Revisited mass-radius relations for exoplanets below 120 M⊕

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Table A.1

Filtered catalogue with robust and reliable mass and radius measurements.

Planet	Reference in NASA Exo. Arch.	Reference in this work
TRAPPIST-1 d	Gillon et al. (2017)	Grimm et al. (2018)

TRAPPIST-1 h	-	Grimm et al. (2018)

TRAPPIST-1 e	Gillon et al. (2017)	Grimm et al. (2018)

TRAPPIST-1 f	Gillon et al. (2017)	Grimm et al. (2018)

TRAPPIST-1 b	Gillon et al. (2017)	Grimm et al. (2018)

TRAPPIST-1 g	Gillon et al. (2017)	Grimm et al. (2018)

TRAPPIST-1 c	Gillon et al. (2017)	Grimm et al. (2018)

LHS 1140 c	Ment et al. (2018)	Ment et al. (2018)

GJ 357 b	–	Luque et al. (2019)

Kepler-78 b	Stassun et al. (2017)	Grunblatt et al. (2015)

K2-229 b	Livingston et al. (2018)	Santerne et al. (2018)

Kepler-10 b	Esteves et al. (2015)	Rajpaul et al. (2017)*

Kepler-80 d	MacDonald et al. (2016)	Hadden & Lithwick (2017)

Kepler-36 b	Carter et al. (2012)	Hadden & Lithwick (2017)

Kepler-93 b	Stassun et al. (2017)	Dressing et al. (2015)

Kepler-65 d	Chaplin et al. (2013)	Mills et al. (2019)

HD 219134 c	Gillon et al. (2017)	Gillon et al. (2017)

HD 219134 b	Gillon et al. (2017)	Gillon et al. (2017)

HD 39091 c	–	Huang et al. (2018)

GJ 9827 b	Rodriguez et al. (2018)	Rice et al. (2019)

HD 3167 b	–	Christiansen et al. (2017)

K2-141 b	Malavolta et al. (2018)	Malavolta et al. (2018)

CoRoT-7 b	Stassun et al. (2017)	Barros et al. (2014)

GJ 1214 b	Harpsoe et al. (2013)	Harpsoe et al. (2013)

K2-291 b	Kosiarek et al. (2019)	Kosiarek et al. (2019)

K2-131 b	–	Dai et al. (2017)

K2-265 b	Lam et al. (2018)	Lam et al. (2018)

Kepler-11 e	Hadden & Lithwick (2017)	Hadden & Lithwick (2017)

Kepler-11 d	Lissauer et al. (2013)	Hadden & Lithwick (2017)

WASP-47 e	Vanderburg et al. (2017)	Vanderburg et al. (2017)

Kepler-454 b	Stassun et al. (2017)	Gettel et al. (2016)

LHS 1140 b	Ment et al. (2018)	Ment et al. (2018)

Kepler-36 c	Carter et al. (2012)	Hadden & Lithwick (2017)

HD 97658 b	Stassun et al. (2017)	Van Grootel et al. (2014)

HD 15337 b	Gandolfi et al. (2019)	Dumusque et al. (2019)

K2-216 b	Persson et al. (2018)	Persson et al. (2018)

Kepler-19 b	Malavolta et al. (2018)	Malavolta et al. (2018)

55 Cnc e	Demory et al. (2016)	Crida et al. (2018)

HD 15337 c	–	Dumusque et al. (2019)

HD 213885 b	–	Espinoza et al. (2020)

EPIC 220 674 823 b	–	Sinukoff et al. (2017)

Kepler-107 c	Bonomo et al. (2019)	Bonomo et al. (2019)

K2-285 b	Palle et al. (2019)	Palle et al. (2019)

Kepler-20 b	Buchhave et al. (2016)	Buchhave et al. (2016)

HD 3167 c	–	Christiansen et al. (2017)

Kepler-94 b	Marcy et al. (2014)	Marcy et al. (2014)*

K2-180 b	–	Korth et al. (2019)

HIP 116454 b	Stassun et al. (2017)	Vanderburg et al. (2017)

Kepler-20 c	Buchhave et al. (2016)	Buchhave et al. (2016)

Kepler-95 b	Marcy et al. (2014)	Marcy et al. (2014)*

KOI-94 e	Weiss et al. (2013)	Masuda et al. (2013)*

WASP-47 d	Vanderburg et al. (2017)	Vanderburg et al. (2017)

GJ 3470 b	Awiphan et al. (2016)	Awiphan et al. (2016)

Kepler-48 c	Marcy et al. (2014)	Marcy et al. (2014)*

K2-263 b	Mortier et al. (2018)	Mortier et al. (2018)

Kepler-18 d	Cochran et al. (2011)	Hadden & Lithwick (2017)

K2-24 c	–	Petigura et al. (2018)

K2-285 c	Petigura et al. (2018)	Petigura et al. (2018)

Kepler-131 b	Marcy et al. (2014)	Marcy et al. (2014)*

K2-32 b	Petigura et al. (2017)	Petigura et al. (2017)

