902 citations · 6.4k across the 108 of their papers we have counts for
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Global structure of isothermal X-ray emission along the Fermi bubbles
J. Kataoka, M. Tahara, T. Totani +4
In our previous works (Kataoka et al. 2013, Tahara et al. 2015), we found absorbed thermal X-ray plasma with kT ~ 0.3 keV observed ubiquitously near the edges of the Fermi bubbles…
Prospect for Future MeV Gamma-ray Active Galactic Nuclei Population Studies
Yoshiyuki Inoue, Yasuyuki T. Tanaka, Hirokazu Odaka +5
While the X-ray, GeV gamma-ray, and TeV gamma-ray skies have been extensively studied, the MeV gamma-ray sky is not well investigated after the Imaging Compton Telescope (COMPTEL)…
Fermi-LAT and Multi-wavelength Monitoring of the Broad Line Radio Galaxy 3C 120
Y. T. Tanaka, A. Doi, Y. Inoue +7
We present six-year multi-wavelength monitoring result for broad-line radio galaxy 3C 120. The source was sporadically detected by Fermi-LAT and after the MeV/GeV gamma-ray detecti…
Suzaku X-ray Observations of the Fermi Bubbles: Northernmost Cap and Southeast Claw Discovered with MAXI-SSC
M. Tahara, J. Kataoka, Y. Takeuchi +8
We report on Suzaku observations of large-scale X-ray structures possibly related with the Fermi Bubbles obtained in 2013 with a total duration of ~ 80 ks. The observed regions wer…
Metal Enrichment in the Fermi Bubbles as a Probe of Their Origin
Yoshiyuki Inoue, Shinya Nakashima, Masaya Tahara +4
The Fermi bubbles are gigantic gamma-ray structures in our Galaxy. The physical origin of the bubbles is still under debate. The leading scenarios can be divided into two categorie…
The Origin of the Extragalactic Gamma-Ray Background and Implications for Dark-Matter Annihilation
M. Ajello, D. Gasparrini, M. Sanchez-Conde +12
The origin of the extragalactic -ray background (EGB) has been debated for some time. { The EGB comprises the -ray emission from resolved and unresolved extragalactic sources…
Six Years of Fermi-LAT and Multi-wavelength Monitoring of the Broad-Line Radio Galaxy 3C 120: Jet Dissipation at Sub-parsec Scales from the Central Engine
Y. T. Tanaka, A. Doi, Y. Inoue +7
We present multi-wavelength monitoring results for the broad-line radio galaxy 3C 120 in the MeV/GeV, sub-millimeter, and 43 GHz bands over six years. Over the past two years, Ferm…