Observations of the Prompt Gamma-Ray Emission of GRB 070125
arXiv:0710.4590 · doi:10.1086/592136
Abstract
The long, bright gamma-ray burst GRB 070125 was localized by the Interplanetary Network. We present light curves of the prompt gamma-ray emission as observed by Konus-WIND, RHESSI, Suzaku-WAM, and \textit{Swift}-BAT. We detail the results of joint spectral fits with Konus and RHESSI data. The burst shows moderate hard-to-soft evolution in its multi-peaked emission over a period of about one minute. The total burst fluence as observed by Konus is erg/cm (20 keV--10 MeV). Using the spectroscopic redshift , we find that the burst is consistent with the ``Amati'' correlation. Assuming a jet opening angle derived from broadband modeling of the burst afterglow, GRB 070125 is a significant outlier to the ``Ghirlanda'' correlation. Its collimation-corrected energy release ergs is the largest yet observed.
arXiv comment25 pages, 6 figures; accepted for publication in ApJ. Improved spectral fits and energetics estimates
References in corpus (18)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Cosmological Constraints from the SDSS Luminous Red Galaxies
- Intrinsic spectra and energetics of BeppoSAX Gamma-Ray Bursts with known redshifts
- Jets in GRBs
- Discovery of the X-Ray Afterglow of the Gamma-Ray Burst of February 28 1997
- The collimation--corrected GRB energies correlate with the peak energy of their spectrum
- The Ep,i - Eiso correlation in GRBs: updated observational status, re-analysis and main implications
- The Complete Spectral Catalog of Bright BATSE Gamma-Ray Bursts
- Gamma-Ray Bursts in the Swift Era
- A Complete Catalog of Swift GRB Spectra and Durations: Demise of a Physical Origin for Pre-Swift High-Energy Correlations
- The Epeak-Eiso plane of long Gamma Ray Bursts and selection effects
- Confirming the gamma-ray burst spectral-energy correlations in the era of multiple time breaks
- A comprehensive study of GRB 070125, a most energetic gamma ray burst
- On the Possibility of Identification of a Short/Hard Burst GRB 051103 with the Giant Flare from a Soft Gamma Repeater in the M81 Group of Galaxies
- An Energetic Afterglow From A Distant Stellar Explosion
- GRB Energetics in the Swift Era
- The Rapidly Flaring Afterglow of the Very Bright and Energetic GRB 070125
- RHESSI Spectral Fits of Swift GRBs
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- The Afterglows of Swift-era Gamma-Ray Bursts. I. Comparing pre-Swift and Swift era Long/Soft (Type II) GRB Optical Afterglows
- Jet breaks and Energetics of Swift GRB X-ray Afterglows
- A Universal Scaling for the Energetics of Relativistic Jets From Black Hole Systems
- A Comparison of the Afterglows of Short- and Long-Duration Gamma-Ray Bursts
- The Collimation and Energetics of the Brightest Swift Gamma-Ray Bursts
- A Comprehensive Study of Gamma-Ray Burst Optical Emission: I. Flares and Early Shallow Decay Component
- Estimating Long GRB Jet Opening Angles and Rest-Frame Energetics
- The Possible Impact of GRB Detector Thresholds on Cosmological Standard Candles
- A Correlated Study of Optical and X-ray Afterglows of GRBs
- Statistical study of gamma-ray bursts with jet break feature in multi-wavelength afterglow emissions
- The Rapidly Flaring Afterglow of the Very Bright and Energetic GRB 070125
- On the Connection of Gamma-Ray Bursts and X-Ray Flashes in the BATSE and RHESSI Databases
- 'Jet breaks' and 'missing breaks' in the X-Ray afterglow of Gamma Ray Bursts
- GRB 070125 and the environments of spectral-line poor afterglow absorbers
- Testing Blandford-Znajek mechanism in black hole hyperaccretion flows for long-duration gamma-ray bursts
- Detectability of Planck-Scale-Induced Blurring with Gamma-Ray Bursts