Cosmology with the 21cm line
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.
The Very Small Array Angela Taylor & Anze Slosar Cavendish Astrophysics University of Cambridge.
Radio Galaxies as Viewed by Chandra: The 3C Snapshot Surveys and Other Aspects D. E. Harris, SAO ~~~~~~~ Collaborators: Massaro, F., Axon, D., Balmaverde,
Acknowledgments
Radio-loud AGN energetics with LOFAR Judith Croston LOFAR Surveys Meeting 17/6/09.
LOFAR-UK A proposal to STFC PPRP PI Professor Rob Fender (Southampton) On behalf of the following consortium: Liverpool John Moores University, The Open.
260404Astroparticle Physics1 Astroparticle Physics Key Issues Jan Kuijpers Dep. of Astrophysics/ HEFIN University of Nijmegen.
The Very Small Array
Deep, high resolution radio imaging of the Subaru/XMM- Newton Deep Survey field
A GPU Implementation of Extragalactic Radio Source Detection A CUDA Approach
Radio Galaxies as Viewed by Chandra: The 3C Snapshot Surveys and Other Aspects
