25 citations · 29 across the 3 of their papers we have counts for
7 papers
Prospects of newly detecting nearby star-forming galaxies by the Cherenkov Telescope Array
Naoya Shimono, Tomonori Totani, Takahiro Sudoh
Prospects of the Cherenkov Telescope Array (CTA) for the study of very high energy gamma-ray emission from nearby star-forming galaxies are investigated. In the previous work, we c…
The Highest Energy HAWC Sources are Likely Leptonic and Powered by Pulsars
Takahiro Sudoh, Tim Linden, Dan Hooper
The HAWC Collaboration has observed gamma rays at energies above 56 TeV from a collection of nine sources. It has been suggested that this emission could be hadronic in nature, req…
Physical Conditions and Particle Acceleration in the Kiloparsec Jet of Centaurus A
Takahiro Sudoh, Dmitry Khangulyan, Yoshiyuki Inoue
The non-thermal emission from the kiloparsec-scale jet of Centaurus A exhibits two notable features, bright diffuse emission and many compact knots, which have been intensively stu…
Multi-wavelength Emission from Galactic Jets: the Case of the Microquasar SS433
Takahiro Sudoh, Yoshiyuki Inoue, Dmitry Khangulyan
SS433 is a Galactic microquasar with powerful jets, where very-high-energy particles are produced. We study particle acceleration in the jets of SS433 in the light of the recent mu…
Pulsars in a Bubble? Following Electron Diffusion in the Galaxy with TeV Gamma Rays
H. Fleischhack, A. Albert, C. Alvarez +32
TeV Halos, extended regions of TeV gamma-ray emission around middle-aged pulsars, have recently been established as a new source class in gamma-ray astronomy. These halos have been…
TeV Halos are Everywhere: Prospects for New Discoveries
Takahiro Sudoh, Tim Linden, John F. Beacom
Milagro and HAWC have detected extended TeV gamma-ray emission around nearby pulsar wind nebulae (PWNe). Building on these discoveries, Linden et al. [1] identified a new source cl…