papers

Publications (12)

astro-ph.HE2011

Discovery of Powerful Gamma-Ray Flares from the Crab Nebula

M. Tavani, A. Bulgarelli, V. Vittorini +65

The well known Crab Nebula is at the center of the SN1054 supernova remnant. It consists of a rotationally-powered pulsar interacting with a surrounding nebula through a relativist…

astro-ph.HE2009

Discovery of extreme particle acceleration in the microquasar Cygnus X-3

M. Tavani, A. Bulgarelli, G. Piano +67

The study of relativistic particle acceleration is a major topic of high-energy astrophysics. It is well known that massive black holes in active galaxies can release a substantial…

astro-ph.IM2012

Evaluating the Maximum Likelihood Method for Detecting Short-Term Variability of AGILE gamma-ray Sources

A. Bulgarelli, A. W. Chen, M. Tavani +3

The AGILE space mission (whose instrument is sensitive in the energy ranges 18-60 keV, and 30 MeV - 50 GeV) has been operating since 2007. Assessing the statistical significance of…

astro-ph.HE2009

Agile Detection of Delayed Gamma-Ray Emission from the Short Gamma-Ray Burst GRB 090510

A. Giuliani, F. Fuschino, G. Vianello +59

Short gamma-ray bursts (GRBs), typically lasting less than 2 s, are a special class of GRBs of great interest. We report the detection by the AGILE satellite of the short GRB 09051…

astro-ph.HE2013

An updated list of AGILE bright gamma-ray sources and their variability in pointing mode

F. Verrecchia, C. Pittori, A. W. Chen +76

We present a variability study of a sample of bright gamma-ray (30 MeV -- 50 GeV) sources. This sample is an extension of the first AGILE catalogue of gamma-ray sources (1AGL), obt…

astro-ph.HE2011

Neutral pion emission from accelerated protons in the supernova remnant W44

A. Giuliani, M. Cardillo, M. Tavani +41

We present the AGILE gamma-ray observations in the energy range 50 MeV - 10 GeV of the supernova remnant (SNR) W44, one of the most interesting systems for studying cosmic-ray prod…

astro-ph.HE2010

Direct Evidence for Hadronic Cosmic-Ray Acceleration in the Supernova Renmant IC 443

M. Tavani, A. Giuliani, A. W. Chen +59

The Supernova Remnant (SNR) IC 443 is an intermediate-age remnant well known for its radio, optical, X-ray and gamma-ray energy emissions. In this Letter we study the gamma-ray emi…

astro-ph.CO2009

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.IM2013

Calibration of AGILE-GRID with In-Flight Data and Monte Carlo Simulations

Andrew W. Chen, A. Argan, A. Bulgarelli +57

Context: AGILE is a gamma-ray astrophysics mission which has been in orbit since 23 April 2007 and continues to operate reliably. The gamma-ray detector, AGILE-GRID, has observed G…

astro-ph.HE2009

First AGILE Catalog of High Confidence Gamma-Ray Sources

C. Pittori, F. Verrecchia, A. W. Chen +80

We present the first catalog of high-confidence gamma-ray sources detected by the AGILE satellite during observations performed from July 9, 2007 to June 30, 2008. Catalogued sourc…

astro-ph.HE2010

Detection of Gamma-Ray Emission from the Vela Pulsar Wind Nebula with AGILE

A. Pellizzoni, A. Trois, M. Tavani +68

Pulsars are known to power winds of relativistic particles that can produce bright nebulae by interacting with the surrounding medium. These pulsar wind nebulae (PWNe) are observed…

astro-ph.HE2011

AGILE detection of Cygnus X-3 γ-ray active states during the period mid-2009/mid-2010

A. Bulgarelli, M. Tavani, A. W. Chen +70

Cygnus X-3 (Cyg X-3) is a well-known microquasar producing variable emission at all wavelengths. Cyg X-3 is a prominent X-ray binary producing relativistic jets, and studying its h…