Damped Lyman{alpha} systems (Ellison+, 2009)

Details Damped Lyman{alpha} systems (Ellison+, 2009) Damped Lyman{alpha} systems (Ellison+, 2009)

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..73920998e&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/392/998. Originally published in: 2009MNRAS.392..998E

Computer Science

Qsos, Redshifts, Equivalent Widths

Scientific paper

We selected sub-DLAs from the compilation of Rao et al. (2006, Cat. ) for follow-up spectroscopy at high resolution, obtaining new echelle spectra of 13 quasi-stellar objects (QSOs) with 17 absorbers along their lines of sight. Nine of these QSOs were observed with UVES at the VLT and four with the High-Resolution Echelle Spectrograph (HIRES) at the Keck telescope. The observations and data reduction are described in detail in Dessauges-Zavadsky et al. (in preparation).
(1 data file).

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