Intergalactic CIV absorption at redshifts 5.4 to 6

Details Intergalactic CIV absorption at redshifts 5.4 to 6 Intergalactic CIV absorption at redshifts 5.4 to 6

2006-07-03

arxiv.org/abs/astro-ph/0607029v2

Mon.Not.Roy.Astron.Soc.Lett. 371 (2006) L78

Astronomy and Astrophysics

Astrophysics

6 pages, 2 figures, accepted for publication in MNRAS on June 28th

Scientific paper

10.1111/j.1745-3933.2006.00212.x

We report the discovery of a strong CIV 1548,1550 absorption system at z_abs = 5.7238 in the near-infrared spectrum (J-band) of the z_em = 6.28 QSO SDSS J1030+0524. These observations, obtained with the Infrared Spectrometer And Array Camera (ISAAC) on the European Southern Observatory Very Large Telescope (ESO VLT), demonstrate that, with modern instrumentation, QSO absorption line spectroscopy can be successfully extended to near-infrared wavelengths to probe the intergalactic medium near the end of the reionization epoch. Although the statistics of this pilot study are limited, the mass density of triply ionized carbon implied by our data is comparable to the values of Omega_CIV reported at lower redshifts. Neither the column density distribution of CIV absorbers nor its integral show significant redshift evolution over a period of time which stretches from 1 to 4.5 Gyr after the big bang, suggesting that a large fraction of intergalactic metals may already have been in place at redshifts above 6. Alternatively, the strong CIV system we have detected may be associated with outflowing, highly-ionized, gas from a foreground massive galaxy; deep imaging and spectroscopy of galaxies near the QSO sightline should be able to distinguish between these two possibilities.

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