Table A.1.
Physical properties of our AGN sample.
XID | R.A. | Decl. | z | z_type | z_ref | log LX, 2 − 10keV | log νLν(6 μm) | αAGN | logM⋆ | logSFR | logL[O III] | S/N[O III] | logL[O II] | S/N[O II] | logL[Ne V] | S/N[Ne V] |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(°) | (°) | (erg s−1) | (erg s−1) | (M⊙) | (M⊙ yr−1) | (erg s−1) | (erg s−1) | (erg s−1) | ||||||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) | (16) | (17) |
cid_1005 | 149.6727 | 2.0058 | 2.227 | photo | M16 | -43.967 | 44.361 | 0.00002 | 10.447 | 1.685 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ |
cid_1007 | 149.6900 | 2.0391 | 1.809 | photo | M16 | 43.554 | 43.154 | 0.00008 | 10.833 | 0.875 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ |
cid_1051 | 150.2529 | 1.8711 | 1.376 | spec | H18 | 43.476 | 44.476 | 1.00000 | 10.988 | 1.727 | ⋯ | ⋯ | 42.590 | 4.72 | ⋯ | ⋯ |
cid_1074 | 149.8269 | 2.0150 | 0.750 | my-photo | This-work | -42.731 | 43.054 | 0.95907 | 9.841 | 0.794 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ |
cid_1168 | 150.2037 | 1.9833 | 0.600 | my-photo | This-work | -42.860 | 41.543 | 1.00000 | 7.971 | -1.484 | 41.173 | 0.39 | ⋯ | ⋯ | ⋯ | ⋯ |
cid_1305 | 150.0450 | 2.2178 | 0.828 | spec | H18 | -43.206 | 43.302 | 0.82546 | 9.669 | 1.421 | 41.281 | 0.19 | 41.292 | 0.57 | ⋯ | ⋯ |
cid_1467 | 149.8375 | 1.9718 | 1.020 | spec | H18 | 42.990 | 43.822 | 0.02199 | 10.762 | 1.948 | 43.365 | 1.01 | 44.307 | 2.54 | ⋯ | ⋯ |
cid_1474 | 149.9241 | 1.8893 | 1.551 | spec | H18 | 43.392 | 44.429 | 0.99999 | 10.369 | 1.669 | ⋯ | ⋯ | 44.810 | 2.25 | 44.667 | 0.99 |
cid_1482 | 150.1530 | 1.8805 | 1.622 | spec | H18 | -43.981 | 43.877 | 0.00006 | 10.529 | 1.556 | ⋯ | ⋯ | 42.977 | 4.81 | 42.389 | 0.43 |
cid_2728 | 150.2385 | 2.0562 | 1.506 | spec | H18 | 43.613 | 44.825 | 1.00000 | 11.069 | 1.961 | ⋯ | ⋯ | 44.348 | 6.85 | 44.292 | 5.43 |
cid_3122 | 149.9663 | 2.0328 | 0.728 | spec | H18 | -43.218 | 43.437 | 1.00000 | 11.076 | 0.899 | 41.790 | 1.21 | 42.093 | 3.38 | ⋯ | ⋯ |
cid_3242 | 149.7112 | 2.1452 | 1.531 | spec | H18 | -43.809 | 44.956 | 1.00000 | 11.231 | 2.472 | ⋯ | ⋯ | 43.212 | 1.82 | 43.785 | 0.92 |
cid_3371 | 149.9374 | 1.7390 | 0.864 | spec | H18 | 43.065 | 42.444 | 0.00003 | 10.708 | 0.992 | 43.041 | 0.16 | 43.978 | 2.24 | ⋯ | ⋯ |
cid_3570 | 149.6409 | 2.1077 | 1.244 | spec | H18 | 43.291 | 44.276 | 1.00000 | 11.006 | 1.475 | ⋯ | ⋯ | 43.124 | 14.07 | ⋯ | ⋯ |
cid_3714 | 150.2400 | 2.3533 | 1.265 | spec | H18 | 43.284 | 43.720 | 0.00000 | 11.069 | 2.179 | ⋯ | ⋯ | 43.288 | 6.94 | ⋯ | ⋯ |
⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
lid_611 | 149.8474 | 2.5692 | 0.913 | spec | H18 | 42.808 | ⋯ | 0.00000 | 11.070 | 2.037 | ⋯ | ⋯ | 43.666 | 1.38 | ⋯ | ⋯ |
lid_617 | 149.6254 | 2.3492 | 1.640 | spec | H18 | 43.257 | 43.660 | 0.00000 | 11.178 | 1.812 | ⋯ | ⋯ | 44.371 | 0.77 | ⋯ | ⋯ |
lid_673 | 149.6210 | 2.0795 | 1.452 | spec | H18 | 43.293 | 45.126 | 1.00000 | 10.953 | 1.086 | ⋯ | ⋯ | 42.650 | 5.00 | ⋯ | ⋯ |
lid_943 | 149.5330 | 1.9588 | 0.565 | spec | H18 | 42.338 | 43.577 | 1.00000 | 9.835 | -0.979 | ⋯ | ⋯ | 42.827 | 1.31 | ⋯ | ⋯ |
lid_950 | 149.5122 | 1.9654 | 2.446 | photo | M16 | 43.648 | 45.109 | 1.00000 | 11.238 | 2.257 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ |
lid_991 | 149.7587 | 1.7552 | 0.831 | photo | M16 | 43.002 | 43.359 | 1.00000 | 10.386 | 0.036 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ |
Notes. This table is available in its entirety at the CDS. Col. (1) contains X-ray IDs from the Civano et al. (2016) catalog. Cols. (2) and (3) contain the R.A. and decl. of the X-ray sources from the Civano et al. (2016) catalog. Col. (4) contains the redshift that we used. Col. (5) contains the type of redshift, including "spec", "photo" and "my-photo". The "spec" represent spectral redshift. The "photo" represent photometric redshift from M16. The "my-photo" is photometric redshift which obtained by SED fitting in this work. Col. (6) lists the references that provide this redshift. "H18" represent Hasinger et al. (2018). Col. (7) contains the logarithm of observed 2-10 keV luminosity in the rest-frame. Among them, negative value represents the upper limit of its luminosity. Col. (8) contains the logarithm of 6 μm luminosity for an AGN in the rest-frame. Col. (9) contains the confidence of AGN components for SED fitting. Cols. (10) and (11) contain the logarithm of M⋆ and SFR for AGN host galaxy. Cols. (12), (14) and (16) contain the logarithm of luminosities for [O III], [O II] and [Ne V] emission lines, respectively. Cols. (13), (15) and (17) contain the S/Ns for [O III], [O II] and [Ne V] emission lines, respectively.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.