Table 2
NEWFIRM and VVV counterparts of the 20 Chandra sources identified through near-IR spectroscopy in this study.
NEWFIRM | VVV | |||||||||
|
||||||||||
No. | J | H | Ks | VVV ID. | Dist. | Z | Y | J | H | Ks |
(mag) | (mag) | (mag) | (′′) | (mag) | (mag) | (mag) | (mag) | (mag) | ||
|
||||||||||
38 | 15.29 ± 0.07 | 11.92 ± 0.10 | 10.13 ± 0.06 | 515727245968 | 0.12 | – | 19.33 ± 0.15 | 15.21 ± 0.01 | 11.99 ± 0.01 | Sat. |
78 | 16.43 ± 0.07 | 15.45 ± 0.10 | 14.99 ± 0.09 | 515726911773 | 0.06 | 17.02 ± 0.01 | 16.74 ± 0.02 | 16.46 ± 0.01 | 15.77 ± 0.04 | 15.38 ± 0.02 |
158 | 12.96 ± 0.03 | 11.39 ± 0.05 | 10.58 ± 0.05 | 515727009565 | 0.06 | 16.44 ± 0.01 | 14.88 ± 0.01 | 12.96 ± 0.01 | 11.30 ± 0.01 | 10.58 ± 0.01 |
239 | 15.74 ± 0.07 | 13.60 ± 0.08 | 12.12 ± 0.06 | 515720865399 | 0.13 | – | 18.42 ± 0.08 | 15.65 ± 0.01 | 13.48 ± 0.01 | 12.16 ± 0.01 |
396 | 15.48 ± 0.05 | 13.18 ± 0.10 | 11.99 ± 0.07 | 515720906266 | 0.96 | – | 18.16 ± 0.06 | 15.49 ± 0.01 | 13.19 ± 0.01 | 12.19 ± 0.01 |
437 | 14.51 ± 0.04 | 12.85 ± 0.06 | 12.01 ± 0.08 | 515720093751 | 0.42 | 17.53 ± 0.02 | 15.97 ± 0.01 | 14.31 ± 0.01 | 12.82 ± 0.01 | 12.00 ± 0.01 |
694 | 12.53 ± 0.05 | 11.75 ± 0.07 | 10.26 ± 0.06 | 515720390344 | 0.44 | 13.56 ± 0.01 | 13.17 ± 0.01 | 13.29 ± 0.01 | 12.70 ± 0.01 | 12.26 ± 0.01 |
750 | No Cov. | No Cov. | No Cov. | 515720338856 | 0.22 | 15.08 ± 0.01 | 15.06 ± 0.01 | 14.91 ± 0.01 | 14.64 ± 0.01 | 14.27 ± 0.01 |
881 | No Cov. | No Cov. | No Cov. | 515725172945 | 0.66 | Sat. | Sat. | Sat. | Sat. | Sat. |
1059 | No Cov. | No Cov. | No Cov. | 515725290815 | 0.30 | Sat. | Sat. | Sat. | Sat. | Sat. |
1128 | No Cov. | No Cov. | No Cov. | 515725286315 | 0.08 | 14.71 ± 0.01 | 13.63 ± 0.01 | 12.53 ± 0.01 | 11.48 ± 0.01 | 10.76 ± 0.01 |
1168 | No Cov. | No Cov. | No Cov. | 515720689720 | 0.26 | 12.75 ± 0.01 | 12.63 ± 0.01 | 12.23 ± 0.01 | 12.14 ± 0.01 | 11.83 ± 0.01 |
1203 | No Cov. | No Cov. | No Cov. | 515720696577 | 0.38 | Sat. | Sat. | Sat. | Sat. | Sat. |
1278 | No Cov. | No Cov. | No Cov. | 515721533405 | 0.18 | – | – | 17.72 ± 0.06 | 13.61 ± 0.01 | 11.26 ± 0.01 |
1279 | No Cov. | No Cov. | No Cov. | 515721039612 | 0.30 | – | – | 16.02 ± 0.01 | 12.19 ± 0.04 | Sat. |
1326 | No Cov. | No Cov. | No Cov. | 515725424702 | 0.20 | 17.59 ± 0.02 | 16.28 ± 0.01 | 14.56 ± 0.01 | 12.71 ± 0.01 | 11.48 ± 0.01 |
1358 | No Cov. | No Cov. | No Cov. | 515725732674 | 0.13 | Sat. | 11.45 ± 0.01 | 10.96 ± 0.01 | 10.46 ± 0.01 | 10.18 ± 0.01 |
1374 | No Cov. | No Cov. | No Cov. | 515725467960 | 0.17 | 14.27 ± 0.01 | 13.84 ± 0.01 | 13.36 ± 0.01 | 12.56 ± 0.01 | 12.38 ± 0.01 |
1379 | No Cov. | No Cov. | No Cov. | 515725581165 | 0.38 | Sat. | Sat. | Sat. | Sat. | Sat. |
1408 | No Cov. | No Cov. | No Cov. | 515725521664 | 0.41 | Sat. | Sat. | Sat. | Sat. | Sat. |
Notes. Column 1: source number in our catalogue. Columns 2 to 4: NEWFIRM J, H, and Ks magnitudes. Column 5: IDs of the VVV counterparts. Column 6: distance (′′) of the VVV counterparts to the corresponding X-ray sources. Columns 7 to 11: VVV Z, Y, J, H, and Ks magnitudes. “Sat.” means that the source is detected but saturated, while a “–” means that the source is not detected in the corresponding filter.
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