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The cosmic evolution of Fermi BL Lacertae objects / Gasparrini, D ; Ajello, M (UC, Berkeley, Space Sci. Dept.) ; Romani, R W (Stanford U., HEPL ; KIPAC, Menlo Park) ; Shaw, M S (Stanford U., HEPL ; KIPAC, Menlo Park)
2013 - 5 p. - Published in : (2013) , pp. 395-399
In : 9th Rencontres du Vietnam: Windows on the Universe, Quy Nhon, Vietnam, 11 - 17 Aug 2013, pp.395-399

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Measurement of the high-energy gamma-ray emission from the Moon with the Fermi Large Area Telescope / Fermi LAT Collaboration
We have measured the gamma-ray emission spectrum of the Moon using the data collected by the Large Area Telescope onboard the Fermi satellite during its first 7 years of operation, in the energy range from 30 MeV up to a few GeV. We have also studied the time evolution of the flux, finding a correlation with the solar activity. [...]
arXiv:1604.03349.- 2016-04-08 - 16 p. - Published in : Phys. Rev. D 93 (2016) 082001 Fulltext: arXiv:1604.03349 - PDF; 10.1103_PhysRevD.93.082001 - PDF; External link: Preprint

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The redshift and afterglow of the extremely energetic gamma-ray burst GRB 080916C / Greiner, J. (Garching, Max Planck Inst., MPE) ; Clemens, C. (Garching, Max Planck Inst., MPE) ; Kruehler, T. (Garching, Max Planck Inst., MPE ; Munich, Tech. U., Universe) ; Kienlin, A.v. (Garching, Max Planck Inst., MPE) ; Rau, A. ; Sari, R. ; Fox, Derek B. (Penn State U., Astron. Astrophys.) ; Kawai, N. (Tokyo Inst. Tech.) ; Afonso, P. (Garching, Max Planck Inst., MPE) ; Ajello, M. (KIPAC, Menlo Park ; UC, Berkeley ; UC, Berkeley, Space Sci. Dept. ; SLAC) et al.
The detection of GeV photons from gamma-ray bursts (GRBs) has important consequences for the interpretation and modelling of these most-energetic cosmological explosions. The full exploitation of the high-energy measurements relies, however, on the accurate knowledge of the distance to the events. [...]
arXiv:0902.0761.- 2009 - 6 p. - Published in : Astronomy and astrophysics 498 (2009) 89-94 External link: Preprint

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Se också: liknande författarnamn
89	Ajello, M
18	Ajello, Marco

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