The flux ratio of the [OIII] λλ5007, 4959 Ǻ lines in AGN

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The flux ratio of the [OIII] λλ5007, 4959 Ǻ lines in AGN

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dc.contributor.author Vranješ, D.
dc.contributor.author Smiljić, Dj.
dc.contributor.author Gligorić, M.
dc.contributor.author Rakić, N.
dc.contributor.author Obradović, D.
dc.contributor.author Kovačević, J.
dc.contributor.editor Kovačević, Andjelka
dc.date.accessioned 2011-01-25T10:17:32Z
dc.date.available 2011-01-25T10:17:32Z
dc.date.issued 2008
dc.identifier.isbn 978-86-80019-30-7 en_US
dc.identifier.uri http://hdl.handle.net/123456789/1558
dc.description.provenance Submitted by Slavisha Milisavljevic (slavisha) on 2011-01-25T10:17:32Z No. of bitstreams: 1 Vranjes.pdf: 783135 bytes, checksum: 158c8f18a82c238495bba3e47bc97fdb (MD5) en
dc.description.provenance Made available in DSpace on 2011-01-25T10:17:32Z (GMT). No. of bitstreams: 1 Vranjes.pdf: 783135 bytes, checksum: 158c8f18a82c238495bba3e47bc97fdb (MD5) Previous issue date: 2008 en
dc.language.iso en en_US
dc.publisher Astronomical Observatory Belgrade en_US
dc.title The flux ratio of the [OIII] λλ5007, 4959 Ǻ lines in AGN en_US
dc.title.alternative ~ analysis of the sample with red asymmetry and without asymmetry of [OIII] line profiles ~ en_US
mf.subject.area 9 en_US
mf.subject.keywords Here we present the measurements of the flux ratio of the [OIII] λλ4959, 5007 Ǻ emission lines for the sample of 10 AGNs, obtained from SDSS Database and from the published observations. We selected the sample using the criteria of high signal to noise ratio and the same line shapes of λ4959 and λ5007 lines. We separated our sample in two subsamples: first one with red asymmetry of [OIII] λλ4959, 5007 Ǻ lines, where we obtained the average flux ratio of 2.981 ± 0.268 and second one with no asymmetry of [OIII] λλ4959, 5007 Ǻ lines, where we obtained the average flux ratio of 2.885 ± 0.173. For the total sample of ten spectra we found that the flux ratio is 2.943 ± 0.149 so the theoretical value of 2.98 befalls within the error band of our result. en_US
mf.document.pages 9 en_US
mf.contributor.editor-in-chief Dimitrijević, S. Milan
mf.contributor.technical-editor Milovanov, Tatjana

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