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A. Cesarini

Researcher at University of Urbino

Publications -  172
Citations -  9714

A. Cesarini is an academic researcher from University of Urbino. The author has contributed to research in topics: Blazar & Crab Nebula. The author has an hindex of 56, co-authored 166 publications receiving 8735 citations. Previous affiliations of A. Cesarini include Harvard University & University of Trento.

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Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results

Michele Armano, +118 more
TL;DR: The first results of the LISA Pathfinder in-flight experiment demonstrate that two free-falling reference test masses, such as those needed for a space-based gravitational wave observatory like LISA, can be put in free fall with a relative acceleration noise with a square root of the power spectral density.
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Fermi Large Area Telescope Observations of Markarian 421: The Missing Piece of its Spectral Energy Distribution

A. A. Abdo, +421 more
TL;DR: In this paper, the gamma-ray activity of the high-synchrotron-peaked BL Lacertae object Markarian 421 (Mrk 421) during the first 1.5 years of Fermi operation was reported.
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A connection between star formation activity and cosmic rays in the starburst galaxy M82

V. A. Acciari, +93 more
- 10 Dec 2009 - 
TL;DR: A cosmic-ray density of 250 eV cm-3 in the starburst core, which is about 500 times the average Galactic density is determined, and suggests that supernovae and massive-star winds are the dominant accelerators.
Journal ArticleDOI

Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μHz.

Michele Armano, +78 more
TL;DR: This performance provides an experimental benchmark demonstrating the ability to realize the low-frequency science potential of the LISA mission, recently selected by the European Space Agency.
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Radio Imaging of the Very-High-Energy gamma-Ray Emission Region in the Central Engine of a Radio Galaxy

V. A. Acciari, +385 more
- 24 Jul 2009 - 
TL;DR: Radio and VHE observations of the radio galaxy Messier 87 are revealed, revealing a period of extremely strong VHE gamma-ray flares accompanied by a strong increase of theRadio flux from its nucleus, implying that charged particles are accelerated to very high energies in the immediate vicinity of the black hole.