Abstract
We have detected gamma-ray emission at the 6 ? level at energies greater than 500 GeV from the supernova remnant RX J0852.0-4622 (G266.2-1.2) using the CANGAROO-II imaging atmospheric Cerenkov telescope. The flux was 0.12 times that of Crab at 1 TeV. The signal centroid is consistent with the peak of the X-ray emission in the northwest rim of the remnant. ? 2005. The American Astronomical Society. All rights reserved.
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CITATION STYLE
Katagiri, H., Enomoto, R., Ksenofontov, L. T., Mori, M., Adachi, Y., Asahara, A., … Yoshikoshi, T. (2005). Detection of Gamma Rays around 1 TeV from RX J0852.0-4622 by CANGAROO-II. The Astrophysical Journal, 619(2), L163–L166. https://doi.org/10.1086/427980
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