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BL Lacs from the EMSS: Number-counts and implications for the luminosity functionBL Lac objects, extracted from the Einstein Extended Medium Sensitivity Survey (EMSS), are examined. X-ray selection proved to be a powerful tool to find new BL Lacs, and allows the creation of complete, well defined and sizable samples. X-ray selected BL Lac objects (XBL) have in general more starlight in the optical spectra than radio selected BL Lacs. Redshifts for a significant fraction of objects in samples of XBL can be determined. It is thus possible to study the cosmological properties of BL Lac objects. Different models of luminosity functions of BL Lacs, including relativistic beaming, are considered and integrated over luminosity and redshift. The results are compared with the observed number-counts. The observed redshift distribution and the models' predictions are analyzed.
Document ID
19900016533
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Wolter, Anna
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA., United States)
Gioia, Isabella M.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA., United States)
Maccacaro, Tommaso
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA., United States)
Schild, Rudy E.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA., United States)
Morris, Simon L.
(Carnegie Institution of Washington Pasadena, CA., United States)
Stocke, John T.
(Colorado Univ. Boulder., United States)
Date Acquired
September 6, 2013
Publication Date
November 1, 1989
Publication Information
Publication: ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 2: AGN and the X Ray Background
Subject Category
Astronomy
Accession Number
90N25849
Funding Number(s)
CONTRACT_GRANT: NAS8-30751
Distribution Limits
Public
Copyright
Other
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