Swift Observations of GRB050603: An afterglow with a steep late time decay slope
نویسندگان
چکیده
We report the results of Swift observations of the Gamma Ray Burst GRB050603. With a V magnitude V=18.2 about 10 hours after the burst the optical afterglow was the brightest so far detected by Swift and one of the brightest optical afterglows ever seen. The Burst Alert Telescope (BAT) light curves show three fast-rise-exponential-decay spikes with T90=12s and a fluence of 7.6×10 ergs cm in the 15-150 keV band. With an Eγ,iso = 1.26× 10 54 ergs it was also one of the most energetic bursts of all times. The Swift spacecraft began observing of the afterglow with the narrow-field instruments about 10 hours after the detection of the burst. The burst was bright enough to be detected by the Swift UV/Optical telescope (UVOT) for almost 3 days and by the X-ray Telescope (XRT) for a week after the burst. The X-ray light curve shows a rapidly fading afterglow with a decay index α=1.76 −0.07. The X-ray energy spectral index was βX=0.71±0.10 with the column density in agreement with the Galactic value. The spectral analysis does not show an obvious change in the X-ray spectral slope over time. The optical UVOT light curve decays with a slope of α=1.8±0.2. The steepness and the similarity of the optical and X-ray decay rates suggest that the afterglow was observed after the jet break. We estimate a jet opening angle of about 1-2. Subject headings: GRBs:individual(GRB 050603) Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Lab, University Park, PA 16802 NASA Goddard Space Flight Center, Greenbelt, MD 20771 Department of Physics, University of Nevada, Las Vegas, NV 89154 ASI Science Data Center, via G. Galilei, I-00044 Frascati (Roma), Italy Universities Space Research Association, Seabrook, MD Department of Physics, Pennsylvania State University, University Park, PA 16802 Department of Physics & Astronomy, University of Leicester, Leicester, LE1 7R, UK Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey RH5 6NT, U.K.
منابع مشابه
The late-time afterglow of the extremely energetic short burst GRB 090510 revisited
Context. The Swift discovery of the short burst GRB 090510 has raised considerable attention mainly because of two reasons: first, it had a bright optical afterglow, and second it is among the most energetic events detected so far within the entire GRB population (long plus short). The afterglow of GRB 090510 was observed with Swift/UVOT and Swift/XRT and evidence of a jet break around 1.5 ks a...
متن کاملGRB 081028 and its late - time afterglow re - brightening
Swift captured for the first time a smoothly rising X-ray re-brightening of clear nonflaring origin after the steep decay in a long gamma-ray burst (GRB): GRB081028. A rising phase is likely present in all GRBs but is usually hidden by the prompt tail emission and constitutes the first manifestation of what is later to give rise to the shallow decay phase. Contemporaneous optical observations r...
متن کاملThe Swift gamma-ray burst GRB 050422
We describe observations of GRB 050422, a Swift-discovered gamma-ray burst. The prompt gamma-ray emission had a T90 duration of 59 s and was multipeaked, with the main peak occurring at T + 53 s. Swift was able to follow the X-ray afterglow within 100 s of the burst trigger. The X-ray light curve, which shows a steep early decline, can be described by a broken power law with an initial decay sl...
متن کاملSwift observations of the prompt X - ray emission and afterglow from GRB 050126 & GRB 050219 A
We report on the temporal and spectral characteristics of the early X-ray emission from the Gamma Ray Bursts GRB050126 and GRB050219A as observed by Swift. The X-ray light-curves of these 2 bursts both show remarkably steep early decays (F(t) ∝ t−3), breaking to flatter slopes on timescales of a few hundred seconds. For GRB050126 the burst shows no evidence of spectral evolution in the 20-150 k...
متن کاملThe early X-ray afterglows of Gamma Ray Bursts
The X-ray light curves of hundreds of bursts are now available, thanks to the X-ray Telescope on board the Swift satellite, on time scales from ∼ 1 minute up to weeks and in some cases months from the burst explosion. These data allow us to investigate the physics of the highly relativistic fireball outflow and its interaction with the circumburst environment. Here we review the main results of...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2006