Abstract
We have detected gamma-ray emission at the 6 σ 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.
Original language | English |
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Pages (from-to) | L163-L166 |
Journal | Astrophysical Journal |
Volume | 619 |
Issue number | 2 II |
DOIs | |
Publication status | Published - 1 Feb 2005 |