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UK funding (£24,664): Science analysis for VIKING: the VISTA Kilo-degree Infrared Galaxy survey Ukri1 Apr 2008 UK Research and Innovation, United Kingdom

Overview

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Science analysis for VIKING: the VISTA Kilo-degree Infrared Galaxy survey

Abstract We are planning to use the new VISTA wide-field survey telescope in the Atacama desert of Chile, to make a near-infrared sky map. VISTA with its 4-metre mirror and 67-megapixel 3-tonne infrared camera will be the world's most powerful survey telescope when operational in 2008. Our map will cover two large stripes of the sky: each stripe will be approximately 75 degrees long and 10 degrees wide, and together they will cover 5 percent of the entire sky. Both stripes are directed away from the plane of our own Milky Way galaxy (one above and one below) to give a clear view of the distant universe. This area will be imaged in 5 different colours of near-infrared light, covering wavelengths between twice and 4 times that of ordinary visible light. The map will reveal objects up to 40 times fainter than existing infrared all-sky surveys. In addition, visible-light (near ultraviolet to red) images of the same area will be made by other wide-field telescopes, to give a combined survey with 9 colours. The resulting sky map will produce a catalogue of over 10 million galaxies and several million stars with this 9-colour information. Astronomers will use these for many purposes: for statistical analyses of the distribution of galaxies and stars, in particular to make a 3-dimensional map of the distribution of distant galaxies; to pinpoint objects detected by telescopes at other wavelengths; and to search for very rare objects such as the most distant quasars, which can be picked out since they will have peculiar colours unlike those of normal stars.
Category Research Grant
Reference ST/F00270X/1
Status Closed
Funded period start 01/04/2008
Funded period end 31/03/2010
Funded value £24,664.00
Source https://gtr.ukri.org/projects?ref=ST%2FF00270X%2F1

Participating Organisations

Queen Mary University of London

The filing refers to a past date, and does not necessarily reflect the current state. The current state is available on the following page: Queen Mary University of London, London.

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