paper

The metal absorption systems of the Hubble Deep Field South QSO

arXiv:astro-ph/9804019 · doi:10.1086/300509

Abstract

The Hubble Deep Field South (HDFS) has been recently selected and the observations are planned for October 1998. We present a high resolution (FWHM \kms) spectrum of the quasar J2233--606 () which is located 5.1 arcmin East of the HDFS. The spectrum obtained with the New Technology Telescope redward of the Lyman-- emission line covers the spectral range 4386--8270 Å. This range corresponds to redshift intervals for CIV and MgII intervening systems of and respectively. The data reveal the presence of two complex intervening CIV systems at redshift and and two complex associated () systems. Other two CIV systems at and , suggested by the presence of strong Lyman-- lines in low resolution ground based and Hubble Space Telescope (HST) STIS observations (Sealey et al. 1998) have been identified. The system at is also responsible for the Lyman limit absorption seen in the HST/STIS spectrum. The main goal of the present work is to provide astronomers interested in the Hubble Deep Field South program with information related to absorbing structures at high redshift, which are distributed along the nearby QSO line of sight. For this purpose, the reduced spectrum, obtained from three hours of integration time, has been released to the astronomical community.

revisited version accepted for publication by Astronomical Journal; minor changes; typographical errors corrected; results and discussion unchanged

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