Mathematics – Logic
Scientific paper
Sep 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998stin...9932026p&link_type=abstract
Technical Report, Thermonuclear supernovae Office of Energy Research
Mathematics
Logic
Red Shift, Supernovae, Cosmology, Batch Processing, Stellar Spectra, Light Curve, Calibrating, Astronomical Observatories
Scientific paper
Our search for high-redshift Type Ia supernovae discovered, in its first years, a sample of seven supernovae. Using a 'batch' search strategy, almost all were discovered before maximum light and were observed over the peak of their light curves. The spectra and light curves indicate that almost all were Type Ia supernovae at redshifts z = 0.35 - 0.5. These high-redshift supernovae can provide a distance indicator and 'standard clock' to study the cosmological parameters q0 , (Lambda), (Omega)0 , and H0. This presentation and the following presentations of Kim et al. (1996), Goldhaber et al. (1996), and Pain et al. (1996) will discuss observation strategies and rates, analysis and calibration issues, the sources of measurement uncertainty, and the cosmological implications, including bounds on q0 , of these first high-redshift supernovae from our ongoing search.
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