/ftp/cats/J/ApJS/143/257



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J/ApJS/143/257      AGN emission line properties        (Kuraszkiewicz+, 2002)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat table4.dat table5.dat
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Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/ApJS/143/257
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drwxr-xr-x 10 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:55 [TAR file] -rw-r--r-- 1 cats archive 490 Dec 4 2004 .message -r--r--r-- 1 cats archive 7805 Dec 4 2004 ReadMe -rw-r--r-- 1 cats archive 552 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 4241 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 9744 Feb 6 2003 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 12702 Jan 31 2003 table4.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1025034 Feb 6 2003 table5.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/ApJS/143/257 AGN emission line properties (Kuraszkiewicz+, 2002) ================================================================================ Emission line properties of active galactic nuclei from a pre-COSTAR Faint Object Spectrograph Hubble Space Telescope spectral atlas. Kuraszkiewicz J.K., Green P.J., Forster K., Aldcroft T.L., Evans I.N., Koratkar A. <Astrophys. J. Suppl. Ser. 143, 257 (2002)> =2002ApJS..143..257K ================================================================================ ADC_Keywords: Clusters, galaxy ; Active gal. nuclei ; Redshifts ; Galaxies, spectra ; Spectra, ultraviolet Keywords: galaxies: active - quasars: emission lines - quasars: general - ultraviolet: galaxies Abstract: We present measurements of the UV/optical emission line parameters in a sample of 158 active galactic nuclei observed with the Faint Object Spectrograph on the Hubble Space Telescope (HST), prior to the installation of COSTAR. We use an automated technique that accounts for galactic reddening, includes iron emission blends, galactic and intrinsic absorption lines, and performs multicomponent fits to the emission line profiles. We present measured line parameters (equivalent width and FWHM) for a large number (28) of different UV/optical lines, including upper limits for undetected lines.

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