The rapidly flaring afterglow of the very bright and energetic GRB 070125

Adria C. Updike, Josh B. Haislip, Melissa C. Nysewander, Andrew S. Fruchter, D. Alexander Kann, Sylvio Klose, Peter A. Milne, G. Grant Williams, Weikang Zheng, Carl W. Hergenrother, Jason X. Prochaska, Jules P. Halpern, Nestor Mirabal, John R. Thorstensen, Alexander J. Van Der Horst, Rhaana L.C. Starling, Judith L. Racusin, David N. Burrows, N. P.M. Kuin, Peter W.A. RomingEric Bellm, Kevin Hurley, Weidong Li, Alexei V. Filippenko, Cullen Blake, Dan Starr, Emilio E. Falco, Warren R. Brown, Xinyu Dai, Nsono Deng, Liping Xin, Yulei Qiu, Jianyan Wei, Yuji Urata, Domenico Nanni, Elisabetta Maiorano, Eliana Palazzi, Giuseppe Greco, Corrado Bartolini, Adriano Guarnieri, Adalberto Piccioni, Graziella Pizzichini, Federica Terra, Kuntal Misra, B. C. Bhatt, G. C. Anupama, X. Fan, L. Jiang, Ralph A.M.J. Wuers, Daniel E. Reichart, Hala A. Eid, Ginger Bryngelson, Jason Puls, R. C. Goldthwaite, Dieter H. Hartmann

Research output: Contribution to journalArticle

23 Scopus citations

Abstract

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 ajet 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, snowing 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.

Original languageEnglish (US)
Pages (from-to)361-375
Number of pages15
JournalAstrophysical Journal
Volume685
Issue number1
DOIs
StatePublished - Sep 20 2008

Keywords

  • Gamma rays: bursts

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Updike, A. C., Haislip, J. B., Nysewander, M. C., Fruchter, A. S., Kann, D. A., Klose, S., Milne, P. A., Williams, G. G., Zheng, W., Hergenrother, C. W., Prochaska, J. X., Halpern, J. P., Mirabal, N., Thorstensen, J. R., Van Der Horst, A. J., Starling, R. L. C., Racusin, J. L., Burrows, D. N., Kuin, N. P. M., ... Hartmann, D. H. (2008). The rapidly flaring afterglow of the very bright and energetic GRB 070125. Astrophysical Journal, 685(1), 361-375. https://doi.org/10.1086/590236