HD 219666 b	Esposito et al. (2018)	Esposito et al. (2018)

K2-110 b	Osborn et al. (2017)	Osborn et al. (2017)

Kepler-10 c	Dumusque et al. (2014)	Dumusque et al. (2014)

K2-24 b	Petigura et al. (2018)	Petigura et al. (2018)

GJ 143 b	–	Dragomir et al. (2019)

GJ 436 b	Turner et al. (2016)	Turner et al. (2016)

HD 21749 b	–	Dragomir et al. (2019)

Kepler-4 b	Borucki et al. (2010)	Borucki et al. (2010)

HD 119130 b	Luque et al. (2018)	Luque et al. (2018)

Kepler-25 c	Marcy et al. (2014)	Marcy et al. (2014)*

Kepler-411 b	Sun et al. (2019)	Sun et al. (2019)

Kepler-411 c	Sun et al. (2019)	Sun et al. (2019)

HAT-P-11 b	Yee et al. (2018)	Allart et al. (2018)

K2-27 b	Petigura et al. (2017)	Petigura et al. (2017)

WASP-166 b	–	Hellier et al. (2017)

HD 89345 b	Yu et al. (2018)	Yu et al. (2018)

WASP-139 b	Hellier et al. (2017)	Hellier et al. (2017)

WASP-107 b	–	Anderson et al. (2017)

HATS-7 b	Bakos et al. (2015)	Bakos et al. (2015)

Kepler-35 b	Welsh et al. (2012)	Welsh et al. (2012)

WASP-156 b	Demangeon et al. (2017)	Demangeon et al. (2017)

K2-55 b	Crossfield et al. (2016)	Dressing et al. (2018)

Kepler-101 b	Bonomo et al. (2014)	Bonomo et al. (2014)*

HAT-P-48 b	–	Bakos et al. (2016)

KELT-11 b	Beatty et al. (2017)	Beatty et al. (2017)

K2-261 b	Johnson et al. (2018)	Brahm et al. (2019)

WASP-127 b	Lam et al. (2017)	Lam et al. (2017)

K2-108 b	Petigura et al. (2017)	Petigura et al. (2017)

HAT-P-18 b	Hartman et al. (2011)	Esposito et al. (2014)

HD 221416 b	Huber et al. (2019)	Huber et al. (2019)

HAT-P-47 b	–	Bakos et al. (2016)

HAT-P-12 b	Hartman et al. (2009)	Huber et al. (2019)

CoRoT-8 b	Bordé et al. (2010)	Bordé et al. (2010)

Kepler-34 b	Welsh et al. (2012)	Welsh et al. (2012)

Kepler-425 b	–	Bonomo et al. (2017)*

NGTS-5 b	–	Eigmüller et al. (2019)

HATS-5 b	Zhou et al. (2014)	Zhou et al. (2014)

WASP-29 b	Stassun et al. (2017)	Gibson et al. (2013)

WASP-69 b	Stassun et al. (2017)	Anderson et al. (2013)

HATS-43 b	–	Brahm et al. (2019)

WASP-131 b	Hellier et al. (2017)	Hellier et al. (2017)

WASP-117 b	Stassun et al. (2017)	Lendl et al. (2014)

WASP-160 b	–	Lendl et al. (2019)

WASP-39 b	Faedi et al. (2011)	Faedi et al. (2011)

WASP-126 b	Maxted et al. (2016)	Maxted et al. (2016)

Kepler-427 b	–	Bonomo et al. (2017)*

HAT-P-19 b	Hartman et al. (2011)	Hartman et al. (2011)

WASP-181 b	–	Turner et al. (2019)

WASP-21 b	Bouchy et al. (2010)	Bouchy et al. (2010)

WASP-83 b	Hellier et al. (2015)	Hellier et al. (2015)

HAT-P-51 b	Hartman et al. (2015)	Hartman et al. (2015)

WASP-151 b	Demangeon et al. (2017)	Demangeon et al. (2017)

WASP-20 b	Anderson et al. (2015)	Bonomo et al. (2017)

K2-287 b	Jordán et al. (2019)	Jordán et al. (2019)

HATS-6 b	Hartman et al. (2015)	Hartman et al. (2015)

HD 149026 b	Stassun et al. (2017)	Bonomo et al. (2017)

Kepler-16 b	Doyle et al. (2011)	Doyle et al. (2011)

K2-295 b	–	Smith et al. (2018)

EPIC 220 501 947 b	–	Smith et al. (2019)

Kepler-426 b	–	Bonomo et al. (2017)

HAT-P-44 b	Hartman et al. (2014)	Hartman et al. (2014)

Qatar-8 b	–	Alsubai et al. (2019)

WASP-63 b	Stassun et al. (2017)	Hellier et al. (2012)

Notes. It compares the reference picked by the NASA Exoplanet Archive (if available) and our selected reference. Where the radius has been obtained from Berger et al. (2018) (due to smaller uncertainty) it is indicated with an asterisk.

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