Table A.1
Area covered and candidate members obtained in previous works of literature.
| Work | Method | No. of identified members | Radius (degree) | RA (J2000) | DEC (J2000) |
|---|---|---|---|---|---|
| Contreras et al. (2002) | Optical Spectroscopy | 66 | 0.5 | 21:39:09.89 | +57:30:56.07 |
| Sicilia-Aguilar et al. (2006b) | Optical Spectroscopy | 172 | 0.6 | 21:37:54.41 | +57:33:15.32 |
| Sicilia-Aguilar et al. (2013) | Optical Spectroscopy | 67 | 0.25 | 21:37:03.17 | +57:29:05.43 |
| Reach et al. (2004) | Spitzer MIR | 17 | 0.12 | 21:36:33.09 | +57:29:13.83 |
| Sicilia-Aguilar et al. (2006a) | Spitzer MIR | 57 | 0.15 | 21:36:39.73 | +57:29:28.45 |
| Morales-Calderón et al. (2009) | Spitzer MIR | 69 | 0.15 | 21:36:36.32 | +57:29:54.78 |
| Rebull et al. (2013) | Spitzer MIR | 14 | 0.50 | 21:33:28.23 | +58:04:59.51 |
| Barentsen et al. (2011) | Hα emission | 158 | 1.5 | 21:40:00.43 | +57:26:42.60 |
| Nakano et al. (2012) | Hα emission | 639 | 1.4 | 21:39:48.76 | +57:30:31.56 |
| Getman et al. (2007) | X-ray emission | 24 | 0.1 | 21:40:36.73 | +58:15:37.51 |
| Mercer et al. (2009) | X-ray emission | 39 | 0.15 | 21:38:54.67 | +57:29:17.61 |
| Getman et al. (2012) | X-ray emission | 457 | 0.25 | 21:37:05.85 | +57:32:30.06 |
| Silverberg et al. (2021) | NIR, MIR and X-ray | 421 | 0.37 | 21:33:59.30 | +57:29:30.76 |
| Sicilia-Aguilar et al. (2004) | Optical photometry, spectroscopy and variability | 53 | 0.35 | 21:39:06.36 | +57:32:56.86 |
| Sicilia-Aguilar et al. (2005) | Optical/2MASS photometry, spectroscopy, and variability | 249 | 0.65 | 21:39:28.19 | +57:31:51.63 |
| Sicilia-Aguilar et al. (2010) | Optical photometry and spectroscopy | 102 | 0.50 | 21:38:08.05 | +57:31:02.52 |
| Meng et al. (2019) | NIR variability | 359 | 0.60 | 21:35:35.94 | +57:40:02.68 |
| Cantat-Gaudin et al. (2018) | Gaia-DR2 | 460 | 0.7 | 21:38:58.80 | +57:30:50.40 |
| Pelayo-Baldárrago et al. (2023) | Gaia-EDR3 | 334 | 2.0 | 21:38:56.86 | +57:44:35.81 |
| Das et al. (2023) | Gaia-DR3 | 1243 | 1.5 | 21:40:39.28 | +57:49:15.51 |
| Gupta et al. (2024) | Subaru-HSC | 458 | 0.37 | 21:38:57.62 | +57:29:20.54 |
Notes. The methods given in column 2 present the dominant mechanisms of the respective works. For Pelayo-Baldárrago et al. (2023), we used sources detected only from the Gaia-EDR3 dataset. Complete details of the methods used in the studies can be found in the respective papers.
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