Table 4.
Summary of the total collection of 1536 members of IC1396 found in the literature.
| Reference | Methods | Number |
|---|---|---|
| of sources | ||
| Marschall & van Altena (1987) | Astrometric data | 31 |
| Kun & Pasztor (1990) | Hα emission/optical-IR photmetry | 18 |
| Sicilia-Aguilar et al. (2004, 2005, 2006a,b | Near- and mid-IR observations/optical photometry/spectroscopy/ | 435 |
| 2010, 2013) | IR excess (Spitzer/2MASS) | |
| Barentsen et al. (2011) | Photometric Hα survey | 101 |
| Mercer et al. (2009) | X-ray and near-IR observations | 29 |
| Morales-Calderón et al. (2009) | Mid-IR variability | 14 |
| Getman et al. (2012), Getman private com. | X-ray emission | 189 |
| Meng et al. (2019) | Near-IR variability | 298 |
| Nakano et al. (2012) | Wide-field emission-line survey | 408 |
| Rebull et al. (2013) | Spitzer mid-IR data | 13 |
Notes. Several objects have been detected in more than one reference, but we list here the reference providing the most accurate coordinates, which are also the ones listed for sources that do not have Gaia counterparts. The complete collection of 1536 known members (plus two spectroscopic members added from this work) is listed in Table A.1.
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