Improved Correlation between the Variability and Peak Luminosity of Gamma-Ray Bursts
arXiv:astro-ph/0509776 · doi:10.1111/j.1365-2966.2005.09836.x
Abstract
A new procedure for smoothing a gamma-ray burst (GRB) lightcurve and calculating its variability is presented. Applying the procedure to a sample of 25 long GRBs, we have obtained a very tight correlation between the variability and the peak luminosity. The only significant outlier in the sample is GRB 030329. With this outlier excluded, the data scatter is reduced by a factor of \sim 3 compared to that of Guidorzi et al. (2005), measured by the deviation of fit. Possible causes for the outlier are discussed.
9 pages, including 7 figure. Expanded as requested by referee. An error in Fig. 1 was corrected (the two 1-sigma lines in the old version were wrong). Accepted for publication by MNRAS
References in corpus (15)
- Discovery of the peculiar supernova 1998bw in the error box of GRB980425
- The Physics of Gamma-Ray Bursts
- A very energetic supernova associated with the gamma-ray burst of 29 March 2003
- Intrinsic spectra and energetics of BeppoSAX Gamma-Ray Bursts with known redshifts
- Spectroscopic Discovery of the Supernova 2003dh Associated with GRB 030329
- The collimation--corrected GRB energies correlate with the peak energy of their spectrum
- Connection Between Energy-dependent Lags And Peak Luminosity In Gamma-ray Bursts
- The afterglow, the redshift, and the extreme energetics of the gamma-ray burst 990123
- A Possible Cepheid-Like Luminosity Estimator for the Long Gamma-Ray Bursts
- Spectroscopy of the Host Galaxy of the Gamma--Ray Burst 980703
- Very high column density and small reddening towards GRB 020124 at z = 3.20
- The redshift determination of GRB 990506 and GRB 000418 with the Echellete Spectrograph Imager on Keck
- The GRB Variability/Peak Luminosity Correlation: new results
- Testing the GRB Variability/Peak Luminosity correlation using the pseudo-redshifts of a large sample of BATSE GRBs
- SCUBA sub-millimeter observations of gamma-ray bursters IV. GRB 021004, 021211, 030115, 030226, 041006
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