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Related papers: Explaining the Gamma Ray Burst Lag/Luminosity and …

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This paper presents an interpretation based on gamma-ray burst source kinematics for the relationship found by Norris et al. between peak luminosity and energy-dependent pulse lag. I argue that the correlation should instead be between…

Astrophysics · Physics 2009-10-31 Jay D. Salmonson

We suggest a connection between the pulse paradigm at gamma-ray energies and the recently demonstrated luminosity distribution in gamma-ray bursts: the spectral evolution timescale of pulse structures is anticorrelated with peak luminosity,…

Astrophysics · Physics 2009-10-31 J. P. Norris , G. F. Marani , J. T. Bonnell

Two different luminosity indicators have recently been proposed for Gamma Ray Bursts that use gamma-ray observations alone. They relate the burst luminosity (L) with the time lag between peaks in hard and soft energies, and the spikiness or…

Astrophysics · Physics 2009-11-06 Bradley E. Schaefer , Ming Deng , David L. Band

We derive a new peak lag vs. peak luminosity relation in gamma-ray burst (GRB) pulses. We demonstrate conclusively that GRB spectral lags are pulse rather than burst properties and show how the lag vs. luminosity relation determined from…

Astrophysics · Physics 2009-11-13 Jon Hakkila , Timothy W. Giblin , Jay P. Norris , P. Chris Fragile , Jerry T. Bonnell

The lag-luminosity relation (LLR) provides a way of estimating GRB luminosity by measuring the spectral lags between different energy bands. We want to understand the origin of the LLR and test its validity. This appears especially…

Astrophysics · Physics 2009-11-13 Mimoza Hafizi , Robert Mochkovitch

Spectral lag, the time difference between the arrival of high-energy and low-energy photons, is a common feature in Gamma-ray Bursts (GRBs). Norris et al. 2000 reported a correlation between the spectral lag and the isotropic peak…

High Energy Astrophysical Phenomena · Physics 2015-05-13 T. N. Ukwatta , M. Stamatikos , K. S. Dhuga , T. Sakamoto , S. D. Barthelmy , A. Eskandarian , N. Gehrels , L. C. Maximon , J. P. Norris , W. C. Parke

Spectral lag, which is defined as the difference in time of arrival of high and low energy photons, is a common feature in Gamma-ray Bursts (GRBs). Previous investigations have shown a correlation between this lag and the isotropic peak…

We have investigated the empirical lag-luminosity relation in the Gamma-ray Burst (GRB) source-frame. We selected two energy bands (100-200 keV and 300-400 keV) in the GRB source-frame, which after redshift correction, lie in the…

High Energy Astrophysical Phenomena · Physics 2010-03-02 T. N. Ukwatta , K. S. Dhuga , M. Stamatikos , T. Sakamoto , W. C. Parke , S. D. Barthelmy , N. Gehrels

A correlation is presented between the pulse lag and the jet-break time for seven BATSE gamma-ray bursts with known redshifts. This is, to our best knowledge, the first known direct tight correlation between a property of the gamma-ray…

Astrophysics · Physics 2009-11-07 Jay D. Salmonson , Titus J. Galama

We analyze the spectral lags of a sample of bright gamma-ray burst pulses observed by CGRO BATSE and compare these with the results of high-resolution spectroscopical investigations. We find that pulses with hard spectra have the largest…

Astrophysics · Physics 2009-11-10 Felix Ryde , Dan Kocevski , Zsolt Bagoly , Nils Ryde , Attila Meszaros

We report test results of the correlation between time variability and peak luminosity of Gamma-Ray Bursts (GRBs), using a larger sample (32) of GRBs with known redshift than that available to Reichart et al. (2001), and using as…

Astrophysics · Physics 2007-08-29 C. Guidorzi , F. Frontera , E. Montanari , F. Rossi , L. Amati , A. Gomboc , K. Hurley , C. G. Mundell

We compared redshifts $z_Y$ from Yonetoku relation and $z_{lag}$ from the lag-luminosity relation for 565 BASTE GRBs and were surprised to find that the correlation is very low. Assuming that the luminosity is a function of both $z_Y$ and…

Relations linking the temporal or/and spectral properties of the prompt emission of gamma-ray bursts (hereafter GRBs) to the absolute luminosity are of great importance as they both constrain the radiation mechanisms and represent potential…

High Energy Astrophysical Phenomena · Physics 2015-05-30 S. Boci , M. Hafizi , R. Mochkovitch

The observed delay in the arrival times between high and low energy photons in gamma-ray bursts (GRBs) has been shown by Norris et al. to be correlated to the absolute luminosity of a GRB. Despite the apparent importance of this spectral…

Astrophysics · Physics 2009-11-07 D. Kocevski , E. P. Liang

We investigated the rest frame spectral lags of two complete samples of bright long (50) and short (6) gamma-ray bursts (GRB) detected by Swift. We analysed the Swift/BAT data through a discrete cross-correlation function (CCF) fitted with…

Using the lag-luminosity relation and various BATSE catalogs we create a large catalog of burst redshifts, peak luminosities and emitted energies. These catalogs permit us to evaluate the lag-luminosity relation, and to study the burst…

Astrophysics · Physics 2009-11-10 D. L. Band , J. P. Norris , J. T. Bonnell

We compute the kinematical dependence of the peak luminosity, the pulse width and the spectral lag of the peak luminosity on the viewing angle $\theta_v$ of a jet. For appropriate model parameters we obtain the peak luminosity-spectral lag…

Astrophysics · Physics 2009-11-06 Kunihito Ioka , Takashi Nakamura

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…

Astrophysics · Physics 2009-11-13 Li-Xin Li , Bohdan Paczynski

In strict analogy to prompt pulses, X-ray flares observed by Swift-XRT in long Gamma-Ray Bursts define a lag-luminosity relation: L_p,iso \propto t_lag^{-0.95+/-0.23}. The lag-luminosity is proven to be a fundamental law extending 5 decades…

High Energy Astrophysical Phenomena · Physics 2015-05-19 R. Margutti

We have analyzed the 241 bursts for which peak counts $\C$ exist in the publicly available Burst and Transient Source Experiment (BATSE) catalog. Introducing peak counts in 1024 ms as a measure of burst brightness $\B$ and the ratio of peak…

Astrophysics · Physics 2009-10-22 D. Q. Lamb , C. Graziani , I. A. Smith
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