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The FLAIR–DENIS Redshift Survey

Published online by Cambridge University Press:  05 March 2013

Q. A. Parker ,
M. Colless  and
G. Mamon
Q. A. Parker
Affiliation:
Anglo-Australian Observatory, Coonabarabran, NSW 2357, Australia. qap@aaocbnu1.aao.gov.au
M. Colless
Affiliation:
Mt Stromlo & Siding Spring Observatories, Private Bag, Weston, ACT 2611, Australia.
G. Mamon
Affiliation:
IAP, Blvd Arago, F-75014, Paris, France.
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Abstract

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The DEep Near-Infrared Survey of the southern sky (DENIS) will produce an important by-product: a clean, complete view of the local Universe to z ∼ 0·07 for 105 galaxies. We identify the FLAIR multi-fibre system on the UKST as an extremely competitive facility to undertake follow-up spectroscopy for this sample due to the need to cover wide areas of sky and observe thousands of objects to a relatively bright (B < 17·5) magnitude.

Type
Hi in the Local Universe
Information
Publications of the Astronomical Society of Australia , Volume 14 , Issue 1 , 1997 , pp. 125 - 126
Copyright
Copyright © Astronomical Society of Australia 1997

References

Parker, Q. A. 1996, Spectrum, 10, 20 Google ScholarPubMed
Rieke, G. H., Reike, M. J., & Paul, A. E. 1993, ApJ, 336, 752 CrossRefGoogle Scholar
Rix, H. W. 1993, PASP, 105, 999 CrossRefGoogle Scholar