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Wide-Field Galaxy and Cluster Surveys Using Cosmos

Published online by Cambridge University Press:  26 July 2016

H.T. MacGillivray  and
D.J. Yentis
H.T. MacGillivray
Affiliation:
Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, Scotland
D.J. Yentis
Affiliation:
Naval Research Laboratory, 4130 Overlook Avenue, Washington D.C., USA

Extract

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We have recently completed a catalogue of ∼ 5 million galaxies in the Southern sky down to a limit of bj = 20.5. The catalogue is based on the ROE/NRL Southern Sky Object Catalogue (Yentis et al. 1992), which is the result of processing of scans made with the COSMOS machine at the Royal Observatory Edinburgh (ROE) on glass copies of the IIIa-J survey carried out with the UK Schmidt Telescope (UKST) in Australia. The ‘COSMOS/UKST Southern Sky Galaxy Catalogue’ is based on 500 fields with |b| > 25 degrees and outwith the Magellanic Clouds.

Type
Part Thirteen: Properties and Clustering of Galaxies and Clusters
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 632 - 634
Copyright
Copyright © Kluwer 1994 

References

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Yentis, D.J., Cruddace, R.G., Gursky, H., Stuart, B.V., Wallin, J.F., MacGillivray, H.T. and Collins, C.A., 1992. In ‘Digitised Optical Sky Surveys’, eds. MacGillivray, H.T. and Thomson, E.B., Kluwer Academic Publishers, Dordrecht, p. 67.Google Scholar