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<< 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?
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Topic revision: r1 - 30 Jul 2008,
BoudRoukema
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