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Matteo Negro

Researcher at University of Turin

Publications -  119
Citations -  4035

Matteo Negro is an academic researcher from University of Turin. The author has contributed to research in topics: High harmonic generation & Attosecond. The author has an hindex of 29, co-authored 114 publications receiving 3473 citations. Previous affiliations of Matteo Negro include Polytechnic University of Milan & Istituto Nazionale di Fisica Nucleare.

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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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Generalized molecular orbital tomography

TL;DR: In this article, a technique that can be applied to more complicated molecules is presented, which can be used to map electron orbitals and provide information about the inner workings of the molecules.
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Localization and broadband follow-up of the gravitational-wave transient GW150914

B. P. Abbott, +1622 more
TL;DR: In this article, the sky localization of the first observed compact binary merger is presented, where the authors describe the low-latency analysis of the LIGO data and present a sky localization map.
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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.