Table 8
Likely counterparts of the X-ray sources listed in Table 7.
ID | NVSS(a) | 2MASS | USNO B1.0(b) | SDSS DR7 | |||||
Name | S [mJy] | Name | K | Name | R | Name | g | Type | |
|
|||||||||
A | 003000+072255 | 47(2) | – | – | 0973-0005315 | 20.0m | J003000.24+072254.7 | 20.3m | 6 |
B | – | – | – | – | 0973-0005428 | 20.4m | J003017.75+072140.6 | 19.6m | 6 |
C | – | – | – | – | – | – | J003022.22+072621.3 | 21.4m | 6 |
D | – | – | 00302977+0720101 | 15.3m | 0973-0005481 | 18.9m | J003029.77+072010.3 | 18.5m | 3 |
0973-0005484 | 19.3m | ||||||||
E | – | – | – | – | – | – | J003049.61+072313.5 | 21.0m | 6 |
F | – | – | 00305500+0723233 | 15.7m | 0973-0005560 | 18.2m | J003054.80+072323.1 | 20.7m | 6 |
J003055.00+072323.2 | 18.5m | 6 | |||||||
G | 003119+072456 | 11.6(6) | – | – | 0974-0005617 | 18.6m | J003119.71+072453.5 | 17.4m | 6 |
Notes. Scans ranging from radio (NVSS) to infrared (2MASS) and optical (USNO and SDSS) wavelength bands are given. The table lists the object’s name and the catalogued flux or apparent magnitude. Here, parentheses indicate the corresponding error on the last decimal. Based on photometric morphology, SDSS provides a separation between galaxy-like (3) and star-like objects (6), see Lupton et al. (2001).
The column lists R2. If not available, R1 or B1 is given instead (see Monet et al. 2003, and references therein).
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