activity
20122021
most citedThe Cosmic Ray Energy Spectrum Observed with the Surface Detector of the Telescope Array Experiment

264 citations · 910 across the 17 of their papers we have counts for

collaborators
Showing 2013Show all

5 papers · 1 filter

astro-ph.HE2013★ 19 cited

Dense Gas Towards the RXJ1713.7-3946 Supernova Remnant

Nigel I. Maxted, Gavin P. Rowell, Bruce R. Dawson +9

We present results from a Mopra 7mm-wavelength survey that targeted the dense gas-tracing CS(1-0) transition towards the young gamma-ray-bright supernova remnant, RXJ1713.7-3946 (S…

astro-ph.HE2013★ 19 cited

Interstellar gas towards CTB 37A and the TeV gamma-ray source HESS J1714-385

Nigel I. Maxted, Gavin P. Rowell, Bruce R. Dawson +8

Observations of dense molecular gas towards the supernova remnants CTB 37A (G348.5+0.1) and G348.5-0.0 were carried out using the Mopra and Nanten2 radio telescopes. We present CO(…

astro-ph.HE2013★ 50 cited

Search for correlations of the arrival directions of ultra-high energy cosmic ray with extragalactic objects as observed by the telescope array experiment

T. Abu-Zayyad, R. Aida, M. Allen +141

We search for correlations between positions of extragalactic objects and arrival directions of Ultra-High Energy Cosmic Rays (UHECRs) with primary energy EeV as observe…

astro-ph.GA2013★ 164 cited

Molecular Clouds Toward the Super Star Cluster NGC3603; Possible Evidence for a Cloud-Cloud Collision in Triggering the Cluster Formation

Yasuo Fukui, Akio Ohama, Naoki Hanaoka +17

We present new large field observations of molecular clouds with NANTEN2 toward the super star cluster NGC3603 in the transitions 12CO(J=2-1, J=1-0) and 13CO(J=2-1, J=1-0). We sugg…

astro-ph.GA2013★ 55 cited

Non-thermal X-rays and interstellar gas toward the γ-ray supernova remnant RX J1713.7-3946: Evidence for X-ray enhancement around CO and HI clumps

H. Sano, T. Tanaka, K. Torii +18

RX J1713.7-3946 is the most remarkable very-high-energy γ-ray supernova remnant which emits synchrotron X-rays without thermal features. We made a comparative study of CO, HI and X…