Early optical brightening in grb 071010b

J. H. Wang, M. E. Schwamb, K. Y. Huang, C. Y. Wen, Z. W. Zhang, S. Y. Wang, W. P. Chen, F. B. Bianco, R. Dave, M. J. Lehner, S. L. Marshall, R. Porrata, C. Alcock, Y. I. Byun, K. H. Cook, S. K. King, T. Lee, Y. Urata

Research output: Contribution to journalArticlepeer-review

13 Citations (Scopus)


We report the detection of early (60-230 s) optical emission of the gamma-ray burst afterglow of GRB 071010B. No significant correlation with the prompt γ-ray emission was found. Our high time resolution data combining with other measurements within 2 days after the burst indicate that GRB 071010B is composed of a weak early brightening (α ∼ 0.6), probably caused by the peak frequency passing through the optical wavelengths, followed by a decay (α∼0.51), attributed to continuous energy injection by patchy jets.

Original languageEnglish
Pages (from-to)L5-L8
JournalAstrophysical Journal
Issue number1 PART 2
Publication statusPublished - 2008

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science


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