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Alberto Manfreda

Researcher at Istituto Nazionale di Fisica Nucleare

Publications -  143
Citations -  8065

Alberto Manfreda is an academic researcher from Istituto Nazionale di Fisica Nucleare. The author has contributed to research in topics: Fermi Gamma-ray Space Telescope & Polarimetry. The author has an hindex of 36, co-authored 84 publications receiving 6579 citations. Previous affiliations of Alberto Manfreda include University of Pisa & Max Planck Society.

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The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV

Markus Ackermann, +143 more
TL;DR: The IGRB spectrum shows a significant high-energy cutoff feature, and can be well described over nearly four decades in energy by a power law with exponential cutoff having a spectral index of $2.32\pm0.02$ and a break energy of $(279\pm52)$ GeV using our baseline diffuse Galactic emission model as mentioned in this paper.
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The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV

Markus Ackermann, +177 more
TL;DR: The first IGRB measurement with the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope (Fermi) used 10 months of sky-survey data and considered an energy range between 200 MeV and 100 GeV.
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FERMI-LAT OBSERVATIONS of HIGH-ENERGY γ-RAY EMISSION TOWARD the GALACTIC CENTER

Marco Ajello, +158 more
TL;DR: The Fermi Large Area Telescope (LAT) has provided the most detailed view to date of the emission toward the Galactic center (GC) in high-energy gamma-rays as mentioned in this paper.
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DEVELOPMENT of the MODEL of GALACTIC INTERSTELLAR EMISSION for STANDARD POINT-SOURCE ANALYSIS of FERMI LARGE AREA TELESCOPE DATA

Fabio Acero, +169 more
TL;DR: In this article, the authors describe the development of the Galactic Interstellar Emission Model (GIEM) which is the standard adopted by the LAT Collaboration and is publicly available, based on a linear combination of maps for interstellar gas column density in Galactocentric annuli and for the inverse-Compton emission produced in the Galaxy.
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The Fermi Galactic Center GeV Excess and Implications for Dark Matter

M. Ackermann, +161 more
TL;DR: In this paper, the uncertainty of the Galactic Center (GC) excess spectrum and morphology due to uncertainties in cosmic-ray source distributions and propagation, uncertainties in the distribution of interstellar gas in the Milky Way, and uncertainties due to a potential contribution from the Fermi bubbles.