Testing the E_p,i - L_p,iso - T_0.45 correlation on a BeppoSAX and Swift sample of gamma-ray bursts
F. Rossi (1), C. Guidorzi (2,3), L. Amati (4), F. Frontera (1,4), P., Romano (2,3), S. Campana (3), G. Chincarini (2,3), E. Montanari (1), A., Moretti (3), G. Tagliaferri (3) ((1) Universita' di Ferrara (2) Universita', di Milano Bicocca (3) INAF-OAB (4) INAF-IASF Bologna, Italy)

TL;DR
This study tests the Firmani correlation among gamma-ray bursts using a combined sample from BeppoSAX and Swift, confirming its existence but finding it similar in scatter and slope to the well-known Amati correlation.
Contribution
It provides an updated analysis of the E_p,i-L_p,iso-T_0.45 correlation, showing it is not significantly different from the E_p,i-E_iso correlation in terms of scatter and slope.
Findings
Confirmed the existence of the correlation with a similar scatter to the Amati correlation.
Found the slope of the product L_p,iso T_0.45 to be approximately 0.5.
No evidence that the correlation differs significantly from the E_p,i-E_iso correlation.
Abstract
Using a sample of 14 BeppoSAX and 74 Swift GRBs with measured redshift we tested the correlation between the intrinsic peak energy of the time-integrated spectrum, E_p,i, the isotropic-equivalent peak luminosity, L_p,iso, and the duration of the most intense parts of the GRB computed as T_0.45 ("Firmani correlation"). For 41 out of 88 GRBs we could estimate all of the three required properties. Apart from 980425, which appears to be a definite outlier and notoriously peculiar in many respects, we used 40 GRBs to fit the correlation with the maximum likelihood method discussed by D'Agostini, suitable to account for the extrinsic scatter in addition to the intrinsic uncertainties affecting every single GRB. We confirm the correlation. However, unlike the results by Firmani et al., we found that the correlation does have a logarithmic scatter comparable with that of the E_p,i-E_iso…
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