The bright optical flash from GRB 060117
arXiv:astro-ph/0606004 · doi:10.1051/0004-6361:20065092
Abstract
We present a discovery and observation of an extraordinarily bright prompt optical emission of the GRB 060117 obtained by a wide-field camera atop the robotic telescope FRAM of the Pierre Auger Observatory from 2 to 10 minutes after the GRB. We found rapid average temporal flux decay of alpha = -1.7 +- 0.1 and a peak brightness R = 10.1 mag. Later observations by other instruments set a strong limit on the optical and radio transient fluxes, unveiling an unexpectedly rapid further decay. We present an interpretation featuring a relatively steep electron-distribution parameter p ~ 3.0 and providing a straightforward solution for the overall fast decay of this optical transient as a transition between reverse and forward shock.
Accepted to A&A, 4 pages, corected few typos pointed out by X.F. Wu
References in corpus (13)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- The Swift X-ray Telescope
- Gamma-Ray Bursts and the Fireball Model
- Observation of contemporaneous optical radiation from a gamma-ray burst
- Predictions for The Very Early Afterglow and The Optical Flash
- Gamma-ray burst early optical afterglows: implications for the initial Lorentz factor and the central engine
- The afterglow of GRB 021004: surfing on density waves
- The Early Light Curve of the Optical Afterglow of GRB 021211
- Swift panchromatic observations of the bright gamma-ray burst GRB050525a
- Energy Injection Episodes in Gamma Ray Bursts: The Light Curves and Polarization Properties of GRB 021004
- The Anomalous Early Afterglow of GRB 050801
- A Reverse-Shock Model for the Early Afterglow of GRB 050525A
- The Early (<1 hr) Multi-Color Afterglow of GRB 050502a: Possible Evidence for a Uniform Medium with Density Clumps
Cited by in corpus (23)
- The Pierre Auger Cosmic Ray Observatory
- The Afterglows of Swift-era Gamma-Ray Bursts. I. Comparing pre-Swift and Swift era Long/Soft (Type II) GRB Optical Afterglows
- Gamma-Ray Bursts in the Swift Era
- The optically unbiased GRB host (TOUGH) survey. I. Survey design and catalogs
- The Remarkable Afterglow of GRB 061007: Implications for Optical Flashes and GRB Fireballs
- Multiwavelength analysis of the intriguing GRB 061126: the reverse shock scenario and magnetization
- Phenomenology of Reverse-Shock Emission in the Optical Afterglows of Gamma Ray Bursts
- Pre-ALMA observations of GRBs in the mm/submm range
- A morphological analysis of gamma-ray burst early optical afterglows
- Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z=3.2 gamma-ray burst
- Searching for differences in Swift's intermediate GRBs
- The Rapid Atmospheric Monitoring System of the Pierre Auger Observatory
- Gamma-ray burst afterglows
- Multi-wavelength observations of afterglow of GRB 080319B and the modeling constraints
- An Estimation of the Gamma-Ray Burst Afterglow Apparent Optical Brightness Distribution Function
- GRB 110715A: The peculiar multiwavelength evolution of the first afterglow detected by ALMA
- A multiwavelength study of Swift GRB 060111B constraining the origin of its prompt optical emission
- Reverse Shock Emission in Gamma-ray Bursts Revisited
- Astronomy with Small Telescopes
- GRB 190919B: Rapid optical rise explained as a flaring activity
- Optical Behavior of GRB 061121 around its X-Ray Shallow Decay Phase
- Early afterglows from radially structured outflows and the application to X-ray shallow decays
- Could bright gamma-ray burst optical transients have been recorded historically?