Table A.2.
Young stellar clusters: members identified.
| RA | DEC | pmRA | pmDEC | π | BP | RP | G | dcent | PROB | H-K | J-H | disk? |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| ° | ° | mas yr−1 | mas yr−1 | mas | mag | mag | mag | ° | ... | mag | mag | ... |
| NGC 1333 | ||||||||||||
| 55.6003 | 32.1583 | 6.96 ± 0.08 | -9.56 ± 0.06 | 3.32 ± 0.09 | 18.651 ± 0.023 | 15.577 ± 0.006 | 16.846 ± 0.003 | 2.9348 | 1.000 | 0.26 ± 0.04 | 0.71 ± 0.04 | |
| 52.3399 | 31.3528 | 7.64 ± 0.06 | -9.59 ± 0.05 | 3.41 ± 0.06 | 18.149 ± 0.015 | 14.594 ± 0.005 | 15.957 ± 0.003 | 0.0567 | 0.993 | 0.35 ± 0.04 | 0.67 ± 0.04 | |
| 52.1815 | 31.2934 | 7.27 ± 0.13 | -9.74 ± 0.10 | 3.35 ± 0.12 | 19.312 ± 0.088 | 15.196 ± 0.034 | 16.805 ± 0.011 | 0.0998 | 0.980 | 0.82 ± 0.03 | 1.26 ± 0.04 | |
| IC 348 | ||||||||||||
| 56.1558 | 32.1032 | 4.36 ± 0.05 | -6.38 ± 0.03 | 3.10 ± 0.05 | 16.683 ± 0.013 | 14.011 ± 0.005 | 15.205 ± 0.003 | 0.0962 | 1.000 | 0.28 ± 0.03 | 0.94 ± 0.03 | |
| 55.3089 | 31.9961 | 4.58 ± 0.02 | -6.08 ± 0.02 | 3.28 ± 0.02 | 12.590 ± 0.003 | 11.151 ± 0.004 | 11.945 ± 0.003 | 0.6569 | 1.000 | 0.18 ± 0.03 | 0.34 ± 0.03 | |
| 56.0903 | 32.1069 | 4.70 ± 0.07 | -6.15 ± 0.05 | 3.12 ± 0.08 | 17.776 ± 0.024 | 14.688 ± 0.009 | 15.984 ± 0.003 | 0.0551 | 1.000 | 0.29 ± 0.03 | 0.93 ± 0.03 | |
| NGC 1893 | ||||||||||||
| 80.6932 | 33.4024 | -0.60 ± 0.03 | -1.54 ± 0.02 | 0.30 ± 0.03 | 14.938 ± 0.003 | 13.667 ± 0.004 | 14.395 ± 0.003 | 0.0486 | 1.000 | 0.30 ± 0.04 | 0.50 ± 0.04 | |
| 80.6866 | 33.4435 | -0.50 ± 0.03 | -1.37 ± 0.02 | 0.34 ± 0.02 | 11.412 ± 0.003 | 11.000 ± 0.004 | 11.274 ± 0.003 | 0.0310 | 0.998 | 0.03 ± 0.03 | 0.05 ± 0.03 | |
| 80.6833 | 33.4407 | -0.50 ± 0.03 | -1.33 ± 0.02 | 0.37 ± 0.03 | 10.332 ± 0.003 | 9.940 ± 0.004 | 10.204 ± 0.003 | 0.0338 | 0.996 | 0.05 ± 0.03 | 0.02 ± 0.03 | |
| ... | ||||||||||||
Notes. Columns 1 to 10 list the Gaia EDR3 coordinates, proper motions, parallax, BP, RP and G magnitudes, angular distance to the center of the cluster, and membership probability (ordered from higher to lower) of each member identified (PROB > 0) within FOV20pc. The members within FOV2pc can be retrieved from dcent and the corresponding angular radius (see Col. 9 in Table A.1). Columns 11 and 12 list the 2MASS colors, when available. Objects identified as disk stars or potential disk stars based on the JHK colors and error bars are tagged with “yes” and “yes?” in the last column. The absence of such tags does not necessarily mean that the star is diskless (Sects. 2.2 and 4.2). Only the three first rows for the three first clusters are shown. A complete version of this table is available at the CDS.
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