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Variable Stellar Object Detection and Light Curves from the Solar Mass Ejection Imager (SMEI)

Published online by Cambridge University Press:  20 April 2012

R. A. Hounsell ,
M. F. Bode ,
M. J. Darnley ,
D. J. Harman ,
P. P Hick ,
A. Buffington ,
B. V. Jackson ,
J. M. Clover  and
A. W. Shafter
R. A. Hounsell
Affiliation:
Astrophysics Research Institute, Liverpool JMU, Birkenhead, CH41 1LD, UK email: [email protected]
M. F. Bode
Affiliation:
Astrophysics Research Institute, Liverpool JMU, Birkenhead, CH41 1LD, UK email: [email protected]
M. J. Darnley
Affiliation:
Astrophysics Research Institute, Liverpool JMU, Birkenhead, CH41 1LD, UK email: [email protected]
D. J. Harman
Affiliation:
Astrophysics Research Institute, Liverpool JMU, Birkenhead, CH41 1LD, UK email: [email protected]
P. P Hick
Affiliation:
San Diego Supercomputer Center, University of California, La Jolla, CA 92093, USA
A. Buffington
Affiliation:
Center for Astrophysics and Space Sciences, Univ. of California, La Jolla, CA 92093, USA
B. V. Jackson
Affiliation:
Center for Astrophysics and Space Sciences, Univ. of California, La Jolla, CA 92093, USA
J. M. Clover
Affiliation:
Center for Astrophysics and Space Sciences, Univ. of California, La Jolla, CA 92093, USA
A. W. Shafter
Affiliation:
Department of Astronomy, San Diego State University, San Diego, CA 92182, USA
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Abstract

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With the advent of surveys such as the Catalina Real-Time Transient Survey, the Palomar Transient Factory, Pan-STARRS and Gaia, the search for variable objects and transient events is rapidly accelerating. There are, however important existing data-sets from instruments not originally designed to find such events. One example of such an instrument is the Solar Mass Ejection Imager (SMEI), an all-sky space-based differential photometer which is able to produce light curves of bright objects (m ≤ 8) with a 102-minute cadence. In this paper we discuss the use of such an instrument for investigations of novæ, and outline future plans to find other variable objects with this hitherto untapped resource.

Keywords

stars: novæ, cataclysmic variablesastronomical data bases: miscellaneousinstrumentation: photometers
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S285: New Horizons in Time-Domain Astronomy , September 2011 , pp. 91 - 94
Copyright
Copyright © International Astronomical Union 2012

References

Bode, M. F., et al. 2006, ApJ, 652, 629CrossRefGoogle Scholar
Buffington, A., et al. 2007, SPIE, 6689.Google Scholar
Buffington, A., Band, D. L., Jackson, B. V., Hick, P. P., Smith, A. C., 2006, ApJ, 637, 880CrossRefGoogle Scholar
Darnley, M. J., et al. 2006, MNRAS, 369, 257CrossRefGoogle Scholar
Eyles, C. J., et al. 2003, Solar Phys, 217, 319CrossRefGoogle Scholar
Hick, P., Buffington, A., Jackson, B. V., 2007, SPIE, 6689.Google Scholar
Hounsell, R., et al. 2011, ATel, 3373, 1Google Scholar
Hounsell, R., et al. 2010, ApJ, 724, 480CrossRefGoogle Scholar
Jackson, B. V., et al. 2004, Solar Phys, 225, 177CrossRefGoogle Scholar
Shafter, A. W., 1997, ApJ, 487, 226CrossRefGoogle Scholar
Shafter, A. W., 2002, AIPC, 637, 462Google Scholar
Steele, I. A., et al. 2004, SPIE, 5489, 679Google Scholar