The Carbon Content of Intergalactic Gas at Z=4.25 and Its Evolution toward Z=2.4
This paper presents ionization-corrected measurements of the carbon abundance in intergalactic gas at 4.0 < z < 4.5, using spectra of three bright quasars obtained with the Magellan Inamori Kycocera Echelle spectrograph on Magellan. By measuring the C IV strength in a sample of 131 discrete H...
Main Author: | Simcoe, Robert A. (Contributor) |
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Other Authors: | Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor) |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2013-01-24T16:36:31Z.
|
Subjects: | |
Online Access: | Get fulltext |
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