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Trigger Simulations for GRB Detection with the Swift Burst Alert Telescope

Published online by Cambridge University Press:  05 September 2012

Amy Lien ,
Takanori Sakamoto ,
Neil Gehrels ,
David Palmer  and
Carlo Graziani
Amy Lien
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA email: [email protected]; [email protected]; [email protected] ORAU
Takanori Sakamoto
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA email: [email protected]; [email protected]; [email protected] CRESST/UMBC
Neil Gehrels
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA email: [email protected]; [email protected]; [email protected]
David Palmer
Affiliation:
Los Alamos National Lab, B244, Los Alamos, NM 87545, USA email: [email protected]
Carlo Graziani
Affiliation:
Department of Astronomy and Astrophysics, University of Chicago 5640 South Ellis Avenue, Chicago, IL 60637, USA email: [email protected]
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Abstract

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Understanding the intrinsic cosmic long gamma-ray burst (GRB) rate is essential in many aspects of astrophysics and cosmology, such as revealing the connection between GRBs, supernovae (SNe), and stellar evolution. Swift, a multi-wavelength space telescope, is quickly expanding the GRB category by observing hundreds of GRBs and their redshifts. However, it remains difficult to determine the intrinsic GRB rate due to the complex trigger algorithm adopted by Swift. Current studies of the GRB rate usually approximate the Swift trigger algorithm by a single detection threshold. Nevertheless, unlike the previously flown GRB instruments, Swift has over 500 trigger criteria based on count rates and additional thresholds for localization. To investigate possible systematic biases and further explore the intrinsic GRB rate as a function of redshift and the GRB luminosity function, we adopt a Monte Carlo approach by simulating all trigger criteria used by Swift. A precise estimation of the intrinsic GRB rate is important to reveal the GRB origins and their relation to the black-hole forming SNe. Additionally, the GRB rate at high redshifts provides a strong probe of the star formation history in the early universe, which is hard to measure directly through other methods.

Keywords

Gamma-ray Bursts
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S279: Death of Massive Stars: Supernovae and Gamma-Ray Bursts , April 2011 , pp. 347 - 348
Copyright
Copyright © International Astronomical Union 2012

References

Fynbo, J. P. U., Jakobsson, P., Prochaska, J. X., et al. 2009, ApJS, 185, 526CrossRefGoogle Scholar
Graziani, C. 2003, Gamma-Ray Burst and Afterglow Astronomy 2001: 662, 79CrossRefGoogle Scholar
Norris, J. P., Bonnell, J. T., Kazanas, D., et al. 2005, ApJ, 627, 324CrossRefGoogle Scholar
Sakamoto, T., Sato, G., Barbier, L., et al. 2009, ApJ, 693, 922CrossRefGoogle Scholar
Wanderman, D. & Piran, T. 2010, mnras, 406, 1944Google Scholar
Fenimore, E. E., Palmer, D., Galassi, M., et al. 2003, Gamma-Ray Burst and Afterglow Astronomy 2001: 662, 491CrossRefGoogle Scholar