Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996hst..prop.6431m&link_type=abstract
HST Proposal ID #6431
Astronomy and Astrophysics
Astrophysics
Hst Proposal Id #6431 Cosmology
Scientific paper
Many fundamental problems in cosmology and astrophysics remain unsettled because the value of the expansion rate is uncertain to a factor of two. The refurbished HST has provided the opportunity to break this impasse. We propose to complete a program, which in combination with other GTO and GO work should lead to a measurement of H_0 to 10 Our main goal is the observation of Cepheids in 19 fields in 18 nearby galaxies, for the purpose of calibrating the best secondary distance indicators, including the infrared Tully-Fisher relation, the Planetary Nebula Luminosity Function, the Surface Brightness Fluctuation method, the type Ia supernovae standard candle and the type II supernova Expanding Photosphere Method. From Cycle 4 observations we have inferred H_0 = 80 +/- 17 km/sec/Mpc. Other groups have adopted the same strategy in part, and one has obtained a significantly lower value of H_0 supported by HST observations of supernova host galaxies. In this proposal we show how these claims can be resolved with Cycle 6 data to attain an unequivocable result from the Key Project. Measurement of Cepheids in the Virgo and Fornax clusters receives strong emphasis in this final cycle. Unique features of this proposal include an end-to-end approach to the extragalactic distance scale, and a careful error budget for the Key Project.
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