Newer edition of SDSS Quasar Catalog available
As of March 2005, the third edition of the SDSS Quasar Catalog,
based on DR3 data and containing 46,420 objects, is available. This
new catalog supersedes all previous editions, which are retained at
their old URLs for reference. Go to the
Third edition of the SDSS Quasar Catalog.
Second edition of the SDSS Quasar Catalog
The DR1 quasar catalog is described in Schneider et al. 2003, AJ
accepted (scheduled to appear in the December 2003 issue and available
at astro-ph/0308443). The
catalog contains 16,713 objects from DR1 that have i-band
absolute magnitudes brighter than -22 and contain at least one broad
emission line. The catalog was created by inspecting all spectra that
were either targeted as quasar candidates, or classified as a quasar
by the spectroscopic
pipelines.
SDSS Quasar Catalog redshifts supersede those in other DR1 data
products
Because of the re-inspection of the spectra, the DR1 Quasar
Catalog provides the most reliable classifications and redshifts of
SDSS quasars. The classifications in the catalog supersede those
found in other DR1 data products accessible from the DR1 data access page, as well as from
the EDR quasar catalog (see below). The improved classifications will
be fed back into other data products for future data
releases.
The DR1 Quasar Catalog is not a statistical sample
There are two reasons:
- It includes objects from all categories of target selection in SDSS, not just those
selected as quasar candidates.
While the catalog does contain target selection flags
which make it easy to remove non-quasar candidates, the
quasars in the catalog were all selected during the
commissioning period. This period saw 12 different
versions of the target selection software; none of the
quasars in the catalog were selected using the final quasar target selection algorithm described in
Richards et al. 2002, which
was the 13th.
The catalog contains both the
TARGET selection flags used to select spectroscopic
targets, and the BEST selection flags obtained by
applying the final target selection version (sometimes to better
photometric data obtained later during the survey - see target and best coverage). However, in addition to
dropping
catalog entries which were not selected by the final version,
one has to account for missing quasar candidates, i.e., those identified by
the final target selection algorithm but without
spectroscopic observations.
These caveats aside, the selection of UV excess quasars has
remained reasonably uniform. These constitute 80% of the objects in
the DR1 Catalog. Changes to the target selection algorithm were
primarily aimed at improving the effectiveness of the identification
of z> 2.5 quasars.
Download the DR1 Quasar Catalog
The catalog is available in the following formats:
- ASCII table
- fits binary table
The catalog files have been generated on August 28, 2003.
Last modified: Tue Mar 29 11:51:05 CST 2005
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