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A low-dispersion survey spectrograph (LDSS-2) for the William Herschel Telescope

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posted on 2024-08-06, 12:40 authored by Jeremy Allingtonsmith, Mike Breare, Richard Ellis, Dave Gellatly, Karl GlazebrookKarl Glazebrook, Paul Jorden, John Maclean, Paddy Oates, Graham Shaw, Nial Tanvir, Keith Taylor, Philip Taylor, John WebsterJohn Webster, Sue Worswick
LDSS-2 is a wide-field, multiaperture spectrograph recently installed on the 4.2-m William Herschel Telescope (WHT) in La Palma. The spectrograph has high system throughput (including the telescope and atmosphere) of similar to 20% at blaze. The field of view is 11.5 arcmin, allowing it to produce spectra of several tens of objects simultaneously at spectral resolutions up to R = 1000. The multiaperture masks are of exceptional quality and can be designed and manufactured rapidly at the telescope to improve target-mask registration and observational flexibility. This paper describes the instrument, the mask manufacturing facility, and the observing procedures required to acquire the target fields. Finally it presents examples of data obtained during the first commissioning run.

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ISSN

0004-6280

Journal title

Publications of the Astronomical Society of the Pacific

Volume

106

Issue

703

Pagination

8 pp

Publisher

University of Chicago Press

Copyright statement

Copyright © 1994 The Astronomical Society of the Pacific. The published version is reproduced in accordance with the copyright policy of the publisher.

Language

eng

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