Table 4.
Measured and inferred CLQ properties.
| Object | MJD | Hβ flux | HβFWHM | Hβz | Hα flux | HαFWHM | Hαz | MBH | λEdd |
|---|---|---|---|---|---|---|---|---|---|
| (SDSS J) | (erg s−1) | (km s−1) | (km s−1) | (erg s−1) | (km s−1) | (km s−1) | (108 M⊙) | ||
| 0823 + 4220 | 52266 | 429 ± 20 | 3913 ± 169 | −44 ± 100 | 2458 ± 25 | 4842 ± 62 | 218 ± 12 | 1.22 ± 0.3 | 0.013 ± 0.001 |
| 54524 | 227 ± 44 | 5073 ± 2252 | 309 ± 933 | 1198 ± 26 | 4453 ± 150 | 62 ± 45 | 0.729 ± 0.050 | 0.012 ± 0.001 | |
| 1723 + 5504 | 51813 | 350 ± 13 | 8891 ± 517 | 1326 ± 221 | 1456 ± 33 | 6275 ± 143 | 227 ± 65 | 3.72 ± 0.17 | 0.013 ± 0.001 |
| 51997 | 509 ± 9 | 5317 ± 170 | 211 ± 61 | 2551 ± 23 | 6404 ± 121 | 203 ± 27 | 4.92 ± 0.18 | 0.016 ± 0.001 | |
| 0126 − 0839 | 52163 | 296 ± 18 | 4200 ± 312 | −181 ± 107 | 980 ± 16 | 3591 ± 73 | −9 ± 25 | 1.22 ± 0.05 | 0.043 ± 0.002 |
| 54465 (a) | 0 | ... | ... | 0 | ... | ... | ... | ... | |
| 0829 + 4154 | 52266 | 1210 ± 201 | 8061 ± 1001 | 1597 ± 163 | 8241 ± 309 | 7297 ± 158 | 1045 ± 15 | 3.11 ± 0.87 | 0.006 ± 0.001 |
| 54524 | 2194 ± 205 | 8201 ± 696 | 1512 ± 150 | 15167 ± 45 | 7231 ± 25 | 846 ± 12 | 3.92 ± 0.58 | 0.008 ± 0.001 | |
| 0002 − 0027 | 51791 | 404 ± 18 | 12203 ± 277 | 2334 ± 246 | 1646 ± 38 | 6835 ± 281 | −304 ± 58 | 5.47 ± 0.46 | 0.014 ± 0.001 |
| 52559 | 362 ± 17 | 13709 ± 618 | 3986 ± 86 | 1105 ± 31 | 8628 ± 340 | −427 ± 93 | 7.19 ± 0.58 | 0.007 ± 0.001 | |
| (BOSS) | 55477 | 1199 ± 28 | 18931 ± 287 | 326 ± 135 | 1655 ± 19 | 7723 ± 116 | −1119 ± 30 | ... | ... |
| 1358 + 4934 | 53438 | 18 ± 9 | 1793 ± 1166 | 2873 ± 551 | 201 ± 22 | 5753 ± 541 | 492 ± 279 | 0.378 ± 0.07 | 0.002 ± 0.001 |
| 54553 | 238 ± 20 | 4527 ± 546 | 359 ± 131 | 870 ± 13 | 3368 ± 92 | 148 ± 22 | 0.282 ± 0.02 | 0.015 ± 0.001 |
Notes. Hβ (Hα) flux, FWHM, and z are the flux, FWHM and redshift with respect to the Hβ (Hα) rest wavelength, of the Hβ (Hα) broad component, MBH is the black hole mass calculated using the relation of Greene et al. (2010) and the broad Hα FWHM, and λEdd is the Eddington ratio. All stated errors are 1σ uncertainties generated from a 102 Monte Carlo simulation of the emission line fitting procedure from Sect. 3.4.3.
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