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GRB 070707: the first short gamma-ray burst observed by INTEGRAL
KTH, School of Engineering Sciences (SCI), Physics. KTH, School of Biotechnology (BIO), Centres, Albanova VinnExcellence Center for Protein Technology, ProNova.
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2008 (English)In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 486, no 2, 405-410 p.Article in journal (Refereed) Published
Abstract [en]

Context. INTEGRAL has observed 47 long-duration GRBs (T-90 greater than or similar to 2 s) and 1 short-duration GRB (T-90 less than or similar to 2 s) in five years of observation since October 2002. Aims. This work presents the properties of the prompt emission of GRB 070707, which is the first short hard GRB observed by INTEGRAL. Methods. The spectral and temporal properties of GRB 070707 were determined using the two sensitive coded-mask gamma-ray instruments on board INTEGRAL, IBIS and SPI. Results. The T-90 duration was 0.8 s, and the spectrum of the prompt emission was obtained by joint deconvolution of IBIS and SPI data to yield a best fit power-law with photon index alpha = -1.19(-0.13)(+0.14) , which is consistent with the characteristics of short-hard gamma-ray bursts. The peak flux over 1 s was 1.79(-0.21)(+0.06) photons cm(-2) s(-1) and the fluence over the same interval was (2.07(-0.32)(+0.06) ) x 10(-7) erg cm(-2) in the energy range 20-200 keV. The spectral lag measured between 25-50 keV and 100-300 keV is 20 +/- 5 ms, consistent with the small or negligible lags measured for short bursts. Conclusions. The spectral and temporal properties of GRB 070707 are comparable to those of the short hard bursts detected by other gamma-ray satellites, including BATSE and Swift. We estimate a lower limit on the Lorentz factor Gamma greater than or similar to 25 for GRB 070707, assuming the typical redshift for short GRBs of z = 0.35. This limit is consistent with previous estimates for short GRBs and is smaller than the lower limits of Gamma greater than or similar to 100 calculated for long GRBs. If GRB 070707 is a member of the recently postulated class of short GRBs at z similar to 1, the lower limit on Gamma increases to Gamma greater than or similar to 35.

Place, publisher, year, edition, pages
2008. Vol. 486, no 2, 405-410 p.
Keyword [en]
gamma rays : bursts, gamma rays : observations
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Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-36341DOI: 10.1051/0004-6361:20079295ISI: 000257551800010Scopus ID: 2-s2.0-47249141934OAI: oai:DiVA.org:kth-36341DiVA: diva2:430615
Note
QC 20110711Available from: 2011-07-11 Created: 2011-07-11 Last updated: 2017-12-11Bibliographically approved

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