Clustering properties of high matter density peaks from UVES observations of QSO pairs

Details Clustering properties of high matter density peaks from UVES observations of QSO pairs Clustering properties of high matter density peaks from UVES observations of QSO pairs

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17..266d&link_type=abstract

Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista

Astronomy and Astrophysics

Astronomy

Cosmology: Observations, Galaxies: High-Redshift, Quasar: Absorption Lines

Scientific paper

The association of high H 0 column density absorption systems in QSO spectra with galactic objects has been widely verified at redshifts up to z ~ 1, by direct imaging of QSO fields and follow-up spectroscopy (Guillemin & Bergeron 1997; Le Brun et al. 1997). We study the transverse clustering properties of these tracers of high matter density peaks, by looking for coincident absorption systems in adjacent lines of sight toward QSO pairs and groups (D'Odorico et al. 2002).

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