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A-STAR: The All-Sky Transient Astrophysics Reporter

Published online by Cambridge University Press:  22 July 2013

J.P. Osborne ,
P. O’Brien ,
P. Evans ,
G.W. Fraser ,
A. Martindale ,
J.-L. Atteia ,
B. Cordier  and
S. Mereghetti
J.P. Osborne
Affiliation:
Dept of Physics & Astronomy, University of Leicester, LE1 7RH, UK
P. O’Brien
Affiliation:
Dept of Physics & Astronomy, University of Leicester, LE1 7RH, UK
P. Evans
Affiliation:
Dept of Physics & Astronomy, University of Leicester, LE1 7RH, UK
G.W. Fraser
Affiliation:
Dept of Physics & Astronomy, University of Leicester, LE1 7RH, UK
A. Martindale
Affiliation:
Dept of Physics & Astronomy, University of Leicester, LE1 7RH, UK
J.-L. Atteia
Affiliation:
UPS-OMP, Université de Toulouse, IRAP, Toulouse, France CNRS, IRAP, 14 avenue Edouard Belin, 31400 Toulouse, France
B. Cordier
Affiliation:
CEA, IRFU, Service d’Astrophysique, 91191 Gif-sur-Yvette, France
S. Mereghetti
Affiliation:
INAF-IASF Milan, via Bassini 15, 20133 Milano, Italy
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Abstract

The small mission A-STAR (All-Sky Transient Astrophysics Reporter) aims to locate the X-ray counterparts to ALIGO and other gravitational wave detector sources, to study the poorly-understood low luminosity gamma-ray bursts, and to find a wide variety of transient high-energy source types, A-STAR will survey the entire available sky twice per 24 hours. The payload consists of a coded mask instrument, Owl, operating in the novel low energy band 4−150 keV, and a sensitive wide-field focussing soft X-ray instrument, Lobster, working over 0.15−5 keV. A-STAR will trigger on ~100 GRBs/yr, rapidly distributing their locations.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 61: Gamma-ray Bursts: 15 Years of GRB Afterglows – Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe , 2013 , pp. 625 - 631
Copyright
© EAS, EDP Sciences 2013

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References

Abadien, J., Abbot, B.P., Abbot, R., et al., 2010, Class. Quantum Grav., 27, 173001 CrossRef
Klimenkon, S., Vedovato, G., Drago, M., et al., 2011, PhRvD, 83, 102001
The IceCube Collaboration, 2011 [arXiv:1111.2741]
Kappes, A., 2007 [arXiv:0711.0563]
Pian, E., Mazalli, P.A., Masetti, N., et al., 2006, Nature, 442, 1011 CrossRef
Racusin, J.L., Karpov, S.V., Sokolowski, M., et al., 2008, Nature, 455, 183 CrossRef
Tanvir, N.R., Fox, D.B., Levan, A.J., et al., 2009, Nature, 461, 1254 CrossRef
Tanvir, N.R., Levan, A.J., Fructer, A.S., et al., 2012, ApJ, 754, 46 CrossRef
Fynbo, J.P.U., Watson, D., Thöne, C.C., et al., 2006, Nature, 444, 1047 CrossRef
Gal-Yam, A., Fox, D.B., Price, P.A., et al., 2006, Nature, 444, 1053 CrossRef
Mereghetti, S., 2008, A&ARv, 15, 225
Soderberg, A.M., Berger, E., Page, K.L., et al., 2008, Nature, 453, 469 CrossRef
Komossa, S., Halpern, J., Schartel, N., et al., 2004, ApJ, 603, L17 CrossRef
Gezari, S., Chornock, R., Rest, A., et al., 2012, Nature, 485, 217 CrossRef
Levan, A.J., Tanvir, N.R., Cenko, S.B., et al., 2011, Science, 333, 199 CrossRef
Bloom, J.S., Giannios, D., Metzger, B., et al., 2011, Science, 333, 203 CrossRef
Burrows, D.N., Kennea, J.K., Ghisellini, G., et al., 2011, Nature, 476, 421CrossRef