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19942025
most citedThe Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission

4.1k citations · 44.6k across the 350 of their papers we have counts for

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Showing 2009 · astro-ph.COShow all

6 papers · 2 filters

astro-ph.CO2009

Analysis of the Spectral Energy Distributions of Fermi bright blazars

S. Cutini, D. Gasparrini, P. Giommi +2

Blazars are a small fraction of all extragalactic sources but, unlike other objects, they are strong emitters across the entire electromagnetic spectrum. In this study we have cond…

astro-ph.CO2009

Study of microwave/gamma-ray properties for Fermi-LAT bright AGNs

D. Gasparrini, E. Cavazzuti, P. Giommi +3

Blazars are a small fraction of all extragalactic sources but, unlike other objects, they are strong emitters across the entire electromagnetic spectrum. Recent data in the microwa…

astro-ph.CO2009★ 45 cited

Multiwavelength observations of 3C 454.3 II. The AGILE 2007 December campaign

I. Donnarumma, G. Pucella, V. Vittorini +75

We report on the second AGILE multiwavelength campaign of the blazar 3C 454.3 during the first half of December 2007. This campaign involved AGILE, Spitzer, Swift,Suzaku,the WEBT c…

astro-ph.CO2009★ 23 cited

The number counts, luminosity functions and evolution of microwave-selected (WMAP) blazars and radio galaxies

P. Giommi, S. Colafrancesco, P. Padovani +3

(Abridged) We carried out an extensive search to identify the counterparts of all the sources listed in the WMAP 3-yr catalogue using literature and archival data. Our work led to…

astro-ph.CO2009★ 1 cited

The June 2008 flare of Markarian 421 from optical to TeV energies

R. M. Wagner, I. Donnarumma, J. Grube +6

We present optical to very-high energy (VHE) gamma-ray observations of Mrk 421 between 2008 May 24 and June 23. A high-energy (HE) gamma-ray signal was detected by AGILE-GRID durin…

astro-ph.CO2009★ 498 cited

GRB 090423 at a redshift of z~8.1

R. Salvaterra, M. Della Valle, S. Campana +42

Gamma-ray bursts (GRBSs) are produced by rare types of massive stellar explosions. Their rapidly fading afterglows are often bright enough at optical wavelengths, that they are det…