VRIJHK photometry of SN 2002cv (Elias-Rosa+, 2008)

Details VRIJHK photometry of SN 2002cv (Elias-Rosa+, 2008) VRIJHK photometry of SN 2002cv (Elias-Rosa+, 2008)

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..83840107e&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/384/107. Originally published in: 2008MNRAS.384..107E

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Supernovae, Photometry: Ubvri, Photometry: Infrared

Scientific paper

The fact that another SN Ia, SN 2002bo, exploded in the same galaxy a few months before SN 2002cv, makes available pre-discovery optical and near-IR (NIR) data and hence templates for photometric measurements via image subtraction. SN 2002cv was observed for seven months, from day 10.7 to +205.9 relative to I-band maximum light. Here, we present the data collected by four different teams: University of California, Berkeley (USA), Imperial College (UK), Padova Observatory (INAF, Italy) and Teramo Observatory (INAF, Italy).
(4 data files).

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