Solar physics with the Square Kilometre Array

Cloud Computing and the Square Kilometre Array

Preliminary Specifications for the Square Kilometre Array

Array cost versus dish diameter for an SKA mid-band scenario with a target sensitivity of A eff /T sys =10,000 m 2 K-1

Galaxy Evolution and Cosmology with the Square Kilometre Array

X iv :a st ro -p h/ 04 09 47 9v 1 2 0 Se p 20 04 Galaxy Evolution and Cosmology with the Square Kilometre Array S. Rawlings, F.B. Abdalla, S.L. Bridle, C.A. Blake, C.M. Baugh L.J. Greenhill, J.M. van der Hulst Astrophysics, Department of Physics, Keble Road, Oxford, OX1 3RH, UK Department of Physics and Astronomy, University College London, London, WC1E 6BT, UK School of Physics, University of ...

Cross correlation surveys with the Square Kilometre Array

Donnacha Kirk1, Aurélien Benoit-Lévy1, Filipe B. Abdalla∗1,2, Philip Bull3, Benjamin Joachimi1 1Department of Physics and Astronomy, University College London, London WC1E 6BT, UK 2Department of Physics and Electronics, Rhodes University, PO Box 94, Grahamstown, 6140 South Africa; 3 Institue of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, N-0315 Oslo, Norway E-mail: drg...

H I science with the Square Kilometre Array

The Square Kilometre Array (SKA) will be a formidable instrument for the detailed study of neutral hydrogen (H I) in external galaxies and in our own Galaxy and Local Group. The sensitivity of the SKA, its wide receiver bands, and the relative freedom from radio frequency interference at the SKA sites will allow the imaging of substantial number of high-redshift galaxies in H I for the first ti...