PDF-Lensing from Planck

Antony Lewis On behalf of the Planck Collaboration several slides credit Duncan Hanson httpcosmologistinfo Observed CMB temperature power spectrum Perturbations accurately linear and Gaussia. Surveys of large scale structure will probe Dark Energy by measuring the BAO scale vs. redshift. . Planned:. DESI, Euclid, WFIRST, .... 2. Hydrogen Intensity Mapping. To measure BAO scale there is no need to resolve individual galaxies. Map intensity of HI gas using redshifted 21 cm emission along the line of sight.. Uro. š. . Seljak. UC Berkeley/LBNL. Dec 18. 2014. Goals and methods. Goals: testing Lambda CDM model . . and its e. xtensions . Testing inflation. Methods: redshift distance relation (SN, BAO…) . Martin Kunz. University of . Geneva & AIMS South Africa. outline. what is the problem?. . dark energy theory. action based models. phenomenological approach. observations. simple principles. current constraints from Planck+. FUNDAMENTAL CONCEPTS OF QUANTUM PHYSICS. . Thermal radiation: The radiation emitted by a body as a result of temperature.. . Blackbody : A body that surface absorbs all the thermal radiation incident on . &. Primordial Gravitational Waves. Jun-Qing Xia. Key Laboratory of Particle Astrophysics, IHEP. Planck Member. CHEP, PKU, April 3, 2014. BICEP2. . Paper (arXiv:1403.3985). 2. Tensor Modes Detection by BICEP2. Kaiki Taro Inoue . (KINDAI U.). Seminar. @Osaka U 22 Feb 2017. Outline. Missing Satellite Problem. Gravitational Lensing . Substructure vs Line-of-sight Halos. ALMA Observations (SDP.81, MG0414+0534). Advanced Chemistry. Ms. . Grobsky. Food For Thought. Rutherford’s model became known as the “planetary model”. The “sun” was the positively-charged dense nucleus and the negatively-charged electrons were the “planets”. Principles & Practice of Remote Sensing (PPRS) . Revision. Dr. Mathias (Mat) Disney. UCL Geography. Office: 113, Pearson Building. Tel: 7670 0592. Email: . mdisney@ucl.geog.ac.uk. www.geog.ucl.ac.uk. Dept. of Physics/CERCA/ISO. Case Western Reserve University. CMB@. 50. June 10-12, 2015 . IAS . Princeton, NJ. Collaborators: . C. . Copi. , D. . Huterer. , D. Schwarz; A. Yoho. ; Simone . Aiola. , A. for. Innovation . and. . Competition. | . Munich. The Digital Single Market Copyright Directive Proposal and beyond:. Towards a ‘toolbox’ for future European Copyright Law. . GRUR meets Brussels Workshop 2017. Ue. -Li Pen. Tingting. Lu. Olivier Dore. Cosmological Errors. How do we know errors on measurement and theory?. For Gaussian field, P(k) is 2-PCF, its error (Fisher) is 4-PCF, and the error on Fisher is 8-PCF.. Michele Liguori. Department of Physics and Astronomy, University of . Padova. On behalf of the Planck collaboration. . CMB basics. In big bang cosmology the Universe is initially in a hot and dense state. Moriond. (Cosmology). 21. st. March 2016. Current and future constraints . on . n. eutrino. physics. . from. . c. osmology. What do we . not. know about neutrinos?. We . only know their mass-squared differences…. 6. Extragalactic Microlensing. Wambsganss. . 2001. /sharp caustic crossing. /2,3-pt lens. Local Group vs. Extragalactic Microlensing. =k. Local Group Microlensing – . very very low optical depth.