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Table 1

Catalog of point sources in the field.

ID/classification RA Dec PSF size (soft) PSF size (hard) Flux soft CR soft HR Zspec Zphot
deg deg pix pix 10-15 erg/cm2/s 10-4 cps
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)

1 34.5809  −5.2543 3.51  −999.00  −0.217 ± 0.308
2 34.5961  −5.2367 2.55  −999.00  −0.377 ± 0.352
3 34.6173  −5.2326 2.47 2.45 0.368 ± 0.289
4 34.6437  −5.2325 2.92 2.92  −0.389 ± 0.057
5 34.5356  −5.2068 2.26 2.26  −0.512 ± 0.057
6 34.6091  −5.2013 1.23  −999.00  −1.000
7 (B1) 34.6386  −5.1977 1.54  −999.00  −0.641 ± 0.359
8 34.5532  −5.1898 1.37  −999.00 0.034 ± 0.299
9 (B2) 34.6345  −5.1892 1.24 1.23  −0.756 ± 0.112
10 (AGN) 34.5717  −5.1849 0.90 0.90  −0.064 ± 0.127 1.6487 (a)
11 34.5514  −5.1785 1.17  −999.00  −0.699 ± 0.296
12 (A) 34.5879  −5.1758 0.62 0.62  −0.530 ± 0.252 1.6230 (b)
13 34.5423  −5.1757 1.36  −999.00 0.235 ± 0.391
14 (IR-24μ/AGN) 34.5997  −5.1739 0.58  −999.00  −0.812 ± 0.268 1.6240 (b)
15 34.5713  −5.1647 0.61  −999.00  −0.341 ± 0.465
16 34.6130  −5.1637 0.53  −999.00 0.443 ± 0.463
17 34.6478  −5.1515 0.97  −999.00  −0.209 ± 0.296
18 34.5667  −5.1499 0.58 0.58  −0.026 ± 0.222
19 34.5872  −5.1332 0.43 0.43 0.343 ± 0.202
20 34.5530  −5.1311 0.83  −999.00  −0.012 ± 0.704
21 34.6180  −5.2642 4.30  −999.00 * * *
22 34.5492  −5.2329 2.96  −999.00  −0.849 ± 0.530
23 34.5358  −5.2123 2.47  −999.00  −0.009 ± 0.370
24 34.5255  −5.1546 1.64  −999.00 0.053 ± 0.441
25 34.5583  −5.2059  −999.00 1.70 0.574 ± 0.239
26 34.5965  −5.1205  −999.00 0.49 0.587 ± 0.258
27 34.5269  −5.2332  −999.00 3.59 0.00 + 0.21 0.00 + 0.51 1.000
28 34.6478  −5.1635  −999.00 1.09 0.334 ± 0.384

Notes. Columns (4) and (5) refer to the pixel size of the PSF at the location of the source as estimated by wavdetect. A value of  −999.9 indicates that the source was not detected in the given band. The soft and hard band correspond to [0.5–2] keV and [2–8] keV, respectively. Fluxes in Col. (6) are unabsorbed fluxes computed assuming a power law of index 1.7 and a galactic NH = 2.2 × 1020 cm-2, using the count rates reported in Col. (7). Source 21 could not be measured because located at the edge of the FoV. If the mode of the flux (count rate) distribution is 0.0, the + sign indicates an upper limit. Fluxes are measured in 10′′ radius aperture. Column (8) provides the hardness ratio HR = (H  −  S)/(H + S) where H and S are count rates measured in hard and soft bands, respectively.

References. Reference for the spectroscopic redhsifts: (a) Papovich et al. (2010); (b) Tanaka et al. (2010). The photometric redshifts are based on the same data and analysis as in Papovich et al. (2010).

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