Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

Designing a space-based galaxy redshift survey to probe dark energy.

Wang, Y. and Percival, W. and Cimatti, A. and Mukherjee, P. and Guzzo, L. and Baugh, C.M. and Carbone, C. and Franzetti, P. and Garilli, B. and Geach, J.E. and Lacey, C.G. and Majerotto, E. and Orsi, A. and Rosati, P. and Samushia, L. and Zamorani, G. (2010) 'Designing a space-based galaxy redshift survey to probe dark energy.', Monthly notices of the Royal Astronomical Society., 409 (2). pp. 737-749.

Abstract

A space-based galaxy redshift survey would have enormous power in constraining dark energy and testing general relativity, provided that its parameters are suitably optimized. We study viable space-based galaxy redshift surveys, exploring the dependence of the Dark Energy Task Force (DETF) figure-of-merit (FoM) on redshift accuracy, redshift range, survey area, target selection and forecast method. Fitting formulae are provided for convenience. We also consider the dependence on the information used: the full galaxy power spectrum P(k), P(k) marginalized over its shape, or just the Baryon Acoustic Oscillations (BAO). We find that the inclusion of growth rate information (extracted using redshift space distortion and galaxy clustering amplitude measurements) leads to a factor of ∼3 improvement in the FoM, assuming general relativity is not modified. This inclusion partially compensates for the loss of information when only the BAO are used to give geometrical constraints, rather than using the full P(k) as a standard ruler. We find that a space-based galaxy redshift survey covering ∼20 000 deg2 over Graphic with σz/(1 +z) ≤ 0.001 exploits a redshift range that is only easily accessible from space, extends to sufficiently low redshifts to allow both a vast 3D map of the universe using a single tracer population, and overlaps with ground-based surveys to enable robust modelling of systematic effects. We argue that these parameters are close to their optimal values given current instrumental and practical constraints.

Item Type:Article
Additional Information:http://adsabs.harvard.edu/abs/2010MNRAS.409..737W
Keywords:Cosmology: observations, Distance scale, Large-scale structure of Universe.
Full text:(VoR) Version of Record
Download PDF
(889Kb)
Status:Peer-reviewed
Publisher Web site:http://dx.doi.org/10.1111/j.1365-2966.2010.17335.x
Publisher statement:This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2010 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Date accepted:No date available
Date deposited:19 February 2015
Date of first online publication:December 2010
Date first made open access:No date available

Save or Share this output

Export:
Export
Look up in GoogleScholar