Consistency with synchrotron emission in the bright GRB 160625B observed by Fermi

We present time-resolved spectral analysis of prompt emission from GRB 160625B, one of the brightest bursts ever detected by Fermi in its nine years of operations. Standard empirical functions fail to provide an acceptable fit to the GBM spectral data, which instead require the addition of a low-ene...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2018-05, Vol.613, p.A16
Hauptverfasser:	Ravasio, M. E., Oganesyan, G., Ghirlanda, G., Nava, L., Ghisellini, G., Pescalli, A., Celotti, A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Cooling Emission analysis Empirical analysis Gamma ray bursts gamma-ray burst: general gamma-ray burst: individual: GRB 160625B Magnetic fields Model testing radiation mechanisms: non-thermal Spectra Spectral analysis
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