| Autor: |
A. R. Rao, Vikas Chand, M. K. Hingar, S. Iyyani, Rakesh Khanna, A. P. K. Kutty, J. P. Malkar, D. Paul, V. B. Bhalerao, D. Bhattacharya, G. C. Dewangan, Pramod Pawar, A. M. Vibhute, T. Chattopadhyay, N. P. S. Mithun, S. V. Vadawale, N. Vagshette, R. Basak, P. Pradeep, Essy Samuel |
| Předmět: |
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| Zdroj: |
Astrophysical Journal; 12/10/2016, Vol. 833 Issue 1, p1-1, 1p |
| Abstrakt: |
AstroSat is a multi-wavelength satellite launched on 2015 September 28. The CZT Imager of AstroSat on its very first day of operation detected a long duration gamma-ray burst (GRB), namely GRB 151006A. Using the off-axis imaging and spectral response of the instrument, we demonstrate that the CZT Imager can localize this GRB correctly to about a few degrees, and it can provide, in conjunction with Swift, spectral parameters similar to those obtained from Fermi/GBM. Hence, the CZT Imager would be a useful addition to the currently operating GRB instruments (Swift and Fermi). Specifically, we argue that the CZT Imager will be most useful for the short hard GRBs by providing localization for those detected by Fermi and spectral information for those detected only by Swift. We also provide preliminary results on a new exciting capability of this instrument: the CZT Imager is able to identify Compton scattered events thereby providing polarization information for bright GRBs. GRB 151006A, in spite of being relatively faint, shows hints of a polarization signal at 100–300 keV (though at a low significance level). We point out that the CZT Imager should provide significant time resolved polarization measurements for GRBs that have fluence three times higher than that of GRB 151006A. We estimate that the number of such bright GRBs detectable by the CZT Imager is five to six per year. The CZT Imager can also act as a good hard X-ray monitoring device for possible electromagnetic counterparts of gravitational wave events. [ABSTRACT FROM AUTHOR] |
| Databáze: |
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