Deep photometry of supernovae

Details Deep photometry of supernovae Deep photometry of supernovae

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988msngr..52...16d&link_type=abstract

ESO Messenger (ISSN 0722-6691), June 1988, p. 16-18.

Astronomy and Astrophysics

Astronomy

4

Astronomical Photometry, Deep Space, Supernovae, Red Shift, Sky Surveys (Astronomy), Stellar Evolution

Scientific paper

Photometric observations of SNs have been initiated at intermediate and late stages, extending to much fainter limits the extensive SN survey of Rosino over the last 30 years. The correspondence between observed and estimated magnitudes via linear decline for the objects of the sample is judged to be good. Before ascertaining the intrinsic object properties, the reddening due to the galactic and internal absorption of the parent galaxy must be taken into account. Also noted are the features of SN 1986 g in NGC 5128.

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