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Table C.1

Stellar properties and coordinates of the targets included in our sample.

Source RA (J2000) Dec (J2000) Stellar Mass (M) d (pc)
Sz 131 16:00:49.414 −41:30:04.263 0.31 160.6
J15450634-3417378 1 15:45:06.322 −34:17:38.332 158.0
J16081497-3857145 16:08:14.960 −38:57:14.910 0.06 158.8
J16085324-3914401 16:08:53.227 −39:14:40.553 0.29 163.0
Sz 72 15:47:50.608 −35:28:35.779 0.14 160.5
Sz 103 16:08:30.254 −39:06:11.538 0.19 157.1
Sz 97 16:08:21.787 −39:04:21.860 0.19 157.3
Sz 117 16:09:44.348 −39:13:30.555 0.23 156.9
Sz 113 16:08:57.786 −39:02:23.260 0.13 160.5
J16134410-3736462 16:13:44.082 −37:36:46.598 0.96 158.5
J16000060-4221567 16:00:00.584 −42:21:57.203 0.15 159.4
J16085529-3848481 16:08:55.275 −38:48:48.551 0.07 155.6
J16002612-4153553 16:00:26.099 −41:53:55.782 0.1 163.2
Sz 106 16:08:39.743 −39:06:25.701 0.5 158.7
Sz 104 16:08:30.798 −39:05:49.238 0.1 159.8
Sz 112 16:08:55.513 −39:02:34.359 0.1 159.3
J16095628-3859518 16:09:56.281 −38:59:51.973 0.06 157.1
Sz 110 16:08:51.553 −39:03:18.087 0.2 157.5

These values are taken from Manara et al. (2023); Alcalá et al. (2014, 2017). The uncertainties on stellar masses are 0.1 dex (Alcalá et al. 2017).

1 this source isn’t included in the subsequent analysis.

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