Table 7
Synoptic table containing the main results for the QSO identified in the present sample of 2PBC sources.
Object | F [OII] | F MgII | z | DL (Mpc) | E(B−V)Gal | L X |
|
||||||
2PBC J2010.3−2522 | 0.3 ± 0.1 | 1.3 ± 0.1 | 0.828 | 5234.4 | 0.164 | 42.6 (15–150)C |
[0.6 ± 0.2] | [1.8 ± 0.3] | 4.03 (0.3–10)X | ||||
47.7 (14-195)B |
Notes. Emission-line fluxes are reported both as observed and (between square brackets) corrected for the intervening Galactic absorption E(B−V)Gal along the object line of sight (from Schlegel et al. 1998). Line fluxes are in units of 10-15 erg cm-2 s-1, X-ray luminosities are in units of 1045 erg s-1, and the reference band (between round brackets) is expressed in keV. In the last column, the upper case letter indicates the satellite and/or the instrument with which the corresponding X-ray flux measurement was obtained. The typical error of the redshift measurement is ±0.001.
From Cusumano et al. (2010) and
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