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Observing Dark Energy with SNAP

2004/06/07 by Eric V. Linder, Linder, Eric V.
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #FOS: Physical sciences

paper · pdf · doi:10.48550/arxiv.astro-ph/0406186

openalex publication_date 2004/06/07 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/01

Abstract

The nature of dark energy is of such fundamental importance -- yet such a mystery -- that a dedicated dark energy experiment should be as comprehensive and powerfully incisive as possible. The Supernova/Acceleration Probe robustly controls for a wide variety of systematic uncertainties, employing the Type Ia supernova distance method, with high signal to noise light curves and spectra over the full redshift range from z=0.1-1.7, and the weak gravitational lensing method with an accurate and stable point spread function.

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