AGNs emission-line from Post-COSTAR (Kuraszkiewicz+, 2004)

Details AGNs emission-line from Post-COSTAR (Kuraszkiewicz+, 2004) AGNs emission-line from Post-COSTAR (Kuraszkiewicz+, 2004)

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..21500165k&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/150/165. Originally published in: 2004ApJS..150..165K

Physics

Atlases, Active Gal. Nuclei, Qsos, Spectra: Ultraviolet

Scientific paper

The sample was assembled by cross-correlating the Veron-Cetty & Veron (1996ESOSR..17....1V, Cat. , 7th Edition) catalog of AGNs with the MAST (Multimission Archive at Space Telescope) holdings. BL Lac objects were ignored, as their spectra show no emission lines. Starburst galaxies and broad absorption line (BAL) quasars (where emission lines are heavily disrupted by absorption features) were not included. We chose all available (UV and optical) spectrophotometric archival data that have been observed with the Faint Object Spectrograph (FOS) on HST after the installation of COSTAR (i.e., after 1993 December). FOS spectra obtained prior to 1993 December have been analyzed by us in Paper II (Kuraszkiewicz et al., 2002, Cat. ).
(5 data files).

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