Rest frame light curves of Swift GRBs

V. Mangano; V. La Parola; E. Troja; G. Cusumano; T. Mineo; D. Burrows; S. Campana; M. Capalbi; G. Chincarini; N. Gehrels; P. Giommi; A. Moretti; M. Perri; P. Romano; ;

doi:10.1393/ncb/i2007-10246-5

arXiv · astro-ph/0701812

Rest frame light curves of Swift GRBs

V. Mangano·V. La Parola·E. Troja·G. Cusumano·T. Mineo·D. Burrows·S. Campana·M. Capalbi·G. Chincarini·N. Gehrels·P. Giommi·A. Moretti·M. Perri·P. Romano·;

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Abstract

We have computed the luminosity rest frame light curves of the first 40 Gamma-ray bursts (GRBs) detected by Swift with well established redshift. We studied average properties of the light curves in the four subsamples of bursts given by z<1, 1 =4. We conclude that all the last three subsamples share the same morphology and the same luminosity range. Very high redshift (z>=4) GRBs detected up to now are not intrinsically longer than lower redshift long GRBs. Nearby long GRBs (z<1) are fainter than average. Possible selection effect are under investigation.

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V. Mangano, V. La Parola, E. Troja, G. Cusumano, T. Mineo, D. Burrows, S. Campana, M. Capalbi, G. Chincarini, N. Gehrels, P. Giommi, A. Moretti, M. Perri, P. Romano, ;. 2007-02-13. Rest frame light curves of Swift GRBs. https://doi.org/10.1393/ncb%2Fi2007-10246-5

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