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Table 2.

GALEX, SDSS, and 2MASS NIR photometry of 53 sample GCs in M 31.

Object FUV NUV u g r i z J H Ks
(mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
B289 20.73 19.82 … … … … … 15.19 15.24 15.88
0.05 0.02 … … … … … 0.04 0.05 0.09
B290 23.81 22.43 … … … … … 16.09 15.9 15.9
0.34 0.1 … … … … … 0.06 0.06 0.06
B295 21.38 20.44 18.25 16.96 16.44 16.16 15.99 15.79 15.99 16.52
0.11 0.01 0.04 0.01 0.01 0.01 0.03 0.06 0.08 0.14
B301 23.3 22.14 19.18 17.54 16.82 16.49 16.24 15.94 15.57 15.97
0.24 0.04 0.06 0.02 0.01 0.01 0.02 0.05 0.05 0.07
B400 22.45 21.16 18.54 16.89 16.24 15.88 15.74 15.41 15.38 15.56
0.17 0.05 0.04 0.01 0.01 0.01 0.02 0.03 0.04 0.05
B468 23.26 22.88 19.85 18.3 17.69 17.36 17.23 17.17 16.88 16.25
0.33 0.2 0.11 0.03 0.02 0.02 0.06 0.14 0.13 0.1
B514 20.61 19.54 17.73 16.13 15.54 15.25 15.13 15.08 14.68 15.47
0.06 0.03 0.03 0.01 0.01 0.01 0.01 0.04 0.04 0.07
SDSS-D … 20.55 19.29 17.9 17.34 17.03 17.03 17.06 16.66 17.27
… 0.09 0.07 0.02 0.02 0.02 0.04 0.11 0.1 0.18
EXT8 … 18.69 16.99 15.84 15.51 15.15 14.97 14.89 14.84 15.46
… 0.06 0.02 0.01 0.01 0.01 0.01 0.02 0.03 0.05
G001 19.09 18.25 16.04 14.22 … 13.26 13.04 12.71 12.51 12.85
0.02 0.01 0.01 0.01 … 0.01 0.01 0.01 0.01 0.01

Notes. Column 1 gives the GC names. Columns 2–11 present the magnitudes from GALEX, SDSS, and 2MASS NIR observations. All magnitudes are in the AB magnitude system. The 1σ magnitude uncertainties from DAOPHOT are listed for each object on the second line for the corresponding passbands. This table is available in its entirety in machine-readable form at the CDS.

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