activity
19972023
most citedDetection of Gamma Rays of Up to 50 TeV From the Crab Nebula

115 citations · 281 across the 13 of their papers we have counts for

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10 papers · 1 filter

astro-ph2006★ 19 cited

Mrk 421, Mrk 501, and 1ES 1426+428 at 100 GeV with the CELESTE Cherenkov Telescope

D. A. Smith, E. Brion, R. Britto +18

We have measured the gamma-ray fluxes of the blazars Mrk 421 and Mrk 501 in the energy range between 50 and 350 GeV (1.2 to 8.3 x 10^25 Hz). The detector, called CELESTE, used firs…

astro-ph2001★ 80 cited

Measurement of the Crab Flux Above 60 GeV with the CELESTE Cherenkov Telescope

M. De Naurois, J. Holder, R. Bazer-Bachi +29

We have converted the former solar electrical plant THEMIS (French Pyrenees) into an atmospheric Cherenkov detector called CELESTE, which records gamma rays above 30 GeV (7E24 Hz).…

astro-ph2000★ 3 cited

Observations of the supernova remnant W28 at TeV energies

G. P. Rowell, T. Naito, S. A. Dazeley +24

The atmospheric Cerenkov imaging technique has been used to search for point-like and diffuse TeV gamma-ray emission from the southern supernova remnant, W28, and surrounding regio…

astro-ph2000★ 29 cited

Very High-Energy Gamma-Ray Observations of PSR B1509-58 with the CANGAROO 3.8m Telescope

T. Sako, Y. Matsubara, Y. Muraki +31

The gamma-ray pulsar PSR B1509-58 and its surrounding nebulae have been observed with the CANGAROO 3.8m imaging atmospheric Cherenkov telescope. The observations were performed fro…

astro-ph1999

The SNR W28 at TeV Energies

G. P. Rowell, T. Naito, S. A. Dazeley +24

The southern supernova remnant (SNR)W28 was observed in 1994 and 1995 by the CANGAROO 3.8m telescope in a search formulti-TeV gamma ray emission, using the Cerenkov imaging techniq…

astro-ph1999★ 1 cited

Initial Performance of CANGAROO-II 7m telescope

Hidetoshi Kubo, S. A. Dazeley, P. G. Edwards +28

CANGAROO group constructed an imaging air Cherenkov telescope (CANGAROO-II) in March 1999 atWoomera, South Australia to observe celestial gamma-rays in hundreds GeV region. It has…