Photometric investigation of bright type II-P Supernova 2004dj
D. Yu. Tsvetkov, V. P. Goranskiy, N. N. Pavlyuk
TL;DR
This paper presents extensive photometric data of supernova 2004dj over 1200 days, analyzing its light curve and comparing it with the host cluster to understand its properties and peculiarities.
Contribution
It provides a detailed long-term photometric dataset for SN 2004dj and examines the supernova's behavior and its relation to the host cluster, with observations of minor peculiarities.
Findings
Photometric behavior typical for SNe II-P
No significant changes in host cluster S96 after outburst
Minor peculiarities observed in the supernova's light curve
Abstract
CCD UBVRI photometry is presented for type II SN 2004dj for about 1200 days, starting day 2 past discovery. The photometric behaviour is typical for SNe II-P, although some minor peculiarities are noticed. We compare the photometric data for the host cluster S96 before and after SN 2004dj outburst and do not find any significant changes.
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Taxonomy
TopicsGamma-ray bursts and supernovae