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S. Maldera

Researcher at Istituto Nazionale di Fisica Nucleare

Publications -  40
Citations -  3689

S. Maldera is an academic researcher from Istituto Nazionale di Fisica Nucleare. The author has contributed to research in topics: Fermi Gamma-ray Space Telescope & Population. The author has an hindex of 23, co-authored 40 publications receiving 3058 citations.

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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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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.
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3FHL: The Third Catalog of Hard Fermi-LAT Sources

Marco Ajello, +168 more
TL;DR: The Third catalog of Hard Fermi-LAT Sources (3FHL) as mentioned in this paper contains 1556 objects characterized in the 10 GeV-2 TeV energy range.
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MINUTE-TIMESCALE >100 MeV γ-RAY VARIABILITY during the GIANT OUTBURST of QUASAR 3C 279 OBSERVED by FERMI-LAT in 2015 June

Markus Ackermann, +131 more
TL;DR: In this article, the authors observed minute-scale variability suggests a very compact emission region at hundreds of Schwarzschild radii from the central engine in conical jet models, where a minimum bulk jet Lorentz factor of 35 is necessary to avoid both internal gamma-ray absorption and super-Eddington jet power.
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The 1st Fermi Lat Supernova Remnant Catalog

Fabio Acero, +156 more
TL;DR: In this paper, the properties of supernova remnants (SNRs) at high energies were uniformly determined using data from the Fermi Large Area Telescope (LAT) using a systematic survey at energies from 1 to 100 GeV.