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Paper detail

The lag-luminosity relation in the gamma-ray burst source-frame

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 observer-frame energy range of the Swift Burst Alert Telescope (BAT). The spectral lags between these energy channels are then presented as a function of the isotropic peak luminosity of the GRBs in the sample.

preprint2010arXivOpen access
T. N. UkwattaK. S. DhugaM. StamatikosT. SakamotoW. C. ParkeS. D. BarthelmyN. Gehrels
astro-ph.HE
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T. N. UkwattaK. S. DhugaM. StamatikosT. SakamotoW. C. ParkeS. D. BarthelmyN. Gehrels

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