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Measuring Cosmic Expansion and Large Scale Structure with DestinyDestiny is a simple, direct, low cost mission to determine the properties of dark energy by obtaining a cosmologically deep supernova (SN) type Ia Hubble diagram and by measuring the large-scale mass power spectrum over time. Its science instrument is a 1.65m space telescope, featuring a near-infrared survey camera/spectrometer with a large field of view. During its first two years, Destiny will detect, observe, and characterize 23000 SN Ia events over the redshift interval 0.4lo00 square degrees to measure the large-scale mass power spectrum. The combination of surveys is much more powerful than either technique on its own, and will have over an order of magnitude greater sensitivity than will be provided by ongoing ground-based projects.
Document ID
Document Type
Conference Paper
Benford, Dominic J. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Lauer, Tod R. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 24, 2013
Publication Date
August 27, 2007
Subject Category
Meeting Information
Century of Cosmology Conference(Venice)
Distribution Limits
Work of the US Gov. Public Use Permitted.