High-redshift 21cm and redshift distortions Antony Lewis Institute of Astronomy, Cambridge Anthony Challinor (IoA, DAMTP); astro-ph/0702600.
Power spectrum of the dark ages Antony Lewis Institute of Astronomy, Cambridge Work with Anthony Challinor (IoA, DAMTP); astro-ph/0702600.
Cosmological observables after recombination Antony Lewis Institute of Astronomy, Cambridge Anthony Challinor (IoA, DAMTP); astro-ph/0702600.
Cosmic bubble collisions by matthew kleban
Naoshi Sugiyama- Cosmic Microwave Background Basic Physical Process: Why so important for cosmology
Cosmic Microwave Background Carlo Baccigalupi, SISSA CMB lectures at TRR33, see the complete program at darkuniverse.uni-hd.de/view/Main/WinterSchoolLecture5.
Radiative Feedback Effects of the First Objects in the Early Universe Kyungjin Ahn The University of Texas at Austin East-Asia Numerical Astrophysics Meeting.
Jonathan Ganc Qualifier for PhD Candidacy October 12, 2009 Department of Physics, University of Texas.
CS267 – April 30th, 2013 Big Bang, Big Data, Big Iron High Performance Computing and the Cosmic Microwave Background Julian Borrill Computational Cosmology.
Atomic Precision Tests and Light Scalar Couplings Philippe Brax IPhT Saclay « The Proton Radius Puzzle » Workshop, Trento November 2012 P.B and C. Burrage,
Liam McAllister Cornell ISM08, Pondicherry December 9, 2008.
Benjamin D. Wandelt Departments of Physics and Astronomy