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20022009
most citedBright AGN Source List from the First Three Months of the Fermi Large Area Telescope All-Sky Survey

431 citations · 1.2k across the 11 of their papers we have counts for

collaborators

22 papers

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.HE2009431 cited

Bright AGN Source List from the First Three Months of the Fermi Large Area Telescope All-Sky Survey

A. A. Abdo

The first three months of sky-survey operation with the Fermi Gamma Ray Space Telescope (Fermi) Large Area Telescope (LAT) reveals 132 bright sources at |b|>10 deg with test statis…

astro-ph2008108 cited

High energy resolution hard X-ray and gamma-ray imagers using CdTe diode devices

Shin Watanabe, Shin-nosuke Ishikawa, Hiroyuki Aono +8

We developed CdTe double-sided strip detectors (DSDs or cross strip detectors) and evaluated their spectral and imaging performance for hard X-rays and gamma-rays. Though the doubl…

astro-ph200822 cited

The NeXT Mission

T. Takahashi, R. Kelley, K. Mitsuda +28

The NeXT (New exploration X-ray Telescope), the new Japanese X-ray Astronomy Satellite following Suzaku, is an international X-ray mission which is currently planed for launch in 2…

astro-ph2008160 cited

Study of Nonthermal Emission from SNR RX J1713.7-3946 with Suzaku

Takaaki Tanaka, Yasunobu Uchiyama, Felix A. Aharonian +11

We present results obtained from a series of observations of the supernova remnant RX J1713.7-3946 by the Suzaku satellite. The observations cover about two-thirds of the remnant s…

astro-ph200742 cited

PoGOLite - A High Sensitivity Balloon-Borne Soft Gamma-ray Polarimeter

Tuneyoshi Kamae, Viktor Andersson, Makoto Arimoto +36

We describe a new balloon-borne instrument (PoGOLite) capable of detecting 10% polarisation from 200mCrab point-like sources between 25 and 80keV in one 6 hour flight. Polarisation…