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 |
|---|---|
| Pages (from-to) | L163-L166 |
| Journal | Astrophysical Journal |
| Volume | 619 |
| Issue number | 2 II |
| DOIs | |
| Publication status | Published - 1 Feb 2005 |
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