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Table 1

Basic properties of young members and photometric candidates in σ Orionis from Peña Ramírez et al. (2012) that are studied in this work.

Resolvable Simbad ID RA Dec Feat. a IR Excess J b Var? c Comments
hh:mm:ss.s dd:mm:ss (mag) (MJup)

Variability and deep image analysis

Mayrit 258337 05:38:38.1 –02:32:03 RV, g, d Y(4.5,  8.0, 12.0) 15.07 56 Y SB1, Known var.
Mayrit 396273 05:38:18.3 –02:35:39 RV, g N 15.29 47 Y
Mayrit 379292 05:38:21.4 –02:33:36 RV, Li, g, d Y(12.0) 15.31 47 ...
[MJO2008] J053852.6–023215 05:38:52.6 –02:32:15 RV, g N 16.18 29 ...
[BNM2013] 90.02 782 05:39:12.9 –02:24:54 Hα N 16.68 24 ...
[BNM2013] 90.02 1834 05:39:00.3 –02:37:06 Hα, d Y(4.5, 8.0) 17.19 19 ...
[BZR99] S Ori 51 05:39:03.2 –02:30:20 g N 17.16 19 ...
[BZR99] S Ori 50 05:39:10.8 –02:37:15 ... N 17.47 17 ... Photometric cand.
[BZR99] S Ori 58 05:39:03.6 –02:25:36 Hα, d Y(4.5, 8.0) 18.42 11 ...

Deep image analysis only

[BZR99] S Ori 60 05:39:37.5 –02:30:42 Hα, d Y(8.0) 19.02 8 ...
[BZR99] S Ori 62 05:39:42.1 –02:30:32 Hα N 19.14 8 ...
[BZR99] S Ori 65 05:38:26.1 –02:23:05 d Y(4.5, 8.0) 20.30 5 ...

Notes.

(a)

RV: radial velocity consistent with systemic cluster velocity, g: low-gravity atmosphere, Li: lithium absorption, Hα: strong, broad Hα emission, d: presence of a disc.

(b)

J-band magnitude from Peña Ramírez et al. (2012).

(c)

Variability was identified from the analysis in this work.

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