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Objective-Prism Redshifts of Faint Galaxies
Published online by Cambridge University Press: 12 April 2016
Abstract
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A large sample of spectra of faint galaxies has been obtained using COSMOS measurements of UKST objective-prism plates. Computer software has been developed to obtain the radial velocities of large numbers of these galaxies automatically over a magnitude range of about B = 16 to 19. Initial tests have been performed on a sample of about 1400 galaxies from an area of about 5 x 4 degrees square.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 78: Astronomy with Schmidt-type telescopes , 1984 , pp. 401 - 403
- Copyright
- Copyright © Reidel 1984
References
Beard, S.M., Cooke, J.A., Emerson, D., Kelly, B.D.: 1983, submitted to Mon. Not. R. astr. Soc.
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Cooke, J.A., Emerson, D., Beard, S.M. and Kelly, B.D.: 1982, “Workshop on Astronomical Measuring Machines 1982”, occasional reports of the Roy. Obs., Edinburgh, 10, pp. 209–218
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