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

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posted on 2024-07-26, 14:50 authored by Michael MurphyMichael Murphy, Glenn KacprzakGlenn Kacprzak, Giulia A. D. Savorgnan, Robert F. Carswell
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.

Funding

Galaxy formation and femtosecond frequency combs

Australian Research Council

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Fundamental physics in distant galaxies

Australian Research Council

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Pristine fuel for early galaxies

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The physics of gas flows around galaxies at cosmic noon

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PDF (Published version)

ISSN

1365-2966

Journal title

Monthly Notices of the Royal Astronomical Society

Volume

482

Issue

3

Pagination

21 pp

Publisher

Oxford University Press (OUP)

Copyright statement

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. Copyright © 2018 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Language

eng

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