The COBREX archival survey: Improved constraints on the occurrence rate of wide-orbit substellar companions - I. A uniform re-analysis of 400 stars from the GPIES survey

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Table A.2

Adopted ages for the YMG of interest.

YMG	Acronym	Age	Source	YMG	Acronym	Age	Source
AB Doradus	ABDMG	$149_{- 49}^{+ 31}$ $149_{ - 49}^{ + 31}$	1	Lower Centaurus-Crux	LCC	15±3	6
Argus	ARG	45 ± 5	2	Tucana Horologium Ass.	THA	$45_{- 4}^{- 5}$ $45_{ - 4}^{ - 5}$	3
β Pic MG	BPMG	24 ± 5	1	TW Hya Ass.	TWA	10±3	3
Carina	CAR	$45_{- 7}^{+ 11}$ $45_{ - 7}^{ + 11}$	3	Upper Centaurus-Lupus	UCL	16±2	6
Carina-Near	CARN	200 ± 50	4	Upper Scorpius	USCO	10±3	6
Columba	COL	$42_{- 4}^{+ 6}$ $42_{ - 4}^{ + 6}$	3	Volans-Carina Ass.	VCA	$87_{- 9}^{+ 5}$ $87_{ - 9}^{ + 5}$	7
ϵ Cha	EPSC	${3.7}_{- 1.4}^{+ 4.6}$ $3.7_{ - 1.4}^{ + 4.6}$	5

Notes. Sources: 1: Desidera et al. (2021); 2: Zuckerman (2019); 3: Bell et al. (2015); 4: Zuckerman et al. (2006), assuming a relative 25% error; 5: Murphy et al. (2013); 6: Pecaut & Mamajek (2016); 7: Gagné et al. (2018a).

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