Lance Miller, Catherine Heymans, Alan Heavens, Ludo Van Waerbeke. Miller et ... Measure PSF create a model convolve with PSF determine the likelihood of the fit ...
Title: CMB Cosmological Parameter Extraction Author: CITA Last modified by: bond Created Date: 9/10/2001 6:14:33 PM Document presentation format: On-screen Show
Shear, Magnification, Amplification. ?1. ?2. e.g. Gunn 1967 (Feynman 1964); Kristian & Sachs 1966 ... Can also use MAGNIFICATION or AMPLIFICATION. Cosmic shear: ...
Zolt n Haiman, Morgan May, and John Kehayias. Outline. Shear-Selected Galaxy Clusters ... Abundance of galaxy clusters (redshift evolution) is exponentially ...
1. Dark Energy and Neutrino Mass Constraints. from WL, SN Ia and RGA ... The existence of non-zero neutrino masses ... The massive neutrinos could suppress the ...
Cosmic Shear with HST. Jason Rhodes, JPL. Galaxies and Structures Through Cosmic Times ... with Richard Massey, Catherine Heymans & Alexie Leauthaud ...
Observation of (molecular absorption lines. in the light of quasars ) ... Different couplings of cosmon to proton and neutron. Differential acceleration ...
L1: The Cosmic Microwave Background & the Thermal History of the Universe. Dick Bond ... Non april fool. Is the universe like a soccer ball? The CMB data decides: ...
Coordinate difference (comoving distance) is not the same as physical distance. Can rewrite conformal ... Affine parameter can be replaced by comoving distance ...
Size magnitude relation. Gardner & Satyapal: Sizes from STIS HDF south images ... Survey to 25th magnitude. Virgo truth' M 5x1013Msun. M 1x1014Msun. Dotted ...
C. Baltay, W. Emmet, A. Szymkowiak, D. Rabinowitz. Yale U. ... Fermi National Laboratory. J. Albert, R. Ellis, R. Massey , R. Smith, K. Taylor, A. Weinstein ...
Orbits and velocities of stars and galaxies measurement of gravitational potential ... stars , galaxies, clusters. One primordial fluctuation spectrum describes ...
Gradient of deflection coherent distortions of galaxy shapes ... Pixellation (=boxcar smoothing subsampling) Noise. Some of the information loss irretrievable ...
There are good methods for deconvolving the PSF. So what's the problem? ... PCA technique is effective at removing systematic shape errors due to PSF. ...
Tracking quintessence by cosmic shear. constraints from ... quintessence at low-z by SNe cosmic shear, using high-z informations (TT-CMB/Cl normalization) ...
Link galaxies to their host halos ... start to see 'two-halo' term unless galaxies are truly isolated ... need to use isolated galaxies in g-g analysis, must ...