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...
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| Format: | Article |
| Language: | en_US |
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IOP Publishing
2013
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| Online Access: | http://hdl.handle.net/1721.1/76593 https://orcid.org/0000-0003-3769-9559 |