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19912026
most citedAdvances in Quantum Metrology

3.9k citations

Showing 2011 · astro-ph.HEShow all

18 papers · 2 filters

astro-ph.HE2011★ 20 cited

A time-variable, phase-dependent emission line in the X-ray spectrum of the isolated neutron star RX J0822-4300

A. De Luca, D. Salvetti, A. Sartori +9

RX J0822-4300 is the Central Compact Object associated with the Puppis A supernova remnant. Previous X-ray observations suggested RX J0822-4300 to be a young neutron star with a we…

astro-ph.HE2011

The flaring blazars of the first 1.5 years of the AGILE mission

L. Pacciani, A. Bulgarelli, A. W. Chen +60

We report the AGILE gamma-ray observations and the results of the multiwavelength campaigns on seven flaring blazars detected by the mission: During two multiwavelength campaigns,…

astro-ph.HE2011★ 2 cited

The observation of Gamma Ray Bursts and Terrestrial Gamma-ray Flashes with AGILE

E. Del Monte, G. Barbiellini, F. Fuschino +50

Since its early phases of operation, the AGILE mission is successfully observing Gamma Ray Bursts (GRBs) in the hard X-ray band with the SuperAGILE imager and in the MeV range with…

astro-ph.HE2011★ 37 cited

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…

astro-ph.HE2011★ 229 cited

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.HE2011★ 20 cited

The AGILE observations of the hard and bright GRB 100724B

E. Del Monte, G. Barbiellini, I. Donnarumma +49

The observation of Gamma Ray Bursts (GRBs) in the gamma-ray band has been advanced by the AGILE and Fermi satellites after the era of the Compton Gamma-Ray Observatory. AGILE and F…

astro-ph.HE2011★ 18 cited

The Identification of the X-ray Counterpart to PSR J2021+4026

Martin C. Weisskopf, Roger W. Romani, Massimiliano Razzano +16

We report the probable identification of the X-ray counterpart to the gamma-ray pulsar PSR J2021+4026 using imaging with the Chandra X-ray Observatory ACIS and timing analysis with…

astro-ph.HE2011★ 16 cited

VLT observations of the two Fermi pulsars PSR J1357-6429 and PSR J1048-5832

R. P. Mignani, A. Shearer, A. De Luca +3

Optical observations of pulsars are crucial to study the neutron star properties, from the structure and composition of the interior, to the properties and geometry of the magnetos…

astro-ph.HE2011★ 80 cited

Observation of the Cosmic Ray Moon shadowing effect with ARGO-YBJ

YBJ Collaboration

Cosmic rays are hampered by the Moon and a deficit in its direction is expected (the so-called \emph{Moon shadow}). The Moon shadow is an important tool to determine the performanc…

astro-ph.HE2011★ 91 cited

The brightest gamma-ray flaring blazar in the sky: AGILE and multi-wavelength observations of 3C 454.3 during November 2010

S. Vercellone, E. Striani, V. Vittorini +84

Since 2005, the blazar 3C 454.3 has shown remarkable flaring activity at all frequencies, and during the last four years it has exhibited more than one gamma-ray flare per year, be…

astro-ph.HE2011★ 30 cited

The remarkable gamma-ray activity in the gravitationally lensed blazar PKS 1830-211

I. Donnarumma, A. De Rosa, V. Vittorini +34

We report the extraordinary gamma-ray activity (E>100 MeV) of the gravitationally lensed blazar PKS 1830-211 (z=2.507) detected by AGILE between October and November 2010. The sour…

astro-ph.HE2011★ 75 cited

Long-term monitoring of the TeV emission from Mrk 421 with the ARGO-YBJ experiment

YBJ Collaboration, B. Bartoli, P. Bernardini +105

ARGO-YBJ is an air shower detector array with a fully covered layer of resistive plate chambers. It is operated with a high duty cycle and a large field of view. It continuously mo…

astro-ph.HE2011★ 67 cited

The Crab Nebula super-flare in April 2011: extremely fast particle acceleration and gamma-ray emission

E. Striani, M. Tavani, G. Piano +47

We report on the extremely intense and fast gamma-ray are above 100 MeV detected by AGILE from the Crab Nebula in mid-April 2011. This event is the fourth of a sequence of reported…

astro-ph.HE2011★ 18 cited

Spectral Evolution of the September 2010 gamma-ray flare from the Crab Nebula (V2)

V. Vittorini, M. Tavani, G. Pucella +1

Strong gamma-ray flares from the Crab Nebula have been recently discovered by AGILE and confirmed by Fermi-LAT. We study here the spectral evolution in the gamma-ray energy range a…

astro-ph.HE2011★ 79 cited

AGILE detection of extreme gamma-ray activity from the blazar PKS 1510-089 during March 2009. Multifrequency analysis

F. D'Ammando, C. M. Raiteri, M. Villata +112

We report on the extreme gamma-ray activity from the FSRQ PKS 1510-089 observed by AGILE in March 2009. In the same period a radio-to-optical monitoring of the source was provided…

astro-ph.HE2011★ 39 cited

Discovery of a faint X-ray counterpart and of a parsec-long X-ray tail for the middle-aged, gamma-ray only pulsar PSR J0357+3205

A. De Luca, M. Marelli, R. P. Mignani +7

The Large Area Telescope (LAT) onboard the Fermi satellite opened a new era for pulsar astronomy, detecting gamma-ray pulsations from more than 60 pulsars, ~40% of which are not se…

astro-ph.HE2011★ 8 cited

X-ray and optical observations of the closest isolated radio pulsar

A. Tiengo, R. P. Mignani, A. De Luca +3

With a parallactic distance of 170 pc, PSR J2144-3933 is the closest isolated radio pulsar currently known. It is also the slowest (P = 8.51 s) and least energetic (Edot = 2.6E28 e…

astro-ph.HE2011★ 352 cited

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…