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Feasibility of a Small, Rapid Optical/IR Response, Next Generation Gamma-Ray Burst Mission

Published online by Cambridge University Press:  22 July 2013

B. Grossan ,
G.F. Smoot ,
V.V. Bogomolov ,
S.I. Svertilov ,
N.N. Vedenkin ,
M. Panasyuk ,
B. Goncharov ,
G. Rozhkov ,
K. Saleev  and
E. Grobovskoj
...Show all authors
B. Grossan
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation University of California at Berkeley Space Sciences Laboratory, USA
G.F. Smoot
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation University of California at Berkeley, USA
V.V. Bogomolov
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation
S.I. Svertilov
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation
N.N. Vedenkin
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation
M. Panasyuk
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation
B. Goncharov
Affiliation:
Moscow State University, Russian Federation
G. Rozhkov
Affiliation:
Moscow State University, Russian Federation
K. Saleev
Affiliation:
Moscow State University, Russian Federation
E. Grobovskoj
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation
A.S. Krasnov
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation
V.S. Morozenko
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation
V.I. Osedlo
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation
E. Rogkov
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation
T.V. Vachenko
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation
E.V. Linder
Affiliation:
Extreme Universe Laboratory, Moscow State University, Russian Federation University of California at Berkeley Space Sciences Laboratory, USA
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Abstract

We present motivations for and study feasibility of a small, rapid-optical/IR response gamma-ray burst (GRB) space observatory. By analyzing existing GRB data, we give realistic detection rates for X-ray and optical/IR instruments of modest size under actual flight conditions. Given new capabilities of fast optical/IR response (~1 s to target) and simultaneous multi-band imaging, such an observatory can have a reasonable event rate, likely leading to new science. Requiring a Swift-like orbit, duty cycle, and observing constraints, a Swift-BAT scaled down to 190 cm2 of detector area would still detect and locate about 25 GRB yr-1 for a trigger threshold of 6.5σ. About 23% of X–ray located GRB would be detected optically for a 10 cm diameter instrument (~6 yr-1 for the 6.5σ X-ray trigger).

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. 633 - 637
Copyright
© EAS, EDP Sciences 2013

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References

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