This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.

The Rapidly Flaring Afterglow of the Very Bright and Energetic GRB 070125

FREE ISSUE

Adria C. Updike1, Josh B. Haislip2, Melissa C. Nysewander3, Andrew S. Fruchter3, D. Alexander Kann4, Sylvio Klose4, Peter A. Milne5, G. Grant Williams6, Weikang Zheng7, Carl W. Hergenrother8, Jason X. Prochaska9, Jules P. Halpern10, Nestor Mirabal10, John R. Thorstensen11, Alexander J. van der Horst12, Rhaana L. C. Starling13, Judith L. Racusin14, David N. Burrows14, N. P. M. Kuin15, Peter W. A. Roming14, Eric Bellm16, Kevin Hurley16, Weidong Li17, Alexei V. Filippenko17, Cullen Blake18, Dan Starr17, Emilio E. Falco19, Warren R. Brown18, Xinyu Dai20, Jinsong Deng7, Liping Xin7, Yulei Qiu7, Jianyan Wei7, Yuji Urata21,22, Domenico Nanni23,24, Elisabetta Maiorano25, Eliana Palazzi25, Giuseppe Greco26, Corrado Bartolini26, Adriano Guarnieri26, Adalberto Piccioni26, Graziella Pizzichini25, Federica Terra23, Kuntal Misra27,28, B. C. Bhatt29, G. C. Anupama30, X. Fan5, L. Jiang5, Ralph A. M. J. Wijers31, Daniel E. Reichart2, Hala A. Eid1, Ginger Bryngelson1, Jason Puls1, R. C. Goldthwaite1, and Dieter H. Hartmann1

Show affiliations

We report on multiwavelength observations, ranging from X-ray to radio wave bands, of the IPN-localized gamma-ray burst GRB 070125. Spectroscopic observations reveal the presence of absorption lines due to O I, Si II, and C IV, implying a likely redshift of z = 1.547. The well-sampled light curves, in particular from 0.5 to 4 days after the burst, suggest a jet break at 3.7 days, corresponding to a jet opening angle of ~7.0°, and implying an intrinsic GRB energy in the 1-10,000 keV band of around Eγ = (6.3–6.9) × 1051 ergs (based on the fluences measured by the gamma-ray detectors of the IPN). GRB 070125 is among the brightest afterglows observed to date. The SED implies a host extinction of AV < 0.9 mag . Two rebrightening episodes are observed, one with excellent time coverage, showing an increase in flux of 56% in ~8000 s. The evolution of the afterglow light curve is achromatic at all times. Late-time observations of the afterglow do not show evidence for emission from an underlying host galaxy or supernova. Any host galaxy would be subluminous, consistent with current GRB host galaxy samples. Evidence for strong Mg II absorption features is not found, which is perhaps surprising in view of the relatively high redshift of this burst and the high likelihood for such features along GRB-selected lines of sight.

Subject headings

gamma rays: bursts


Dates

Issue 1 (2008 September 20)

Received 2008 February 4, accepted for publication 2008 May 7

Metrics

Total article downloads: 499

More metrics

Permissions

Get permission to re-use this article



View by subject



Export