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Table 6.
Samples used with Gaia EDR3 data from our IC1396 stellar member analysis.
| Sample | Nr. sources | Criteria | Code (*) |
|---|---|---|---|
| KM plus 2 new spectroscopic members | 1538 | Listed in the literature +Spectroscopy | KM |
| KM used for the maximum likelihood analysis | 578 | Fractional parallax error (f < 0.25) | – |
| RUWE < 1.4. | |||
| Parallax (0.6–1.6 mas) | |||
| New members obtained from the Mahalanobis distance | 334 | Errors magnitude < 0.05 mag | NM |
| Errors proper motion < 0.1 mas yr−1 | |||
| Age cut (0.1–10 Myr) |
Notes. (*)The code will be used throughout the paper for a better understanding of the sample used in the analysis.
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