M. Battelino
Royal Institute of Technology
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Publication
Featured researches published by M. Battelino.
The Astrophysical Journal | 2010
F. Ryde; Magnus Axelsson; Bing Zhang; S. McGlynn; Asaf Pe'er; Christoffer Lundman; S. Larsson; M. Battelino; B. Zhang; E. Bissaldi; J. Bregeon; M. S. Briggs; J. Chiang; F. de Palma; S. Guiriec; Josefin Larsson; F. Longo; S. McBreen; N. Omodei; Vahe Petrosian; Robert D. Preece; A. J. van der Horst
The Fermi Gamma-ray Space Telescope observed the bright and long GRB090902B, lying at a redshift of z = 1.822. Together the Large Area Telescope (LAT) and the Gamma-ray Burst Monitor (GBM) cover th ...
Monthly Notices of the Royal Astronomical Society | 2011
F. Ryde; Asaf Pe’er; T. Nymark; Magnus Axelsson; E. Moretti; Christoffer Lundman; M. Battelino; E. Bissaldi; J. Chiang; M. S. Jackson; S. Larsson; F. Longo; S. McGlynn; N. Omodei
The emission from a gamma-ray burst (GRB) photosphere can give rise to a variety of spectral shapes. The spectrum can retain the shape of a Planck function or it can be broadened and have the shape ...
The Astrophysical Journal | 2009
David L. Band; Magnus Axelsson; L. Baldini; G. Barbiellini; Matthew G. Baring; D. Bastieri; M. Battelino; R. Bellazzini; E. Bissaldi; G. Bogaert; Jerry T. Bonnell; J. Chiang; J. Cohen-Tanugi; V. Connaughton; S. Cutini; F. de Palma; B. L. Dingus; E. Do Couto E Silva; G. Fishman; A. Galli; N. Gehrels; N. Giglietto; Jonathan Granot; S. Guiriec; R. Hughes; T. Kamae; Nu. Komin; F. Kuehn; M. Kuss; F. Longo
The Large Area Telescope (LAT) instrument on the Fermi mission will reveal the rich spectral and temporal gamma-ray burst (GRB) phenomena in the >100 MeV band. The synergy with Fermis Gamma-ray Burst Monitor detectors will link these observations to those in the well explored 10-1000 keV range; the addition of the >100 MeV band observations will resolve theoretical uncertainties about burst emission in both the prompt and afterglow phases. Trigger algorithms will be applied to the LAT data both onboard the spacecraft and on the ground. The sensitivity of these triggers will differ because of the available computing resources onboard and on the ground. Here we present the LATs burst detection methodologies and the instruments GRB capabilities.
