Cosmology with the SKA -- overview

Advancing Astrophysics with the Square Kilometre Array PoS 016 (2014)

Authors:

R Maartens, FB Abdalla, Matthew Jarvis, FTSKAC Swg

Abstract:

The new frontier of cosmology will be led by three-dimensional surveys of the large-scale structure of the Universe. Based on its all-sky surveys and redshift depth, the SKA is destined to revolutionize cosmology, in combination with future optical/ infrared surveys such as Euclid and LSST. Furthermore, we will not have to wait for the full deployment of the SKA in order to see transformational science. In the first phase of deployment (SKA1), all-sky HI intensity mapping surveys and all-sky continuum surveys are forecast to be at the forefront on the major questions of cosmology. We give a broad overview of the major contributions predicted for the SKA. The SKA will not only deliver precision cosmology -- it will also probe the foundations of the standard model and open the door to new discoveries on large-scale features of the Universe.

Evolution in the bias of faint radio sources to z ∼ 2.2

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 440:3 (2014) 2322-2332

Authors:

SN Lindsay, MJ Jarvis, K McAlpine

Probing the bright radio flare and afterglow of GRB 130427A with the Arcminute Microkelvin Imager

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 440:3 (2014) 2059-2065

Authors:

GE Anderson, AJ van der Horst, TD Staley, RP Fender, RAMJ Wijers, AMM Scaife, C Rumsey, DJ Titterington, A Rowlinson, RDE Saunders

Galaxy and Mass Assembly: the evolution of bias in the radio source population to z∼1.5

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 440:2 (2014) 1527-1541

Authors:

SN Lindsay, MJ Jarvis, MG Santos, MJI Brown, SM Croom, SP Driver, AM Hopkins, J Liske, J Loveday, P Norberg, ASG Robotham

A search for H i absorption in nearby radio galaxies using HIPASS

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 440:1 (2014) 696-718

Authors:

JR Allison, EM Sadler, AM Meekin