SIMBAD references

2005ApJ...619L.163K - Astrophys. J., 619, L163-L166 (2005/February-1)

Detection of gamma rays around 1 TeV from RX J0852.0-4622 by CANGAROO-II.

KATAGIRI H., ENOMOTO R., KSENOFONTOV L.T., MORI M., ADACHI Y., ASAHARA A., BICKNELL G.V., CLAY R.W., DOI Y., EDWARDS P.G., GUNJI S., HARA S., HARA T., HATTORI T., HAYASHI S., ITOH C., KABUKI S., KAJINO F., KAWACHI A., KIFUNE T., KIUCHI R., KUBO H., KURIHARA T., KUROSAKA R., KUSHIDA J., MATSUBARA Y., MIYASHITA Y., MIZUMOTO Y., MURAISHI H., MURAKI Y., NAITO T., NAKAMORI T., NAKASE T., NISHIDA D., NISHIJIMA K., OHISHI M., OKUMURA K., PATTERSON J.R., PROTHEROE R.J., SAKAMOTO N., SAKAMOTO Y., SWABY D.L., TANIMORI T., TANIMURA H., THORNTON G.J., TSUCHIYA K., WATANABE S., YAMAOKA T., YANAGITA S., YOSHIDA T. and YOSHIKOSHI T.

Abstract (from CDS):

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.

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Journal keyword(s): Gamma Rays: Observations - Stars: Supernovae: Individual: Alphanumeric: RX J0852.0-4622

Simbad objects: 8

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