It can probe the dark matter on scales where other methods ... 350 megapixels. Megacam: Build a big camera... Put it on a good telescope... Such as the CFHT ...
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 ...
compatible with a cosmological constant, WL~0.7. SNe: ... Produces calibrated star catalogs in the CFHTLS Deep fields, in natural Megacam magnitudes. ...
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
Christophe Alard (IAP), R mi Cabanac (CFHT), Bernard Fort (IAP) ... automated softwares. How to find them? Develop automated procedure to search the lenses ...
m me si les r sultats actuels marquants viennent plut t de la cosmologie (SNLS, ... les r percutions sur le fonctionnement actuel d'un CFH aujourd'hui tr s ...
Interface with CNES and industrial(s) Interface with Berkeley scientific group WL and SN ... B.Milliard (LAM) WL scientist. WL SNAP Group contact. J.P Kneib (LAM) ...
Testing Galfit. Clemens Trachternach1, Olaf Schmith sen1, Gijs Verdoes Klein2, ... 3Argelander Institut f r Astronomie, Uni ... to fit it with a new component ...
Outline Introduction Current Status Discussion Future Introduction The development of cosmology is largely driven by observations The accelerating expansion of the ...
WHIM Backlight Scaling relation fudge factor Point source contaminant Cooling problem get-out clause AGN/GALAXY COEVOLUTION Kirpal Nandra Imperial College London
Tracking quintessence by cosmic shear. constraints from ... quintessence at low-z by SNe cosmic shear, using high-z informations (TT-CMB/Cl normalization) ...
PI : Chris Martin (Caltech) PI : O. LeF vre (Marseille) G. Vettolani (Bologna) THE GALEX-VVDS DEEP SURVEYS : Evolution of the Far UV luminosity Function
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: ...
For a given quintessence potential V(f), we set the 'initial conditions' at z=0 ... Approximating Quintessence for Phenomenology Friedmann Equations DM B. 1 ...
Major questions. What is the Dark Matter? What is the Dark Energy/?? Scalar field? ... Can marginalise over nuisance' parameters, such as a bias in the photo-zs ...
Cliquez pour modifier les styles du texte du masque. Deuxi me niveau. Troisi me niveau ... Cliquez pour modifier les styles du texte du masque. Deuxi me niveau ...
... Billions of galaxies, HI mass function evolution poorly ... Jy- mJy (up to 1016 M?? of HI) Angular scale 5' T 30', freq res 500 khz. Challenging theory ...
Colloque ... Large-scale structure induces correlations between the observed shapes of ... Quintessence study underway , aiming to. constrain, for example, ...
Gauss-Bonnet Lagrangian. Solution in static spherical. symmetry in a linearized. PPN metric with ... coupled Gauss-Bonnet. see L. A., C. Charmousis, S. Davis ...
Cosmology with Spectroscopic and Photometric Redshift Surveys The post-2dF/SDSS/WMAP3 universe The 2MASS Redshift Survey The Photo-z MegaZ-LRG The Dark Energy Survey
... of luminous red galaxies and misalignment with their host dark matter halos ... Directly probe the matter distribution. es. Observable. Ellipticity of ...
EVOLUCI N DEL PLANO FUNDAMENTAL DE GALAXIAS DE TIPO TEMPRANO EN EGS Mirian Fern ndez Lorenzo Colaboradores: J. Cepa, A. Bongiovanni, A.M. P rez Garc a , A ...
A universal force in 4D mediated by a massless tensor field. What is ... coupled Gauss-Bonnet. see L. A., C. Charmousis, S. Davis 2006. Boisseau et al. 2000 ...
A critical review of global efforts in this area. Assess what ... weak lensing and acoustic baryonic oscillations (based on photo-z, i.e. requires IR as well) ...
Galaxy properties in different environments: Observations. Michael Balogh ... galaxies also observed (e.g. Chester & Roberts 1964; Visvanathan 1981; Tully, ...
Une m thode de mesure bas e sur les SNIa, chandelles standardisables. ... mesurer l' quation d' tat du vide cosmique w(z)=p/r. permet d'acc der la nature de ...
Shear, Magnification, Amplification. ?1. ?2. e.g. Gunn 1967 (Feynman 1964); Kristian & Sachs 1966 ... Can also use MAGNIFICATION or AMPLIFICATION. Cosmic shear: ...
Old view: Theory prior = delta function of THE correct one and only theory ... DUNE-WL (50% sky, gals @z = 0.1-1.1, 35/min2 ) Planck1yr. es=0.02 0.07-0.06 ...
Standard Rulers vs Standard Candles: Constraints Comparison. Gamma Ray Bursts as Standard Candles ... Majajan, Sarkar, Padmanbhan, Phys.Lett.B641:6-10,2006 ...
HST, Spitzer, VLA, GALEX, CFHT LS blah blah blah 'AEGIS' ApJL special issue (~20 ... AGN contribution to the total luminosity of the universe (c.f. stars) ...
AGN Feedback deposits large amounts of energy influencing the evolution of ... (Overzier, Venemans, Kurk, Miley, de Breuk, van Breugel, Maschietto, van Breugel, ...
Scanning-free-automatized detection pipeline has been set up (shapelet-neural ... 250H/year of photo. Rencontre de Monriond 2006 SNLS 1st year cosmological results ...