Table 1.
Summary of the sample.
XID | XID | CID | RA | Dec | zspec |
---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) |
34 | 42 | 326 (a) |
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![]() |
2.940 (b) |
262 | 337 | 5479 |
![]() |
![]() |
3.660 |
403 | 539 | 273 |
![]() |
![]() |
4.755 |
412 | 551 | 6294 |
![]() |
![]() |
3.700 |
490 | 666 | 9834 |
![]() |
![]() |
2.578 |
546 | 746 | 10578 |
![]() |
![]() |
3.064 |
Notes. (1) X-ray ID in Xue et al. (2011) catalog (4 Ms). (2) X-ray ID in Luo et al. (2017) catalog (7 Ms). (3) CANDELS ID in Grogin et al. (2011) catalog. (4) J2000 right ascension and (5) declination. (6) Spectroscopic redshift as given by Luo et al. (2017).
This source is not included in CANDELS, thus the ID from GEMS (Häussler et al. 2007) is reported.
Using the CIV, HeII and NV lines in the UV-spectrum we derive a better estimate of zspec = 2.937 (see Sect. 4).
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