Hintze Centre for Astrophysical Surveys

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Radio polarimetry as a probe of unresolved jets: the 2013 outburst of XTE J1908+094

(2015)

Authors:

PA Curran, JCA Miller-Jones, AP Rushton, DD Pawar, GE Anderson, D Altamirano, HA Krimm, JW Broderick, TM Belloni, RP Fender, EG Kording, D Maitra, S Markoff, S Migliari, C Rumsey, MP Rupen, DM Russell, TD Russell, CL Sarazin, GR Sivakoff, R Soria, AJ Tetarenko, D Titterington, V Tudose
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Molecular and atomic gas in dust lane early-type galaxies – I. Low star formation efficiencies in minor merger remnants

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 449:4 (2015) 3503-3516

Authors:

Timothy A Davis, Kate Rowlands, James R Allison, Stanislav S Shabala, Yuan-Sen Ting, Claudia del P. Lagos, Sugata Kaviraj, Nathan Bourne, Loretta Dunne, Steve Eales, Rob J Ivison, Steve Maddox, Daniel JB Smith, Matthew WL Smith, Pasquale Temi
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The LOFAR Transients Pipeline

Astronomy and Computing Elsevier 11 (2015) 25-48

Authors:

John D Swinbank, Tim D Staley, Gijs J Molenaar, Evert Rol, Antonia Rowlinson, Bart Scheers, Hanno Spreeuw, Martin E Bell, Jess W Broderick, Dario Carbone, Hugh Garsden, Alexander J van der Horst, Casey J Law, Michael Wise, Rene P Breton, Yvette Cendes, Stéphane Corbel, Jochen Eislöffel, Heino Falcke, Rob Fender, Jean-Mathias Grießmeier, Jason WT Hessels, Benjamin W Stappers, Adam J Stewart, Ralph AMJ Wijers, Rudy Wijnands, Philippe Zarka
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Cosmology from a SKA HI intensity mapping survey

Sissa Medialab Srl (2015) 019

Authors:

Mario Santos, Phil Bull, David Alonso, Stefano Camera, Pedro Ferreira, Gianni Bernardi, Roy Maartens, Matteo Viel, Francisco Villaescusa-Navarro, Filipe Batoni Abdalla, Matt Jarvis, R Benton Metcalf, Alkistis Pourtsidou, Laura Wolz
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Cosmology with SKA radio continuum surveys

Proceedings of Science Sissa Medialab srl (2015)

Authors:

Matthew Jarvis, David Bacon, Chris Blake, Michael L Brown, Sam N Lindsay, Alvise Raccanelli, Mario Santos, Dominik Schwarz

Abstract:

Radio continuum surveys have, in the past, been of restricted use in cosmology. Most studies have concentrated on cross-correlations with the cosmic microwave background to detect the integrated Sachs-Wolfe effect, due to the large sky areas that can be surveyed. As we move into the SKA era, radio continuum surveys will have sufficient source density and sky area to play a major role in cosmology on the largest scales. In this chapter we summarise the experiments that can be carried out with the SKA as it is built up through the coming decade. We show that the SKA can play a unique role in constraining the non-Gaussianity parameter to \sigma(f_NL) ~ 1, and provide a unique handle on the systematics that inhibit weak lensing surveys. The SKA will also provide the necessary data to test the isotropy of the Universe at redshifts of order unity and thus evaluate the robustness of the cosmological principle.Thus, SKA continuum surveys will turn radio observations into a central probe of cosmological research in the coming decades.
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