activity
20042026
most citedFermi Large Area Telescope Fourth Source Catalog

1.4k citations · 24.1k across the 269 of their papers we have counts for

collaborators
Showing 2010Show all

15 papers · 1 filter

astro-ph.CO2010

Flux variability in the FSRQ 1510-089. A radio-gamma perspective

M. Orienti, G. Giovannini, D. Dallacasa +5

The knowledge of the physical conditions occurring in the relativistic jet of radio-loud active galactic nuclei (AGNs) is important to understand the mechanisms at the basis of the…

astro-ph.HE2010★ 364 cited

Gamma-ray flares from the Crab Nebula

LAT Collaboration

A young and energetic pulsar powers the well-known Crab Nebula. Here we describe two separate gamma-ray (photon energy >100 MeV) flares from this source detected by the Large Area…

astro-ph.HE2010★ 82 cited

The first gamma-ray outburst of a Narrow-Line Seyfert 1 Galaxy: the case of PMN J0948+0022 in July 2010

L. Foschini, G. Ghisellini, Y. Y. Kovalev +24

We report on a multiwavelength campaign on the radio-loud Narrow-Line Seyfert 1 (NLS1) Galaxy PMN J0948+0022 (z=0.5846) performed in 2010 July-September and triggered by a high-ene…

physics.ao-ph2010★ 45 cited

Gamma-Ray Localization of Terrestrial Gamma-Ray Flashes

M. Marisaldi, A. Argan, A. Trois +59

Terrestrial Gamma-Ray Flashes (TGFs) are very short bursts of high energy photons and electrons originating in Earth's atmosphere. We present here a localization study of TGFs carr…

astro-ph.HE2010★ 18 cited

Study of the gamma-ray source 1AGL J2022+4032 in the Cygnus Region

A. W. Chen, G. Piano, M. Tavani +58

Identification of gamma-ray-emitting Galactic sources is a long-standing problem in astrophysics. One such source, 1AGL J2022+4032, coincident with the interior of the radio shell…

astro-ph.HE2010★ 22 cited

Agile Observations of the "Soft" Gamma-Ray Pulsar PSR B1509-58

M. Pilia, A. Pellizzoni, A. Trois +60

We present the results of new Agile observations of PSR B1509-58 performed over a period of 2.5 years following the detection obtained with a subset of the present data. The modula…