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Table 2

Photometric and spectroscopic properties of the 22 AGN candidates.

ID RA Dec zphot zspec C H M 1450 log FX log LX A Previous catalogues
erg/cm2/s erg/s
273 53.1220463 −27.9387409 4.49 4.7621 c 23.96 −21.37 −15.97 43.80 2 M208, X403
4285 53.1664941 −27.8716803 4.28 cf 25.57 −20.22 −16.46 42.90 3 –
4356 53.1465968 −27.8709872 4.70 cf 26.36 −18.44 −16.38 43.40 4 M70437, L306, X485
4952 53.1605007 −27.8649890 4.32 c 25.47 −20.20 −16.50 42.90 3 –
5375 53.1026292 −27.8606307 4.41 c 25.16 −20.16 −16.66 42.75 4 X331
5501 53.1280240 −27.8593930 5.39 c 25.71 −20.23 −16.45 43.10 4 –
8687 53.0868634 −27.8295859 4.23 c 26.90 −19.19 −16.43 42.90 4 –
8884 53.1970699 −27.8278566 4.52 c 25.74 −19.04 −16.77 42.65 4 –
9713 53.1715890 −27.8208052 5.86 5.702 c 26.54 −19.87 −16.46 43.15 4 HUDF322
9945 53.1619508 −27.8190897 4.34 4.4973 cd 24.99 −20.93 −16.65 42.75 4 –
11 287 53.0689924 −27.8071692 4.94 c 25.06 −20.48 −16.42 43.10 4 M8728
12 130 53.1514304 −27.7997601 4.43 4.624 c 25.54 −20.60 −16.58 42.85 5 HUDF3094
14 800 53.0211735 −27.7823645 4.92 4.8235 c 23.43 −22.51 −16.38 43.10 3 M10548
16 822 53.1115637 −27.7677714 4.52 c 25.67 −18.97 −15.91 43.85 4 M70168, L245, X371
19 713 53.1198898 −27.7430349 4.84 c 25.31 −18.14 −16.48 43.00 4 E1516, X392
20 765 53.1583449 −27.7334854 5.23 f 24.44 −21.06 −16.29 43.25 3 E2551
23 757 53.2036444 −27.7143907 4.13 c 24.56 −20.72 −16.49 42.85 1 –
28 476 53.0646867 −27.8625539 6.26 f 26.77 −19.03 −16.60 43.10 4 M70407
29 323 53.0409764 −27.8376619 9.73 cf 26.33 −19.50 −15.96 44.00 3 M70340, L103, X156
31 334 53.2131871 −27.7816486 4.73 f 26.41 −19.60 −15.69 43.75 4 –
33 073 53.0547529 −27.7368325 4.98 c 26.89 −19.19 −16.44 43.10 2 E2199
33 160 53.0062504 −27.7340678 6.06 cf 25.90 −19.62 −16.26 43.65 3 E2498, L57, X85

Notes. ID from Guo et al. (2013) catalogue. Photometric redshifts (zphot) from Dahlen et al. (2013) catalogue. Spectroscopic redshifts after: Column C indicates the compactness of the sources: c = compact, d = diffuse, f = faint object. X-ray fluxes are computed in the 0.5−2 keV band and X-ray luminosities in the 2−10 keV band. M,E in previous catalogues are from Fiore et al. (2012), L from Luo et al. (2008), X from Xue et al. (2011). Column A indicates the GOODS-S field area according to Table 1.

(1)

Vanzella et al. (2008);

(3)

M. Dickinson & D. Stern (priv. comm.);

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