PPT-Simulating Interferometers for the CMB Sky

Eric Lopez UC Berkeley With Peter Timbie and the Observational Cosmology Group UW Madison Outline of Talk CMB 101 What is a Power Spectrum Polarization and Bmodes The EPIC mission The Basics of Interferometers. Coffee makers with other date codes are not affected The model number and date code are located on the nameplate of the coffee maker as shown below The name plate is on the bottom of the coffee maker If you have a CM12B One Cup Coffee Maker date cod Taxis buses and transfer buses to terminals rental cars and hotels are located outside the terminals Du 57572r h57572r You are here F57590r alla Public rea F57590r resen 57572rer Passengers only Tr57573dl 57590st Internet WiFi 57590ver hela 64258ygp & Large scale structure. Tarun Souradeep. I.U.C.A.A. .. Cosmology . IUCAA . VSP program. (. May 18-22, . 2012). Lec. . 2:. Cosmic Content. Perturbed Universe . Simple. … yet, an . exotic. Gaussianities. Antony Lewis. http://cosmologist.info/. Lewis . arXiv:1107.5431. Hanson . & Lewis . arXiv:0908.0963. Lewis, Challinor & Hanson . arXiv:1101.2234. Pearson, Lewis & Regan . arXiv:1201.1010. The value of . reionization. fraction derived from CMB polarization measurements has decreased steadily since WMAP2003 (WMAP2005, WMAP2007, WMAP2011, and Planck 2015). The final word from Planck is not out yet , and whenever it is out, it will surely not be “a 100-sigma measurement” of . Gaussianity. measurement. Dr. . Rajib. . Saha. Assistant Professor. Physics Department. IISER Bhopal. INDO-UK Scientific Seminar: Confronting particle cosmology with PLANCK and LHC . IUCAA, August 11, 2011. G. g. Distributions. What is . G. g. ?. How are . G. g. ’s. measured?. What does the standard model predict?. Simulating . G. g. distributions.. Constraining the . Oslo method. .. Testing the Porter-Thomas distribution. Towards the first detection using SPT polarisation. ASA 2016 meeting, . Sydney. 04. 07. 2016. Srinivasan. . Raghunathan. School of Physics. University of Melbourne. In a nutshell . …. . South Pole Telescope – Observes CMB (both T, and P).. Garnero. 2007. McNamara & . Zhong. 2005. Mantle seismic heterogeneity as a function of depth. Romanowicz. , 2003. We expect a thermal boundary layer at the CMB. Lay et al., 2008. We expect denser mantle “dregs” to settle to the bottom. Activities funded by NASA proposal: . PI Steve Meyer entire CMB community. Workshops:. The Path to CMBPOL: Upcoming Measurement of CMB Polarization, Chicago July 1-3, 2009. Technology Development for a CMB Probe of Inflation, Boulder, 25-28 August 2008. . In order to simulate the performance of an interferometer, 20 by 20 degree sections were extracted from the simulated CMB map. For each array configuration tested a map of . uv. plane coverage was created and then applied to the Fourier transform of the CMB section. The power spectra were then extracted by computing the variance in an annulus with a radius given by the . . In order to simulate the performance of an interferometer, 20 by 20 degree sections were extracted from the simulated CMB map. For each array configuration tested a map of . uv. plane coverage was created and then applied to the Fourier transform of the CMB section. The power spectra were then extracted by computing the variance in an annulus with a radius given by the . 1 A Brief History of LIGO One hundred years ago, using his recently general relativity theory, Albert Einstein predicted the existence of gravitational waves and described their properties. To Einstei 1ABriefHistoryofLIGOOnehundredyearsagousinghisrecentlygeneralrelativitytheoryAlbertEinsteinpredictedtheexistenceofgravitationalwavesanddescribedtheirpropertiesToEinsteinthesewavesseemedtooweakevertobe