- ... quasars
- Figures 2 to 21, 23 to 25, 31 to 34 and Tables 3 to 16 are only available in electronic form at http://www.edpsciences.org
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...2004)
- The reason why we did
not use later releases (DR3 or DR4) is because, as discussed
in the following, we had to inspect individually each
spectrum to remove broad absorption line quasars, and
DR2 has a number of objects for which this process is feasible.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... quasars
- We regard the SDSS spectroscopic targets as quasars
when the objects are classified as "quasars''
(specClass=3) or "high-z quasars''
(specClass=4)
by the SDSS classification algorithm.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... IRAF
- IRAF (Image Reduction and Analysis Facility) is distributed
by the National Optical Astronomy Observatory, which is operated
by the Association of Universities for Research in Astronomy Inc.,
under corporative agreement with the National Science Foundation.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.