Sign on

SAO/NASA ADS Astronomy Abstract Service

· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· Full Refereed Journal Article (PDF/Postscript)
· arXiv e-print (arXiv:astro-ph/0405051)
· References in the article
· Citations to the Article (14) (Citation History)
· Refereed Citations to the Article
· SIMBAD Objects (223)
· NED Objects (83)
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
The Kast Ground-based Ultraviolet Spectral Survey of 79 Quasi-stellar Objects at Redshift 2 for Lyα Forest and Metal Absorption
Authors:
Tytler, David; O'Meara, John M.; Suzuki, Nao; Kirkman, David; Lubin, Dan; Orin, Adam
Affiliation:
AA(), AB(), AC(Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive, San Diego, CA 92093-0424 ), AD(Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive, San Diego, CA 92093-0424 ), AE(Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive, San Diego, CA 92093-0424 ), AF(Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive, San Diego, CA 92093-0424 )
Publication:
The Astronomical Journal, Volume 128, Issue 3, pp. 1058-1077. (AJ Homepage)
Publication Date:
09/2004
Origin:
UCP
AJ Keywords:
Cosmology: Observations, Galaxies: Quasars: Absorption Lines, Galaxies: Quasars: Emission Lines
DOI:
10.1086/423293
Bibliographic Code:
2004AJ....128.1058T

Abstract

We present spectra of 79 bright QSOs obtained with the Kast spectrograph on the 3 m Shane Telescope at Lick Observatory. The QSOs have emission redshifts 1.89-2.45, and most are near the mean value of zem=2.17. Two of them, one a new discovery, are broad absorption line QSOs. The spectra have ~250 km s-1 resolution, and they cover 3175-5880 Å with signal-to-noise ratios of 6-20 per 1.13 Å pixel in the Lyα forest between Lyα and Lyβ. We show the continuum levels that we used in a previous paper to make a calibrated measurement of the amount of absorption in the Lyα forest at z=1.9. We measure redshifts for 140 absorption-line systems, and we list the metal ions that we see in each system. We identify 526 emission lines and list their observed wavelengths, which we use to obtain new emission redshifts. We find that three emission lines, or line blends, in the forest have mean rest wavelengths of 1070.95+/-1.00, 1123.13+/-0.51, and 1175.88+/-0.30 Å.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)
   

Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints