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SDSSNBCQSC - Sloan Digital Sky Survey NBC Quasar Candidate Catalog |
HEASARC Archive |
Much more information on the SDSS is available at the project's web site at http://www.sdss.org/.
Efficient photometric selection of quasars from the Sloan Digital Sky Survey: 100000 z<3 quasars from data release one. Richards G.T., Nichol R.C., Gray A.G., Brunner R.J., Lupton R.H., Vanden Berk D.E., Chong S.S., Weinstein M.A., Schneider D.P., Anderson S.F., Munn J.A., Harris H.C., Strauss M.A., Fan X., Gunn J.E., Ivezic Z., York D.G., Brinkmann J., Moore A.W. <Astrophys. J. Suppl. Ser., 155, 257-269 (2004)> =2004ApJS..155..257R
Name
The NBC Quasar Candidate Catalog designation using the unique
catalog number and the prefix '[RNG2004] ' recommended by the Dictionary
of Nomenclature of Celestial Objects.
SDSS_Name
The standard SDSS designation of the object, in the format
'SDSS Jhhmmss.ss+ddmmss.s' using the sexagesimal J2000.0 coordinates.
RA
The Right Ascension of the UVX quasar candidate in the selected
equinox. This was given in J2000.0 decimal degrees to a precision of 0.1
microdegrees (0.36 milliarcseconds) in the original table.
Dec
The Declination of the UVX quasar candidate in the selected
equinox. This was given in J2000.0 decimal degrees to a precision of 0.1
microdegrees (0.36 milliarcseconds) in the original table.
LII
The Galactic Longitude of the object.
BII
The Galactic Latitude of the object.
SDSS_ID
The SDSS object identifier string, in the format
'skyVersion-run-rerun-camcol-field-id'.
Row_Pixel
The row position of the object in the field, in pixels.
Column_Pixel
The column position of the object in the field, in pixels.
Umag
The u-band magnitude of the object. All magnitudes are "asinh" point
spread function (PSF) magnitudes (Lupton et al., 1999AJ....118.1406L) and
uncorrected for Galactic extinction.
Gmag
The g-band magnitude of the object. All magnitudes are "asinh" point
spread function (PSF) magnitudes (Lupton et al., 1999AJ....118.1406L) and
uncorrected for Galactic extinction.
Rmag
The r-band magnitude of the object. All magnitudes are "asinh" point
spread function (PSF) magnitudes (Lupton et al., 1999AJ....118.1406L) and
uncorrected for Galactic extinction.
Imag
The i-band magnitude of the object. All magnitudes are "asinh" point
spread function (PSF) magnitudes (Lupton et al., 1999AJ....118.1406L) and
uncorrected for Galactic extinction.
Zmag
The z-band magnitude of the object. All magnitudes are "asinh" point
spread function (PSF) magnitudes (Lupton et al., 1999AJ....118.1406L) and
uncorrected for Galactic extinction.
Umag_Error
The error in the u-band magnitude.
Gmag_Error
The error in the g-band magnitude.
Rmag_Error
The error in the r-band magnitude.
Imag_Error
The error in the i-band magnitude.
Zmag_Error
The error in the z-band magnitude.
Umag_Extinction
The Galactic extinction in the u-band, in magnitudes.
Gmag_Extinction
The Galactic extinction in the g-band, in magnitudes.
Rmag_Extinction
The Galactic extinction in the r-band, in magnitudes.
Imag_Extinction
The Galactic extinction in the i-band, in magnitudes.
Zmag_Extinction
The Galactic extinction in the z-band, in magnitudes.
Quasar_Density
The kernel density estimate (KDE) computed quasar
probability density for the object.
Star_Density
The kernel density estimate (KDE) computed star probability
density for the object. For the final catalog, NBC-selected quasars were
rejected if the stellar density exceeded 0.01.
Redshift
The photometric redshift of the object, determined by the
method described in Weinstein et al., 2004ApJS..155..243W using an
algorithm that minimizes the difference between the measured colors of
each object and the median color of quasars as a function of redshift.
Redshift_Lower_Limit
The lower limit to the photometric redshift range.
Redshift_Upper_Limit
The upper limit to the photometric redshift range.
Redshift_Probability
The probability that the photometric redshift is
within the quoted range: see Weinstein et al., 2004ApJS..155..243W for more
details.
Previous_Class
The previous classification for the catalog object based
a match to three spectroscopic databases: (1) the SDSS-DR1 Quasar Catalog
(Schneider et al., 2003AJ....126.2579S, the HEASARC Browse table SDSSQUASAR),
which includes only bona fide quasars: objects from this are labeled as
'DR1QSO'; (2) the 2QZ NGP Catalog (Croom et al., 2004MNRAS.349.1397C),
which includes quasars as well as non-quasars: objects from this are labeled
with '2QZ' and then the object type, e.g., '2QZNELG', '2QZQSO', etc.; and
(3) "good" spectroscopic IDs from the SDSS-DR2 database (Abazajian et al.,
2004AJ....128..502A), which include quasars as well as non-quasars: objects
from this are labeled with 'DR2' and then the object type, e.g.,
'DR2GALAXY', 'DR2QSO', etc. Matching to these 3 catalogs was done in series
in the order given, such that an object will only match the first
occurrence. Objects with no matches have been given the value of 'U' for
unknown.
Previous_Redshift
The previous redshift for the catalog object, taken
from the sources listed for the previous_class parameter.
Flux_20_cm
The 20-cm flux density, in mJy, of the radio counterpart
to the catalog object. Objects were matched to the FIRST Catalog
(Becker et al., 1995ApJ...450..559B, White et al., 1997ApJ...475..479W)
and to the Spitzer First Look Survey (Condon et al., 2003AJ....125.2411C),
if the positions agreed within 1.5 arcseconds - the same radius used for
the SDSS's target selection algorithm. For FIRST radio sources, the peak
20 cm flux density is listed, whereas, for objects from Condon et al.'s
deep 20 cm survey, the integrated 20 cm flux density is listed. Objects
that match both radio catalogs have only their FIRST data reported (as
can be discerned by their >~ 1 mJy flux densities).
RASS_Count_Rate
The ROSAT All-Sky Survey (RASS) broadband (0.1 - 2.4
keV) vignetting-corrected count rate, in ct/s , of the X-ray counterpart to
the catalog object, using a 30 arcseconds matching radius. The expected
number of SDSS quasar candidates superposed on unrelated RASS 30" radius
X-ray error circles is about 69 or 5% of the tabulated 1304 likely
SDSS/RASS positional matches.
Proper_Motion
The proper motion of the catalog object, in mas/yr.
The authors matched the quasar candidates to the improved USNO-B+SDSS
proper motions tabulated by Munn et al. (2004AJ....127.3034M), which
is 90% complete to g ~ 19.7 using criteria specified in section 4.4.3
of the published paper. 99.5% of the spectroscopically confirmed quasars
in the sample have proper motions less than 20 mas/yr. There are 799
objects with proper motions >= 20 mas/yr in the catalog, most of which
are likely to be stars.