Table 2
Aperture photometry corrected for extinction in the Milky Way of the two galaxies and of the star-forming regions.
| ID | Distance | u | g | i | z | NUV | FUV | |
| (arcsec) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | |
|
|
||||||||
| VCC 1249 | 0 | 15.60 ± 0.03 | 14.73 ± 0.03 | 14.19 ± 0.03 | 14.11 ± 0.03 | 17.46 ± 0.15 | 18.68 ± 0.18 | |
| M 49 | 334.0 | 10.28 ± 0.03 | 8.83 ± 0.03 | 7.81 ± 0.03 | 7.49 ± 0.03 | 13.91 ± 0.15 | 14.82 ± 0.17 | |
| C1 | 151.4 | 21.33 ± 0.04 | 21.31 ± 0.04 | 21.53 ± 0.04 | 22.12 ± 0.04 | 20.77 ± 0.16 | 20.80 ± 0.29 | |
| C2 | 126.1 | 21.31 ± 0.04 | 21.41 ± 0.04 | 21.83 ± 0.04 | 22.51 ± 0.05 | 21.52 ± 0.16 | 21.09 ± 0.32 | |
| C3 | 119.4 | 23.53 ± 0.06 | 23.27 ± 0.06 | 23.15 ± 0.05 | 23.00 ± 0.06 | – | – | |
| C4 | 137.9 | 23.09 ± 0.05 | 22.56 ± 0.06 | 22.33 ± 0.04 | 22.28 ± 0.04 | (23.04 ± 0.15) | (22.48 ± 0.40) | |
| C5 | 156.4 | 22.91 ± 0.05 | 22.69 ± 0.05 | 23.00 ± 0.05 | 23.28 ± 0.05 | – | – | |
| C6 | 70.7 | 21.92 ± 0.04 | 21.94 ± 0.04 | 22.31 ± 0.04 | 22.10 ± 0.04 | 21.37 ± 0.16 | 21.17 ± 0.33 | |
| C7 | 55.1 | 23.17 ± 0.06 | 22.87 ± 0.06 | 21.75 ± 0.04 | 21.22 ± 0.03 | – | – | |
| C8 | 61.1 | 22.31 ± 0.06 | 22.15 ± 0.06 | 22.14 ± 0.05 | 21.69 ± 0.04 | 21.43 ± 0.16 | 20.98 ± 0.31 | |
| C12 | 5.8 | 22.17 ± 0.06 | 21.48 ± 0.07 | 21.11 ± 0.06 | 21.10 ± 0.05 | – | – | |
| C17 | 19.2 | 23.94 ± 0.09 | 22.81 ± 0.16 | 22.03 ± 0.06 | 22.08 ± 0.06 | – | – | |
Notes. The photometry of M 49 is computed within an aperture of about 5.7 arcmin radius (or ~ 1.6 Re; Ferrarese et al. 2006). (1) Naming of the star-forming regions as in Lee et al. (1997); (2) projected distance from the center of VCC 1249. The photometric uncertainties are the quadratic sum of the ZP error and the Poisson error.
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