<< Cosmo.WebHome %TOC% ---- %INCLUDE{"BenasqueNotes2008Head"}% ---+ Rob Crittendon IS ArXiv:0801.4380 * a lot from Giannantonio et al. 2008 ArXiv:0801.4380 * about 80% of ISW signal is from z < 1 for a standard Lambda model * strength of the correlation as fn of 1+z is consistent with what is expected * Qn: how do we distiguish ISW from foregrounds? * long list of effects such as: * independent of WMAP frequencies * independent of the frequences of the probe object, ranging from radio to Xray ---++ future of ISW * VSA-ISW survey * Pan-STARRS %$3\pi$% Survey * "dark energy survey" over 5000 sq. deg * Planck ---+++ long-term * SKA * LSST * Joint Dark Energy Mission / EUCLID ---++ other * Frommert et al. 2008 try to reconstruct the ISW sky * constraints on MOND/TeVeS?
This topic: Cosmo
>
WebPreferences
>
WebHome
>
BenasqueNotes2008
>
BenasqueCrittendon2008
Topic revision:
30 Jul 2008,
BoudRoukema
(raw view)
Copyright © CC-BY-SA by the contributing authors. All material on this collaboration platform is copyrighted under CC-BY-SA by the contributing authors unless otherwise noted.
Ideas, requests, problems regarding Foswiki?
Send feedback