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New Results from the REX Survey

Published online by Cambridge University Press:  12 April 2016

A. Caccianiga ,
M. J. M. Marchā ,
T. Maccacaro ,
A. Wolter ,
R. Della Ceca  and
I. M. Gioia
A. Caccianiga
Affiliation:
Observatório Astronómico de Lisboa, Tapada da Ajuda, 13Ą9-018, Portugal
M. J. M. Marchā
Affiliation:
Observatório Astronómico de Lisboa, Tapada da Ajuda, 13Ą9-018, Portugal
T. Maccacaro
Affiliation:
Osservatorio Astronomico di Brera, via Brera 28, I-20121, Milan, Italy
A. Wolter
Affiliation:
Osservatorio Astronomico di Brera, via Brera 28, I-20121, Milan, Italy
R. Della Ceca
Affiliation:
Osservatorio Astronomico di Brera, via Brera 28, I-20121, Milan, Italy
I. M. Gioia
Affiliation:
Istituto di Radio Astronomia del CNR, via Gobetti 101, Bologna, Italy

Abstract

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The REX survey is an ongoing project aimed at the selection of new samples of QSOs and BL Lac objects. Spectroscopic identification of the ~1600 sources in the survey is in progress reaching, so far, about 40% of complete identification level. In this paper, the most recent results derived from the REX survey are briefly summarized.

Type
Part 3. X-ray Surveys for AGN
Information
International Astronomical Union Colloquium , Volume 184: AGN Surveys , 2002 , pp. 257 - 258
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

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