SIMBAD references

2008ApJ...683..383E - Astrophys. J., 683, 383-388 (2008/August-2)

CANGAROO-III search for gamma rays from Kepler's supernova remnant.

ENOMOTO R., HIGASHI Y., YOSHIDA T., TANIMORI T., BICKNELL G.V., CLAY R.W., EDWARDS P.G., GUNJI S., HARA S., HARA T., HATTORI T., HAYASHI S., HIRAI Y., INOUE K., KABUKI S., KAJINO F., KATAGIRI H., KAWACHI A., KIFUNE T., KIUCHI R., KUBO H., KUSHIDA J., MATSUBARA Y., MIZUKAMI T., MIZUMOTO Y., MIZUNIWA R., MORI M., MURAISHI H., MURAKI Y., NAITO T., NAKAMORI T., NAKANO S., NISHIDA D., NISHIJIMA K., OHISHI M., SAKAMOTO Y., SEKI A., STAMATESCU V., SUZUKI T., SWABY D.L., THORNTON G., TOKANAI F., TSUCHIYA K., WATANABE S., YAMADA Y., YAMAZAKI E., YANAGITA S., YOSHIKOSHI T. and YUKAWA Y.

Abstract (from CDS):

Kepler's supernova, discovered in 1604 October, produced a remnant that has been well studied observationally in the radio, infrared, optical, and X-ray bands, and theoretically. Some models have predicted a TeV gamma-ray flux that is detectable with current Imaging Cerenkov Atmospheric Telescopes. We report on observations carried out in 2005 April with the CANGAROO-III Telescope. No statistically significant excess was observed, and limitations on the allowed parameter range in the model are discussed.

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Journal keyword(s): Gamma Rays: Observations - supernovae: individual (Kepler's SNR)

Simbad objects: 5

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