A progress report on the Berkeley search for distant supernovae to measure Omega

Details A progress report on the Berkeley search for distant supernovae to measure Omega A progress report on the Berkeley search for distant supernovae to measure Omega

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992daec.conf..395p&link_type=abstract

In Distribution of Matter in the Universe, 2nd DAEC mtg, ed. G.A. Mamon and D. Gerbal (Meudon: Obs. de Paris) p. 395-399

Physics

Scientific paper

Over the past two years, in collaboration with the Anglo-Australian Observatory, we have constructed a prototype version of the hardware and software needed to discover distant supernovae for a measurement of Omega, the ratio of the average density of the universe to the critical density. To make this measurement, we will use Type Ia supernova, which are now thought to be adequate standard candles for this purpose.

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