High Redshift Type Ia Supernova Lightcurves

Details High Redshift Type Ia Supernova Lightcurves High Redshift Type Ia Supernova Lightcurves

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...204.6316s&link_type=abstract

American Astronomical Society Meeting 204, #63.16; Bulletin of the American Astronomical Society, Vol. 36, p.983

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Scientific paper

We report on results from 14 additional supernovae observed by the Supernova Cosmology Project. Most of the supernovae were found during observing runs in fall of 1997 and spring of 1998, along with other supernova data already published, as well as from spring 2001. All supernova lightcurves were fit to empirically determined fits to find the most probable values for the "stretch" and peak supernova flux, as had been done with previous SCP ground-based observations. Each supernova in this group has been confirmed spectroscopically or based on the lightcurve fit, with redshift known from galaxy spectra. We show the current status of these lightcurves.

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