GRB 070306: A Highly Extinguished Afterglow
Abstract
We report on the highly extinguished afterglow of GRB 070306 and the properties of the host galaxy. An optical afterglow was not detected at the location of the burst, but in near-infrared a doubling in brightness during the first night and later power-law decay in the K band provided a clear detection of the afterglow. The host galaxy is relatively bright, R ~ 22.8. An optical low resolution spectrum revealed a largely featureless host galaxy continuum with a single emission line. Higher resolution follow-up spectroscopy shows this emission to be resolved and consisting of two peaks separated by 7 AA, suggesting it to be [O II] at a redshift of z = 1.49594 +- 0.00006. The infrared color H-K = 2 directly reveals significant reddening. By modeling the optical/X-ray spectral energy distribution at t = 1.38 days with an extinguished synchrotron spectrum, we derive A_V = 5.5 +- 0.6 mag. This is among the largest values ever measured for a GRB afterglow and visual extinctions exceeding unity are rare. The importance of early NIR observations is obvious and may soon provide a clearer view into the once elusive 'dark bursts'.
Cite
@article{arxiv.0803.4017,
title = {GRB 070306: A Highly Extinguished Afterglow},
author = {A. O. Jaunsen and E. Rol and D. J. Watson and D. Malesani and J. P. U. Fynbo and B. Milvang-Jensen and J. Hjorth and P. M. Vreeswijk and J. -E. Ovaldsen and K. Wiersema and N. R. Tanvir and J. Gorosabel and A. J. Levan and M. Schirmer and A. J. Castro-Tirado},
journal= {arXiv preprint arXiv:0803.4017},
year = {2008}
}
Comments
28 pages, 6 figures, accepted for publication in ApJ