The CIV mass density of the universe at redshift 5

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dc.contributor.authorPettini, M
dc.contributor.authorMadau, P
dc.contributor.authorBolte, M
dc.contributor.authorProchaska, JX
dc.contributor.authorEllison, SL
dc.contributor.authorFan, XH
dc.date.accessioned2025-01-21T01:08:58Z
dc.date.available2025-01-21T01:08:58Z
dc.date.issued2003
dc.description.abstractIn order to search for metals in the Lyalpha forest at redshifts z(abs) > 4, we have obtained spectra of high signal-to-noise ratio and moderately high resolution of three QSOs at z(em) > 5: 4 discovered by the Sloan Digital Sky Survey. These data allow us to probe to metal enrichment of the intergalactic medium at early times with higher sensitivity than previous studies. We find 16 C IV absorption systems with column densities log N (C IV) = 12.50-13.98 over a total redshift path DeltaX = 3.29. In the redshift interval z = 4.5-5.0, where our statistics are most reliable, we deduce a comoving mass density of C3+ ions Omega(CIV) = (4.3 +/- 2.5) x 10(-8) ( 90% confidence limits) for absorption systems with log N (C-IV) greater than or equal to 13.0 ( for an Einstein - de Sitter cosmology with h = 0.65). This value of Omega(CIV) is entirely consistent with those measured at z < 4; we confirm the earlier finding by Songaila that neither the column density distribution of C iv absorbers nor its integral show significant redshift evolution over a period of time that stretches from similar to 1.25 to similar to 4.5 Gyr after the big bang. This somewhat surprising conclusion may be an indication that the intergalactic medium was enriched in metals at z >> 5, perhaps by the sources responsible for its reionization. Alternatively, the C iv systems we see may be associated with outflow from massive star- forming galaxies at later times, while the truly intergalactic metals may reside in regions of the Ly alpha forest of lower density than those probed up to now.
dc.fuente.origenWOS
dc.identifier.eissn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/96530
dc.identifier.wosidWOS:000185257600004
dc.issue.numero2
dc.language.isoen
dc.pagina.final703
dc.pagina.inicio695
dc.revistaAstrophysical journal
dc.rightsacceso restringido
dc.subjectcosmology : observations
dc.subjectgalaxies : high-redshift
dc.subjectintergalactic medium
dc.subjectquasars : absorption lines
dc.titleThe CIV mass density of the universe at redshift 5
dc.typeartículo
dc.volumen594
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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