽¹⁾	0.1458(62)⁽¹⁾	${89.15}_{- 0.20}^{+ 0.07}$ $89.15_{ - 0.20}^{ + 0.07}$ ⁽¹⁾	−15.81 (10)⁽¹⁾	${3.6}_{- 1.0}^{+ 1.1}$ $3.6_{ - 1.0}^{ + 1.1}$ ⁽³⁾	77 ± 3
HD 73583 b	6.3980580(26)⁽¹⁾	2592.56287(25)⁽¹⁾	${2.100}_{- 0.013}^{+ 0.015}$ $2.100_{ - 0.013}^{ + 0.015}$ ⁽¹⁾	6.9 ± 0.2⁽¹⁾	0.0618(20)⁽¹⁾	88.35 ± 0.07⁽¹⁾	+21.52⁽²⁾	${4.37}_{- 1.3}^{+ 1.5}$ $4.37_{ - 1.3}^{ + 1.5}$ ⁽³⁾	105±3
HD 73583 c	18.879300(48)⁽¹⁾	2949.58243(77)⁽¹⁾	${3.60}_{- 0.05}^{+ 0.03}$ $3.60_{ - 0.05}^{ + 0.03}$ ⁽¹⁾	6.9 ± 0.20⁽¹⁾	0.1270(40)⁽¹⁾	89.96 ± 0.03⁽¹⁾	+21.52⁽²⁾	${2.89}_{- 0.51}^{+ 0.53}$ $2.89_{ - 0.51}^{ + 0.53}$ ⁽³⁾	73.2 ± 2.3
HD235088b	7.4341394 (60)⁽¹⁾	2798.4635(56)⁽¹⁾	2.700 ± 0.025⁽¹⁾	4.4 ± 0.5⁽¹⁾	0.0725(35)⁽¹⁾	88.85 ± 0.30⁽¹⁾	−27.370(2)⁽²⁾	~2.5⁽¹⁾	106±5
K2-77 b	8.200139 (60)⁽¹⁾	2522.6338(35)⁽¹⁾	2.68 ± 0.22⁽¹⁾	${6.3}_{- 1.1}^{+ 1.5}$ $6.3_{ - 1.1}^{ + 1.5}$ ⁽¹⁾	0.0751 (45)⁽¹⁾	${88.7}_{- 0.4}^{+ 0.7}$ $88.7_{ - 0.4}^{ + 0.7}$ ⁽¹⁾	+7.35 (20)⁽²⁾	~3.4⁽¹⁾	100±6
TOI-2046b	1.4971842 (6)⁽¹⁾	1792.2767(23)⁽¹⁾	2.410(32)⁽¹⁾	21 ± 1⁽²⁾	0.0267(18)⁽²⁾	83.6 ± 0.9⁽¹⁾	−9.480(43)⁽¹⁾	374.7±7.8⁽¹⁾	193±13
TOI-1807b	0.54937084 (65)⁽¹⁾	2664.06930(75)⁽¹⁾	0.970 ± 0.022⁽¹⁾	${1.45}_{- 0.18}^{+ 0.25}$ $1.45_{ - 0.18}^{ + 0.25}$ ⁽¹⁾	0.0121 (9)⁽¹⁾	81.7 ± 1.8⁽¹⁾	−7.33 ± 0.59⁽³⁾	${2.39}_{- 0.46}^{+ 0.45}$ $2.39_{ - 0.46}^{ + 0.45}$ ⁽²⁾	235 ± 6
TOI-1136d	12.51937 (41)⁽¹⁾	2349.525(5)⁽¹⁾	4.12 ± 0.11⁽¹⁾	11.0 ± 0.5⁽¹⁾	0.1057(46)⁽¹⁾	89.41 ± 0.28⁽¹⁾	+6.91 ± 0.33⁽²⁾	~2.2 ± 0.6⁽¹⁾	92 ± 4
TOI-1268b	8.1577094(45)⁽¹⁾	3000.66841 (14)⁽²⁾	4.001 ± 0.025⁽¹⁾	21 ± 2⁽¹⁾	0.0711 (63)⁽¹⁾	${88.63}_{- 0.30}^{+ 0.32}$ $88.63_{ - 0.30}^{ + 0.32}$ ⁽¹⁾	+3.79 ± 0.14⁽³⁾	${31.7}_{- 2.6}^{+ 2.5}$ $31.7_{ - 2.6}^{ + 2.5}$ ⁽¹⁾	105±8
TOI-2076 b	10.355183 (65)⁽¹⁾	3079.5495(45)⁽²⁾	3.251 ± 0.03⁽³⁾	8.5 ± 0.2⁽³⁾	0.0682(13)⁽³⁾	88.9 ± 0.11⁽³⁾	−13.19 ± 0.21⁽⁴⁾	~2⁽³⁾	71.6±1.3
TOI-1683b	3.057541 (14)⁽¹⁾	2522.7001 (12)⁽¹⁾	${1.43}_{- 0.05}^{+ 0.07}$ $1.43_{ - 0.05}^{ + 0.07}$ ⁽¹⁾	${5.0}_{- 0.6}^{+ 0.8}$ $5.0_{ - 0.6}^{ + 0.8}$ ⁽¹⁾	0.0368(23)⁽¹⁾	86.80 ± 0.38⁽¹⁾	+38.4 ± 0.3⁽²⁾	~5⁽³⁾	130±8
WASP-189b	2.7240330(42)⁽¹⁾	1926.5416960(65)⁽¹⁾	4.351 ± 0.026⁽²⁾	18.6 ± 6.2⁽²⁾	0.05053(98)⁽¹⁾	84.03 ± 0.14⁽¹⁾	−24.465 ± 0.012⁽¹⁾	182 ± 13⁽¹⁾	200 ± 4
HAT-P-57b	2.4652950(32)⁽¹⁾	5113.48127 (48) ^(a,1)	3.499 ± 0.019⁽¹⁾	19.1 ± 0.8⁽¹⁾	0.0406(11)⁽¹⁾	88.26 ± 0.85⁽¹⁾	−5.99 ± 0.35⁽¹⁾	<215⁽¹⁾	180±5
