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Paper: Galactic SNRs in the PMN Survey
Volume: 271, Neutron Stars in Supernova Remnants
Page: 387
Authors: Filipovic, M. D.; Stupar, M.; Jones, P. A.; White, G. L.
Abstract: We used the Parkes-MIT-NRAO (PMN) survey (Condon et al. 1993) to investigate a complete sample of Galactic supernova remnants (SNRs). We measured flux density of the whole sample at 4.85 GHz. From the Green (2000) list of 225 galactic SNRs, some 141 SNRs are covered with the Parkes radio telescope and 84 with the Green Bank survey. About 4% of all measured SNR fluxes are missing due to blank fields (no observations) or large size of the SNRs (>30 arcmin). Also, a considerable number of SNRs (~10%) are embedded in surrounding HII regions or simply are not resolved (SNR sizes below 5 arcmin). Here, we report our measured 4.85 GHz flux densities of 121 Galactic SNR from PMN South survey.
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