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The Byurakan-IRAS Galaxy (BIG) Sample: The Redshift Survey

Published online by Cambridge University Press:  12 April 2016

A.M. Mickaelian ,
S.K. Balayan  and
S.A. Hakopian
A.M. Mickaelian
Affiliation:
Byurakan Astrophysical Observatory (BAO), Byurakan 378433, Armenia. E-mail: aregmick@bao.sci.am
S.K. Balayan
Affiliation:
Byurakan Astrophysical Observatory (BAO), Byurakan 378433, Armenia. E-mail: aregmick@bao.sci.am
S.A. Hakopian
Affiliation:
Byurakan Astrophysical Observatory (BAO), Byurakan 378433, Armenia. E-mail: aregmick@bao.sci.am

Abstract

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The Byurakan-IRAS Galaxy (BIG) sample (1967 galaxies) is based on optical identifications of IRAS PSC sources at δ>+61° and |b| >15° (FBS area). A redshift survey for brighter objects (B<18m) is being carried out with the Byurakan Observatory 2.6m, Special Observatory 6m, and Observatoire de Haute-Provence 1.93m telescopes. 213 objects have been observed, and redshifts in the range 0.008-0.173 have been measured. For this subsample, 15% of the objects are AGNs, and 15% are LIGs and ULIGs.

Type
Part 2. Infrared and Submillimeter Surveys for AGN
Information
International Astronomical Union Colloquium , Volume 184: AGN Surveys , 2002 , pp. 217 - 219
Copyright
Copyright © Astronomical Society of the Pacific 2002

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