VLULXCAT - Extremely Luminous X-Ray Source Candidates Catalog
In order to know whether an X-ray source falls within a particular galaxy, for each galaxy, the authors collected its center's RA, Dec, distance, and D25 isophotal info, which includes major axis length, minor axis length, and the position angle of the major axis from the PGC2003 Catalog (Paturel et al. 2003, A&A, 412, 45), which includes the full RC3 catalog and has all of the necessary parameters except for distance. The authors restricted the minimum major axis length to be 10 arcseconds, and collected their distances from NED as much as possible. Their final sample includes 77,000 galaxies within 250 Mpc.
The authors used all of the Chandra ACIS data in TE mode that were released before 2014, which includes 9400 ObsIDs. A roughly linear relation between the flux and count rate derived by PIMMS 4.6b was established assuming a power-law spectral shape and galactic foreground extinction (Kalberla et al. 2005, A&A, 440, 775). Any source with a PIMMS luminosity larger than 5 x 1039 erg s-1 would be recalculated by the CIAO script model flux assuming a power-law index of 1.7 in the 0.3 - 8.0 keV energy band. After the recalculation, 1,809 X-ray sources with Lx > 3 x 1040 erg s-1 falling within 640 D25 contours covered by 905 ObsIDs were picked out. A large fraction of the 1,809 sources are galactic nuclei and some of them are repeated. Only off-nuclear sources are considered in this paper. In addition, the centers of the galaxies given by PGC2003 are not necessarily precise and the specific environments of the 1,809 sources are different. Therefore, the authors visually checked the Chandra and DSS images simultaneously, since two-band inspection can help to exclude the nuclear sources, bright knots, and extended sources. X-ray sources with clear DSS features would be dropped because, for a source with a visual magnitude <20 and a distance >30 Mpc, its absolute magnitude would be brighter than -12.4, which is beyond the limit of the brightest star clusters.
An extreme luminous X-ray source catalog based on Chandra ACIS observations. Gong H., Liu J., Maccarone T. <Astrophys. J. Suppl. Ser., 222, 12 (2016)> =2016ApJS..222...12G (SIMBAD/NED BibCode)
The Chandra ACIS ObsID observation identifier in which the source was detected.
The exposure time of the Chandra ACIS ObsID observation identifier in which the source was detected, in seconds (converted by the HEASARC from the ks units given in the original table).
The PGC2003 designation of the galaxy within whose D25 contour the X-ray source is located. Notice that the CDS Dictionary of Astronomical Nomenclature prefers the prefix of 'LEDA' rather than 'PGC' for these galaxies.
The Chandra X-ray source designation. This was created by the HEASARC based on the J2000.0 position using the standard 'CXOU' prefix recommended for unregistered Chandra X-ray Observatory sources.
The Right Ascension of the X-ray source in the selected equinox. This was given in J2000.0 decimal degrees to a precision of 10-5 degrees (0.036 arcseconds) in the original table.
The Declination of the X-ray source in the selected equinox. This was given in J2000.0 decimal degrees to a precision of 10-5 degrees (0.036 arcseconds) in the original table.
The Galactic Longitude of the X-ray source.
The Galactic Latitude of the X-ray source.
The X-ray source net counts in the 0.3 - 8.0 keV energy band from Wavdetect.
The distance to the X=ray source (assuming it is physically associated with the galaxy within whose D-25_ contour it lies), in Mpc.
The 0.3-8 keV absorbed flux of the X-ray source, in erg s-1 cm-2, as derived by the CIAO script modelflux.
The 0.3-8 keV luminosity of the X-ray source, in erg s-1, using the flux as derived by the CIAO script modelflux and the quoted distance. Luminosities are given using their fluxes directly since the galactic absorption is low.
The Kolmogorov-Smirnov (K-S) test probability that the source is constant. The K-S tests the null hypothesis that the photon accumulation is uniform. A variable source is defined by PK-S < 0.01.
Comments on the source identification, nature, etc.
This parameter gives the codes for the references given in the comments, as follows:
b = SIMBAD 1 = Farrell et al. (2009, Nature, 460, 73) 2 = Sutton et al. (2012, MNRAS, 423, 1154), Gutierrez & Moon (2014, ApJ, 797, L7)