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The Catalina Real-time Transient Survey

Published online by Cambridge University Press:  20 April 2012

A. J. Drake
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA. email: [email protected]
S. G. Djorgovski
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA. email: [email protected] Distinguished Visiting Professor, King Abdulaziz Univ., Jeddah, Saudi Arabia.
A. Mahabal
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA. email: [email protected]
J. L. Prieto
Affiliation:
Dept. of Astrophysical Scinces, Princeton University, NJ 08544, USA.
E. Beshore
Affiliation:
Lunar and Planetary Lab, University of Arizona, Tucson, AZ 85721, USA.
M. J. Graham
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA. email: [email protected]
M. Catalan
Affiliation:
Depto. de Astronomia y Astrofisica, Pont. Uni. Catolica de Chile, Santiago, Chile.
S. Larson
Affiliation:
Lunar and Planetary Lab, University of Arizona, Tucson, AZ 85721, USA.
E. Christensen
Affiliation:
Gemini South Observatory, c/o AURA, Casilla 603, La Serena, Chile.
C. Donalek
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA. email: [email protected]
R. Williams
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA. email: [email protected]
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Abstract

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The Catalina Real-time Transient Survey (CRTS) currently covers 33,000 deg2 of the sky in search of transient astrophysical events, with time base-lines ranging from 10 minutes to ~7 years. Data provided by the Catalina Sky Survey provide an unequalled base-line against which > 4,000 unique optical transient events have been discovered and openly published in real-time. Here we highlight some of the discoveries of CRTS.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

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