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Title: Observing dark energy with SNAP

Journal Article · · Astrophysics
OSTI ID:827586

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.

Research Organization:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE Director. Office of Science. Office of High Energy Physics (US)
DOE Contract Number:
AC03-76SF00098
OSTI ID:
827586
Report Number(s):
LBNL-56022; R&D Project: PB1150; TRN: US0403564
Journal Information:
Astrophysics, Vol. 1, Issue 0406186; Other Information: Journal Publication Date: 06/07/2004; PBD: 7 Jun 2004
Country of Publication:
United States
Language:
English

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