Catalog Service: SN 2011dh. The first two years
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We present optical and near-infrared (NIR) photometry and spectroscopy as well as modelling of the lightcurves of the Type IIb supernova (SN) 2011dh. Our extensive dataset, for which we present the observations obtained after day 100, spans two years, and complemented with Spitzer mid-infrared (MIR) data, we use it to build an optical-to-MIR bolometric lightcurve between days 3 and 732.
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This resource was registered on: 2015 Aug 21 07:40:59ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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