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Spectroscopic and Photometric Observations of SN IIn 1995N

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arxiv astro-ph/0504116 v1 pith:MHPQ4TO5 submitted 2005-04-05 astro-ph

classification astro-ph
keywords observationsallowavailablebandsdatadecadeenergyestimate
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We present the results of a long-term program of monitoring of the famous SN 1995N, observed both in photometry (UBVRIJHK bands) and optical spectroscopy. The observations span a period of about 9 years. These new data, together with others available in literature, extend from the X-ray wavelengths to the radio, and allow to estimate the total energy radiated by the supernova over a decade after its explosion.

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