Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-27T00:36:31.226Z Has data issue: false hasContentIssue false
  • English
  • Français

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: [email protected]
S.K. Balayan
Affiliation:
Byurakan Astrophysical Observatory (BAO), Byurakan 378433, Armenia. E-mail: [email protected]
S.A. Hakopian
Affiliation:
Byurakan Astrophysical Observatory (BAO), Byurakan 378433, Armenia. E-mail: [email protected]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

References

Afanasiev, V.L. et al. 1995, at http://www.sao.ru/bta/bta6m.html#instr Google Scholar
Balayan, S.K., Hakopian, S.A., Mickaelian, A.M., & Burenkov, A.N. 2001, AstL, 27, 284 Google Scholar
IRAS 1988, IRAS Catalogs and Atlases, 2. The Point Source Catalog, Joint IRAS Science Working Group, NASA, Washington, DC: US GPO Google Scholar
Markarian, B.E., Lipovetski, V.A., Stepanian, J.A., Erastova, L.K., Shapovalova, A.I. 1989, Commun. Special Astrophys. Obs., 62, 5 Google Scholar
Mickaelian, A.M. 1995, Ap, 38, 349 Google Scholar
Mickaelian, A.M. 2001, Ap, 44, 185 Google Scholar
Mickaelian, A.M., Hakopian, S.A., Balayan, S.K., Burenkov, A.N., 1998, AstL, 24, 736 Google Scholar
Mickaelian, A.M., Hakopian, S.A., Balayan, S.K. 1999, Proceedings of the IAU Symposium No. 194., ASP, 156 Google Scholar
Mickaelian, A.M., Véron-Cetty, M.-P., Véron, P. 2001, ASP Conference Series No. 232, 278 Google Scholar
Veilleux, S., Osterbrock, D.E., 1987, ApJS 63, 295 CrossRefGoogle Scholar
Véron, P., Gonçalves, A.C., Véron-Cetty, M.-P., 1997, A&A, 319, 52 Google Scholar