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Exploring the Time Domain with Synoptic Sky Surveys

Published online by Cambridge University Press:  20 April 2012

S. G. Djorgovski ,
A. A. Mahabal ,
A. J. Drake ,
M. J. Graham ,
C. Donalek  and
R. Williams
S. G. Djorgovski
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA email: george@astro.caltech.edu
A. A. Mahabal
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA email: george@astro.caltech.edu
A. J. Drake
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA email: george@astro.caltech.edu
M. J. Graham
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA email: george@astro.caltech.edu
C. Donalek
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA email: george@astro.caltech.edu
R. Williams
Affiliation:
California Institute of Technology, Pasadena, CA 91125, USA email: george@astro.caltech.edu
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Abstract

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Synoptic sky surveys are becoming the largest data generators in astronomy, and they are opening a new research frontier that touches practically every field of astronomy. Opening the time domain to a systematic exploration will strengthen our understanding of a number of interesting known phenomena, and may lead to the discoveries of as yet unknown ones. We describe some lessons learned over the past decade, and offer some ideas that may guide strategic considerations in the planning and execution of future synoptic sky surveys.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S285: New Horizons in Time-Domain Astronomy , September 2011 , pp. 141 - 146
Copyright
Copyright © International Astronomical Union 2012

References

Bauer, A., et al. , 2009, ApJ, 705, 46CrossRefGoogle Scholar
Djorgovski, S. G., et al. , 2001a, ASPCS, 225, 52Google Scholar
Djorgovski, S. G., et al. , 2001b, in Mining the Sky, eds. Banday, A. et al. , ESO Astroph. Symp., p. 305, Berlin: Springer-VerlagGoogle Scholar
Djorgovski, S. G., et al. , 2008, AN, 329, 263Google Scholar
Djorgovski, S. G., et al. , 2011a, in: eds. Mihara, T. & Kawai, N. (eds.), The First Year of MAXI: Monitoring Variable X-ray Sources (Tokyo: JAXA Special Publ.), in pressGoogle Scholar
Djorgovski, S. G., et al. , 2011b, in: Srivasatava, A., Chawla, N. V. and Perera, A. S. (eds.), CIDU Conf. 2011, (NASA), p. 174.Google Scholar
Donalek, C., et al. , 2008, AIPC, 1082, 252Google Scholar
Drake, A. J., et al. , 2009, ApJ, 696, 870CrossRefGoogle Scholar
Drake, A. J., et al. , 2010, ApJ, 718, L127CrossRefGoogle Scholar
Drake, A. J., et al. , 2011, ApJ, 738, 125Google Scholar
Drake, A. J., et al. , 2012, ApJ, submitted (arXiv/1009.3048)Google Scholar
Granett, B., et al. , 2003, BAAS, 35, 1300Google Scholar
Harwit, M. 1975, QJRAS, 16, 378Google Scholar
Mahabal, A. A., et al. , 2001, BAAS, 33, 1461Google Scholar
Mahabal, A. A., et al. , 2008, AN, 329, 288Google Scholar
Mahabal, A. A., et al. , 2011, BASI, 39, 387Google Scholar
Paczyński, B. 2000, PASP, 112, 1281CrossRefGoogle Scholar
Rau, A. et al. , 2009, PASP, 121, 1334Google Scholar
Tonry, J. 2011, PASP, 123, 58Google Scholar
Williams, R., et al. , 2009, ASPCS, 411, 115Google Scholar
Zwicky, F. 1957, Morphological Astronomy, (Berlin: Springer-Verlag)Google Scholar