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Abstract Observed CMB polarization maps can be split into gradient-like (E) and curl- like (B) modes. I review the details of this decomposition, and the.
NITheP WITS node seminar: Dr. H. Cynthia Chiang (University of Kwa-Zulu Natal)
Proracun VF
Cosmic Microwave Background Carlo Baccigalupi, SISSA CMB lectures at TRR33, see the complete program at darkuniverse.uni-hd.de/view/Main/WinterSchoolLecture5.
Cosmic Shear with HST Jason Rhodes, JPL Galaxies and Structures Through Cosmic Times Venice Italy March 27, 2006 with Richard Massey, Catherine Heymans.
The Einstein Inflation Probe: Mission Concept Study Gary Hinshaw, NASA/GSFC May 12, 2004 Beyond Einstein @ SLAC.
CMB polarisation results from QUIET Ingunn Kathrine Wehus 23rd Rencontres de Blois, 1/6 -11.
[RADIO 250] LEC 09 Basic Ultrasound (1).pdf
Confinement of spin diffusion to single molecular layers in layered organic conductor crystals András Jánossy 1 Ágnes Antal 1 Titusz Fehér 1 Richard Gaál.
The Cosmic Microwave Background Lecture 2 Elena Pierpaoli.
Planning for B s Mixing for Winter 2005
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