<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Schneider, Donald P.</style></author><author><style face="normal" font="default" size="100%">Richards, Gordon T.</style></author><author><style face="normal" font="default" size="100%">Hall, Patrick B.</style></author><author><style face="normal" font="default" size="100%">Strauss, Michael A.</style></author><author><style face="normal" font="default" size="100%">Anderson, Scott F.</style></author><author><style face="normal" font="default" size="100%">Boroson, Todd A.</style></author><author><style face="normal" font="default" size="100%">Ross, Nicholas P.</style></author><author><style face="normal" font="default" size="100%">Shen, Yue</style></author><author><style face="normal" font="default" size="100%">Brandt, W. N.</style></author><author><style face="normal" font="default" size="100%">Fan, Xiaohui</style></author><author><style face="normal" font="default" size="100%">Inada, Naohisa</style></author><author><style face="normal" font="default" size="100%">Jester, Sebastian</style></author><author><style face="normal" font="default" size="100%">Knapp, G. R.</style></author><author><style face="normal" font="default" size="100%">Krawczyk, Coleman M.</style></author><author><style face="normal" font="default" size="100%">Thakar, Anirudda R.</style></author><author><style face="normal" font="default" size="100%">Vanden Berk, Daniel E.</style></author><author><style face="normal" font="default" size="100%">Wolfgang Voges</style></author><author><style face="normal" font="default" size="100%">Yanny, Brian</style></author><author><style face="normal" font="default" size="100%">York, Donald G.</style></author><author><style face="normal" font="default" size="100%">Bahcall, Neta A.</style></author><author><style face="normal" font="default" size="100%">Bizyaev, Dmitry</style></author><author><style face="normal" font="default" size="100%">Blanton, Michael R.</style></author><author><style face="normal" font="default" size="100%">Brewington, Howard</style></author><author><style face="normal" font="default" size="100%">Brinkmann, J.</style></author><author><style face="normal" font="default" size="100%">Eisenstein, Daniel</style></author><author><style face="normal" font="default" size="100%">Frieman, Joshua A.</style></author><author><style face="normal" font="default" size="100%">Fukugita, Masataka</style></author><author><style face="normal" font="default" size="100%">Gray, Jim</style></author><author><style face="normal" font="default" size="100%">Gunn, James E.</style></author><author><style face="normal" font="default" size="100%">Hibon, Pascale</style></author><author><style face="normal" font="default" size="100%">Ivezić, Željko</style></author><author><style face="normal" font="default" size="100%">Kent, Stephen M.</style></author><author><style face="normal" font="default" size="100%">Kron, Richard G.</style></author><author><style face="normal" font="default" size="100%">Lee, Myung Gyoon</style></author><author><style face="normal" font="default" size="100%">Lupton, Robert H.</style></author><author><style face="normal" font="default" size="100%">Malanushenko, Elena</style></author><author><style face="normal" font="default" size="100%">Malanushenko, Viktor</style></author><author><style face="normal" font="default" size="100%">Oravetz, Dan</style></author><author><style face="normal" font="default" size="100%">Pan, K.</style></author><author><style face="normal" font="default" size="100%">Pier, Jeffrey R.</style></author><author><style face="normal" font="default" size="100%">Price, Ted N.</style></author><author><style face="normal" font="default" size="100%">Saxe, David H.</style></author><author><style face="normal" font="default" size="100%">Schlegel, David J.</style></author><author><style face="normal" font="default" size="100%">Simmons, Audry</style></author><author><style face="normal" font="default" size="100%">Snedden, Stephanie A.</style></author><author><style face="normal" font="default" size="100%">SubbaRao, Mark U.</style></author><author><style face="normal" font="default" size="100%">Szalay, Alexander S.</style></author><author><style face="normal" font="default" size="100%">Weinberg, David H.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">The Sloan Digital Sky Survey Quasar Catalog. V. Seventh Data Release</style></title><secondary-title><style face="normal" font="default" size="100%">The Astronomical Journal</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2010</style></year><pub-dates><date><style  face="normal" font="default" size="100%">June 1, 2010</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">http://adsabs.harvard.edu/abs/2010AJ....139.2360S</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">139</style></volume><pages><style face="normal" font="default" size="100%">2360-2373</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We present the fifth edition of the Sloan Digital Sky Survey (SDSS)Quasar Catalog, which is based upon the SDSS Seventh Data Release. Thecatalog, which contains 105,783 spectroscopically confirmed quasars,represents the conclusion of the SDSS-I and SDSS-II quasar survey. Thecatalog consists of the SDSS objects that have luminosities larger thanM&lt;sub&gt;i&lt;/sub&gt; = -22.0 (in a cosmology with H &lt;sub&gt;0&lt;/sub&gt; = 70 kms&lt;sup&gt;-1&lt;/sup&gt; Mpc&lt;sup&gt;-1&lt;/sup&gt;, Ω&lt;sub&gt; M &lt;/sub&gt; = 0.3, andΩ&lt;sub&gt;Λ&lt;/sub&gt; = 0.7), have at least one emission line withFWHM larger than 1000 km s&lt;sup&gt;-1&lt;/sup&gt; or have interesting/complexabsorption features, are fainter than i ≈ 15.0, and have highlyreliable redshifts. The catalog covers an area of ≈9380deg&lt;sup&gt;2&lt;/sup&gt;. The quasar redshifts range from 0.065 to 5.46, with amedian value of 1.49; the catalog includes 1248 quasars at redshiftsgreater than 4, of which 56 are at redshifts greater than 5. The catalogcontains 9210 quasars with i &amp;lt; 18; slightly over half of the entrieshave i &amp;lt; 19. For each object the catalog presents positions accurateto better than 0farcs1 rms per coordinate, five-band (ugriz) CCD-basedphotometry with typical accuracy of 0.03 mag, and information on themorphology and selection method. The catalog also contains radio,near-infrared, and X-ray emission properties of the quasars, whenavailable, from other large-area surveys. The calibrated digital spectracover the wavelength region 3800-9200 Å at a spectral resolutionof ~= 2000; the spectra can be retrieved from the SDSS public database&lt;/p&gt;
</style></abstract><notes><style face="normal" font="default" size="100%">n/a</style></notes><custom3><style face="normal" font="default" size="100%">eprintid: arXiv:1004.1167</style></custom3></record></records></xml>