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Optical and Far-Infrared Properties of UM Survey Emission-Line Galaxies

Published online by Cambridge University Press:  07 August 2017

Gordon M. MacAlpine  and
John J. Salzer
Gordon M. MacAlpine
Affiliation:
Department of Astronomy, University of Michigan, Ann Arbor, MI 48109
John J. Salzer
Affiliation:
Arecibo Observatory, P.O. Box 995, Arecibo, PR 00613

Extract

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For the University of Michigan (UM) survey, the Curtis Schmidt telescope at CTIO is used with Kodak IIIa-J plates and the 1.°8 objective prism to detect emission-line galaxies (ELGs) and quasars. Line emission is the primary selection criterion. The quasar sample has been investigated by Lewis, MacAlpine, and Weedman (1979) and by MacAlpine and Feldman (1982) while a study of the ELGs was begun by Lewis (1983). Here, we report on a more extensive analysis of the 172 ELG candidates in the UM Lists IV (MacAlpine and Lewis 1978) and V (MacAlpine and Williams 1981) areas.

Type
Part 7: Dust, Molecules, Infrared and MM Radiation
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 400 - 401
Copyright
Copyright © Kluwer 1989 

References

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