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Observing dark energy with SNAP

Title: Observing dark energy with SNAP
Authors: Linder, Eric V.; Collaboration, SNAP
Contributors: United States. Department of Energy. High Energy Physics Division.
Source: Journal Name: Astrophysics; Journal Volume: 1; Journal Issue: 0406186; Other Information: Journal Publication Date: 06/07/2004
Publisher Information: Lawrence Berkeley National Laboratory
Publication Year: 2004
Collection: University of North Texas: UNT Digital Library
Subject Terms: Lawrence Berkeley Laboratory; Probes; Spectra; 72 Physics Of Elementary Particles And Fields; 71 Classical And Quantum Mechanics; General Physics
Description: 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.
Document Type: article in journal/newspaper
File Description: vp.; Text
Language: English
Relation: osti: 827586; https://digital.library.unt.edu/ark:/67531/metadc780134/; ark: ark:/67531/metadc780134
Availability: https://digital.library.unt.edu/ark:/67531/metadc780134/
Accession Number: edsbas.EC375AC4
Database: BASE