TOI-2018 b	7.435583(22)⁽¹⁾	2746.4287(21)⁽²⁾	2.36 ± 0.09⁽¹⁾	6.5 ± 0.5⁽¹⁾	0.0609(22)⁽¹⁾	88.52 ± 0.22⁽¹⁾	−25.617 ± 0.002⁽³⁾	4.4 ± 1.0⁽¹⁾	89.1 ± 3.3

Notes. ^(a)T₀ given in BJD – 2457 000, except for HAT-P-57b that is BJD – 2450 000. ^(b)T₁₄ is the total transit duration between the first and fourth (T₄) contacts, and T₁₂ is the duration of the ingress-egress. ^(c)Calculated from K_p = 2π a_p P⁻¹ sin i_p using the parameters in this table, when there is no reference. K2-100b: ⁽¹⁾Stefansson et al. (2018), ⁽²⁾Barragán et al. (2019). MASCARA-2b: ⁽¹⁾Lund et al. (2017), ⁽²⁾Talens et al. (2018), ⁽³⁾Casasayas-Barris et al. (2019). V1298 Tau c: ⁽¹⁾J. Livingston, priv. comm., ⁽²⁾David et al. (2019), ⁽³⁾Suárez Mascareño et al. (2021), ⁽⁴⁾Gaidos et al. (2022). TOI-1431 b:⁽¹⁾ Addison et al. (2021), ⁽²⁾Stangret et al. (2021). TOI-2048 b: ⁽¹⁾This work (Appendix C), ⁽²⁾Newton et al. (2022). HD 63433 b: ⁽¹⁾Mann et al. (2020), ⁽²⁾Zhang et al. (2022c), ⁽³⁾Mallorquín et al. (2023). HD 63433 c: ⁽¹⁾Mann et al. (2020), ⁽²⁾Zhang et al. (2022c), ⁽³⁾Mallorquín et al. (2023). HD 73583 b: ⁽¹⁾This work (Appendix E), ⁽²⁾Gaia DR2 (Soubiran et al. 2018), ⁽³⁾Barragán et al. (2022), El Mufti et al. (2021). HD 73583 c:⁽¹⁾This work (Appendix E), ⁽²⁾Gaia DR2 (Soubiran et al. 2018), ⁽³⁾Barragán et al. (2022), El Mufti et al. (2021). HD 235088 b: ⁽¹⁾Orell-Miquel et al. (2023), ⁽²⁾Gaia DR2 (Soubiran et al. 2018). K2-77 b: ⁽¹⁾This work (Appendix F), ⁽²⁾Gaidos et al. (2017). TOI-2046 b: ⁽¹⁾Kabáth et al. (2022), ⁽²⁾Computed using this table parameters. TOI-1807b: ⁽¹⁾This work (Appendix G), ⁽²⁾Nardiello et al. (2022), ⁽³⁾Gaia DR2 (Soubiran et al. 2018). TOI-1136 d: ⁽¹⁾Dai et al. (2023a), ⁽²⁾Gaia DR2 (Soubiran et al. 2018). TOI-1268 b: ⁽¹⁾Šubjak et al. (2022), ⁽²⁾This work (Sect. 3.2),⁽³⁾ Gaia DR2 (Soubiran et al. 2018). TOI-2076 b: ⁽¹⁾Zhang et al. (2023b), ⁽²⁾This work (Appendix B.14), ⁽³⁾Osborn et al. (2022),⁽⁴⁾Gaia DR2 (Soubiran et al. 2018). TOI-1683b: ⁽¹⁾This work (Appendix K), ⁽²⁾Gaia DR2 (Soubiran et al. 2018), ⁽³⁾Zhang et al. (2023b). WASP-189b: ⁽¹⁾Lendl et al. (2020), ⁽²⁾Anderson et al. (2018). HAT-P-57b: ⁽¹⁾Hartman et al. (2015). TOI-2018 b: ⁽¹⁾Dai et al. (2023b), ⁽²⁾This work (Sect. 3.3), ⁽³⁾Gaia DR2 (Soubiran et al. 2018).

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