Figure 4 from GRB 090510: A GENUINE SHORT GRB FROM A BINARY NEUTRON STAR COALESCING INTO A KERR

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GRB 090510: A GENUINE SHORT GRB FROM A BINARY NEUTRON STAR COALESCING INTO A KERR–NEWMAN BLACK HOLE

Authors: R. Ruffini, M. Muccino, Y. Aimuratov, C. L. Bianco, C. Cherubini, M. Enderli, M. Kovacevic, R. Moradi, A. V. Penacchioni, G. B. Pisani, J. A. Rueda, and Y. Wang

2016 The Astrophysical Journal 831 178.

Provider: AAS Journals

Caption: Figure 4.

Top panel: GBM NaI-n6 light curve of GRB 090510 and interval considered to compute ﹩{E}_{\mathrm{iso}}﹩. Bottom panel: Comptonized+power-law best fit of the corresponding spectrum (from ﹩{T}_{0}+0.528﹩ to ﹩{T}_{0}+1.024﹩ s).

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