SDSS Spectroscopic Surveys

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SDSS Spectroscopic Surveys

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dc.contributor.author Ivezić, Željko
dc.contributor.editor Popović, Luka Č.
dc.date.accessioned 2011-01-10T11:03:54Z
dc.date.available 2011-01-10T11:03:54Z
dc.date.issued 2007
dc.identifier.isbn 978-86-80019-17-8 en_US
dc.identifier.uri http://hdl.handle.net/123456789/1455
dc.description.provenance Submitted by Slavisha Milisavljevic (slavisha) on 2011-01-10T11:03:54Z No. of bitstreams: 1 I07.pdf: 3882263 bytes, checksum: a2d681e9e8f4a2ef72cfb6975c8502cb (MD5) en
dc.description.provenance Made available in DSpace on 2011-01-10T11:03:54Z (GMT). No. of bitstreams: 1 I07.pdf: 3882263 bytes, checksum: a2d681e9e8f4a2ef72cfb6975c8502cb (MD5) Previous issue date: 2007 en
dc.language.iso en en_US
dc.publisher Nenad Milovanović & Milan S. Dimitrijević, Astronomical Observatory, Belgrade en_US
dc.title SDSS Spectroscopic Surveys en_US
mf.subject.keywords In addition to optical photometry of unprecedented quality, the Sloan Digital Sky Survey (SDSS) is also producing a massive spectroscopic database. The SDSS spectra have a wavelength coverage from 3800 to 9200 Å, with a resolution of about 2000. The recent Data Release 5 includes spectra for over 150,000 stars and nearly a million extragalactic objects. I will discuss a subset of science results based on the analysis of SDSS spectra, including kinematics and metallicity distribution of the Milky Way stars, determination of the stellar mass of galaxies, and a sample of AGN with unusual line profiles. en_US
mf.document.pages 21 en_US
mf.contributor.editor-in-chief Dimitrijević, S. Milan

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