UBVRI photometry of SN1994D in NGC 4526

Details UBVRI photometry of SN1994D in NGC 4526 UBVRI photometry of SN1994D in NGC 4526

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...294l...9w&link_type=abstract

Astronomy and Astrophysics, v.294, p.L9

Astronomy and Astrophysics

Astrophysics

4

Supernovae, Sn1994D, Photometry, Distance

Scientific paper

In this paper, we present UBVRI photometric results of SN1994D which covers the period from March 11 to April 4. All these data were obtained with a Ford 2048x2048 CCD, which has been attached to the 60/90cm Schmidt telescope in Xinglong station, BAO. The light curves indicate that the supernova is a normal type Ia, a good distance indicator of its parent galaxy. The distance modulus of NGC 4526 is given as 30.07+/-0.42.

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