Table 3
Details of the astrometric fits for all detected sources.
d a |
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Epoch | [arcsec] | π fit |
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RA (J2000) | Dec (J2000) | (MJD) | S/N | [pc] | [mas] | [mas yr-1] | [mas yr-1] | ||
|
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M15A | 21:29:58.246512(4) | 12:10:01.2339(1) | 55 146 | 24 | 1.2 (3) | −0.02 (10) | −0.54 (14) | −4.33 (25) | 1.4 |
0.06 (1) | −0.56 (14) | −4.34 (25) | 1.3 | ||||||
M15C | 21:30:01.203493(7) | 12:10:38.1592(2) | 55 146 | 15 | 56.0 (3) | 0.22(17) | −0.75 (9) | −3.52 (13) | 0.7 |
2.79 (1) | −0.76 (10) | −3.53 (15) | 0.9 | ||||||
AC211 | 21:29:58.312403(4) | 12:10:02.6740(2) | 55 871 | 24 | 1.5 (3) | 0.17(7) | −0.46 (8) | −4.31 (20) | 3.4 |
0.07 (1) | −0.49 (8) | −4.32 (20) | 3.4 | ||||||
S1 | 21:29:51.9034555(4) | 12:10:17.13240(1) | 55 352 | 287 | 95.5 (3) | 0.04(25) | +0.06 (28) | +0.53 (59) | 2749 |
4.77 (1) | +0.05 (30) | +0.53 (62) | 3034 | ||||||
S2 | 21:30:02.085700(8) | 12:09:04.2203(2) | 55 871 | 17 | 79.2 (3) | 0.45(8) | −0.07 (13) | −1.26 (29) | 2.9 |
3.95 (1) | −0.05 (8) | −1.27 (17) | 1.0 |
Notes. For the proper motion results and the goodness-of-fit, , the results for a fixed parallax π = 0.1 and for the fitted parallax, πfit, are listed. The positions listed are for the indicated MJDs (epochs with the best S/N). For S1 the positions were measured relative to the phase calibrator while the positions of the remaining sources were measured relative to S1.
Distance (in arcsec and pc) from the assumed cluster center at RA = 212958330 ± 0
013, Dec = 12°10′01.̋2 ±0.̋2 (Goldsbury et al. 2010).
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