XMMCTY2AGN - XMM-COSMOS X-Ray Selected Type-2 AGN
The bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS survey. Lusso E., Comastri A., Vignali C., Zamorani G., Treister E., Sanders D., Bolzonella M., Bongiorno A., Brusa M., Civano F., Gilli R., Mainieri V., Nair P., Aller M., Carollo M., Koekemoer A.M., Merloni A., Trump J.R. <Astron. Astrophys. 534, A110 (2011)> =2011A&A...534A.110L (SIMBAD/NED BibCode)
(1) Values of 0.00 for the bolometric correction kbol parameter (called hardxray_bc in this version) have been set to nulls: there were 15 such cases;
(2) The corresponding values of the (logarithm of the) bolometric luminosity for these 15 cases haves also been set to null values: in the original table, these had (unphysically large) values in the range 56 to 83.
The XMM-COSMOS identification (XID) Number for the source, from Cappelluti et al. (2009, A&A, 497, 635).
The name for the X-ray source using the naming convention recommended by the Dictionary of Nomenclature of Celestial Objects for XMM-COSMOS sources, viz. the 'XMMC' prefix and the source (XID) number, e.g., 'XMMC 5094'.
The name of the X-ray source in the form 'XMMU JHHMMSS.s+DDMMSS' where the prefix is the usual one for XMM-Newton sources and the remainder of the field is the J2000.0 equatorial coordinates truncated to 0.1 seconds of time in RA and to 1 arcsecond in Declination.
The Right Ascension of the source in the selected equinox. This was given in J2000.0 equatorial coordinates in decimal degrees to a precision of 10-5 degrees in the original Brusa et al. (2010, ApJ, 716, 348) table.
The Declination of the source in the selected equinox. This was given in J2000.0 equatorial coordinates in decimal degrees to a precision of 10-5 degrees in the original Brusa et al. (2010, ApJ, 716, 348) table.
The Galactic Longitude of the source.
The Galactic Latitude of the source.
The spectroscopic redshift of the source. The origin of the redshifts for these sources is given in Footnote 2 in the Section 2 of the reference paper.
The logarithm of the intrinsic X-Ray luminosity of the source in the hard X-ray (2 - 10 keV) energy band, in erg s-1.
The logarithm of the nuclear bolometric luminosity of the source, in erg s-1. The method used to estimate this parameter is discussed in Section 6 of the reference paper.
The hard-X-ray bolometric correction, kbol, of the source, defined as the ratio of the bolometric and hard X-ray luminosities.
The logarithm of the stellar mass of the associated galaxy, in solar masses.
The star formation rate of the associated galaxy, in solar masses per year.
The absolute U magnitude of the associated galaxy.
The absolute V magnitude of the associated galaxy.
The absolute J magnitude of the associated galaxy.
The morphological classification of the associated galaxy (Type-2 AGN host), coded from 0 to 99 as follows:
0 = elliptical 1 = S0 2 = bulge-dominated 3 = intermediate-bulge 4 = disk-dominated 5 = irregular 6 = compact/irregular 7 = compact 8 = unresolved/compact 9 = blended 10 = bulge-dominated/close-companion 11 = intermediate-bulge/close-companion 12 = S0/close-companion 23 = possible mergers 99 = no classification