2005/04/05 by A. Pastorello, I. Aretxaga, Pastorello, A. +7
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Nuclear Physics and Applications #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0504116
5 pages, 3 figures. To appear in proceedings of the International Conference "1604-2004: Supernovae as Cosmological Lighthouses" (Padova, Italy, June 16-19, 2004), eds. M. Turatto, W. Shea, S. Benetti and L. Zampieri, ASP conference Series
arxiv created 2005/04/05 · openalex publication_date 2005/04/05 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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.