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20022009
most citedMeasurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope

911 citations

51 papers

astro-ph.HE2009

Neutral versus ionized absorber as an explanation of the X-ray dippers

M. Balucinska-Church, M. J. Church, T. Dotani +1

We present results of the Suzaku observation of the dipping, periodically bursting low mass X-ray binary XB 1323-619 in which we concentrate of the spectral evolution in dipping in…

astro-ph.CO200914 cited

X-ray Diagnostics of Thermal Conditions of the Hot Plasmas in the Centaurus Cluster

I. Takahashi, M. Kawaharada, K. Makishima +9

X-ray data of the Centaurus cluster, obtained with {\it XMM-Newton} for 45 ksec, were analyzed. Deprojected EPIC spectra from concentric thin shell regions were reproduced equally…

astro-ph.HE200952 cited

Pulsed Gamma-rays from PSR J2021+3651 with the Fermi Large Area Telescope

A. A. Abdo

We report the detection of pulsed gamma-rays from the young, spin-powered radio pulsar PSR J2021+3651 using data acquired with the Large Area Telescope (LAT) on the Fermi Gamma-ray…

astro-ph.GA200921 cited

The variability of Sagittarius A* at 3 millimeter

Juan Li, Zhi-Qiang Shen, Atsushi Miyazaki +5

We have performed monitoring observations of the 3-mm flux density toward the Galactic Center compact radio source Sgr A* with the Australia Telescope Compact Array since 2005 Octo…

astro-ph.HE200935 cited

Suzaku Wide Band Analysis of the X-ray Variability of TeV Blazar Mrk 421 in 2006

Masayoshi Ushio, Takaaki Tanaka, Grzegorz Madejski +9

We present the results of X-ray observations of the well-studied TeV blazar Mrk 421 with the Suzaku satellite in 2006 April 28. During the observation, Mrk 421 was undergoing a lar…

astro-ph.HE2009911 cited

Measurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope

LAT Collaboration

Designed as a high-sensitivity gamma-ray observatory, the Fermi Large Area Telescope is also an electron detector with a large acceptance exceeding 2m^2 sr at 300 GeV. Building on…