Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-04-06
Astronomy and Astrophysics
Astrophysics
32 pages, 5 figures, Accepted Astrophysical Journal
Scientific paper
10.1086/306106
We present an empirical method which measures the distance to a Type Ia supernova (SN Ia) with a precision of ~ 10% from a single night's data. This method measures the supernova's age and luminosity/light-curve parameter from a spectrum, and the extinction and distance from an apparent magnitude and color. We are able to verify the precision of this method from error propagation calculations, Monte Carlo simulations of well-sampled SNe Ia, and the Hubble diagram of scarcely observed supernovae. With the reduction in telescope time needed, this method is three to four times more efficient for measuring cosmological parameters than conventional light-curve based distance estimates.
Filippenko Alexei V.
Kirshner Robert P.
Nugent Peter
Perlmutter Saul
Riess Adam G.
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