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The Catalina Real-time Transient Survey

Published online by Cambridge University Press:  20 April 2012

A. J. Drake ,
S. G. Djorgovski ,
A. Mahabal ,
J. L. Prieto ,
E. Beshore ,
M. J. Graham ,
M. Catalan ,
S. Larson ,
E. Christensen  and
C. Donalek
...Show all authors
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.

Keywords

(stars:) supernovæ: general(galaxies:) BL Lacertae objects: generalstars: dwarf novæ starsstars: flaregalaxies: dwarf
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S285: New Horizons in Time-Domain Astronomy , September 2011 , pp. 306 - 308
Copyright
Copyright © International Astronomical Union 2012

References

Della Valle, M. & Panagia, N. 2003, ApJ, 587, L71Google Scholar
Drake, A. J., et al. , 2009a, ApJ, 696, 87Google Scholar
Drake, A. J., et al. , 2009b, CBET, 1958Google Scholar
Drake, A. J., et al. , 2009c, CBET, 1766Google Scholar
Drake, A. J., et al. , 2010, ApJ, 718, 127Google Scholar
Drake, A. J., et al. , 2011a, APJ, 735, 106Google Scholar
Drake, A. J., et al. , 2011b, ATEL, 3343Google Scholar
Drake, A. J., et al. , 2011c, ApJ, arXiv:1009.308Google Scholar
Djorgovski, S. G., et al. , 2011, JAXA, in press, arXiv:1102.5004Google Scholar
Filippenko, A., Li, W. D., Treffers, R. R., & Modjaz, M. 2001, PASP Conf Ser., 246, 121Google Scholar
Kauffmann, G., et al. , 2003, MNRAS, 341, 33Google Scholar
Kozlowski, S., et al. , 2010, ApJ, 722, 1624Google Scholar
Mahabal, A. et al. , 2009, ATEL, 1713, 1Google Scholar
Neill, J., et al. , 2011, ApJ, 727, 15CrossRefGoogle Scholar
Pastorello, A. et al. , 2010a, CBET, 2413Google Scholar
Pastorello, A. et al. , 2010b, ApJ, 724, 16LGoogle Scholar
Quimby, R. et al. , 2007, ApJ, 668, 99Google Scholar
Quimby, R. et al. , 2011, NATURE, 474, 487Google Scholar
Stanek, K. Z., et al. , 2006, AcA, 56, 333Google Scholar
Stoll, R., et al. , 2011, ApJ, 730, 34Google Scholar
Tremonti, C. et al. , 2014, ApJ, 613, 898Google Scholar