Free Access

Table 3

Details of the astrometric fits for all detected sources.

d a
Epoch [arcsec] π fit
RA (J2000) Dec (J2000) (MJD) S/N [pc] [mas] [mas yr-1] [mas yr-1]

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.

(a)

Distance (in arcsec and pc) from the assumed cluster center at RA = 212958330 ± 0013, Dec = 12°1001.̋2 ±0.̋2 (Goldsbury et al. 2010).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.