4.7 Article

The UVES Spectral Quasar Absorption Database (SQUAD) data release 1: the first 10 million seconds

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 482, Issue 3, Pages 3458-3479

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/sty2834

Keywords

line: profiles; instrumentation: spectrographs; quasars: absorption lines; cosmology: miscellaneous; cosmology: observations

Funding

  1. Australian Research Council [DP0877998, DP110100866, DP130100568, DP170103470]
  2. Australian Research Council [DP0877998] Funding Source: Australian Research Council

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We present the first data release (DR1) of the LIVES Spectral Quasar Absorption Database (SQUAD), comprising 467 fully reduced, continuum-fitted high-resolution quasar spectra from the Ultraviolet and Visual Echelle Spectrograph (LIVES) on the European Southern Observatory's Very Large Telescope. The quasars have redshifts z = 0-5, and a total exposure time of 10 million seconds provides continuum-to-noise ratios of 4-342 (median 20) per 2.5 km s(-1) pixel at 5500 angstrom. The SQUAD spectra are fully reproducible from the raw, archival LIVES exposures with open-source software, including our UVES_POPLER tool for combining multiple extracted echelle exposures which we document here. All processing steps are completely transparent and can be improved upon or modified for specific applications. A primary goal of SQUAD is to enable statistical studies of large quasar and absorber samples, and we provide tools and basic information to assist three broad scientific uses: studies of damped Lyman-alpha systems (DLAs), absorption-line surveys, and time-variable absorption lines. For example, we provide a catalogue of 155 DLAs whose Lyman-alpha lines are covered by the DR1 spectra, 18 of which are reported for the first time. The H I column densities of these new DLAs are measured from the DR1 spectra. DR1 is publicly available and includes all reduced data and information to reproduce the final spectra.

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