Real-time, fast radio transient searches with GPU de-dispersion

Monthly Notices of the Royal Astronomical Society 417:4 (2011) 2642-2650

Authors:

A Magro, A Karastergiou, S Salvini, B Mort, F Dulwich, K Zarb Adami

Abstract:

The identification and subsequent discovery of fast radio transients using blind-search surveys require a large amount of processing power, in worst cases scaling as. For this reason, survey data are generally processed off-line, using high-performance computing architectures or hardware-based designs. In recent years, graphics processing units (GPUs) have been extensively used for numerical analysis and scientific simulations, especially after the introduction of new high-level application programming interfaces. Here, we show how GPUs can be used for fast transient discovery in real time. We present a solution to the problem of de-dispersion, providing performance comparisons with a typical computing machine and traditional pulsar processing software. We describe the architecture of a real-time, GPU-based transient search machine. In terms of performance, our GPU solution provides a speed-up factor of between 50 and 200, depending on the parameters of the search. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS.

Herschel-ATLAS Galaxy Counts and High-redshift Luminosity Functions: The Formation of Massive Early-type Galaxies

\apj 742 (2011) 24-24

Authors:

A Lapi, J González-Nuevo, L Fan, A Bressan, G De Zotti, L Danese, M Negrello, L Dunne, S Eales, S Maddox, R Auld, M Baes, DG Bonfield, S Buttiglione, A Cava, DL Clements, A Cooray, A Dariush, S Dye, J Fritz, D Herranz, R Hopwood, E Ibar, R Ivison, MJ Jarvis, S Kaviraj, M López-Caniego, M Massardi, MJ Micha lowski, E Pascale, M Pohlen, E Rigby, G Rodighiero, S Serjeant, DJB Smith, P Temi, J Wardlow, P van der Werf

The environment and characteristics of low-redshift galaxies detected by the Herschel-ATLAS

\mnras 418 (2011) 64-73-64-73

Authors:

A Dariush, L Cortese, S Eales, E Pascale, MWL Smith, L Dunne, S Dye, D Scott, R Auld, M Baes, J Bland-Hawthorn, S Buttiglione, A Cava, DL Clements, A Cooray, G Dezotti, S Driver, J Fritz, HL Gomez, A Hopkins, R Hopwood, RJ Ivison, MJ Jarvis, DH Jones, L Kelvin, HG Khosroshahi, J Liske, J Loveday, S Maddox, BF Madore, MJ Micha lowski, P Norberg, S Phillipps, M Pohlen, CC Popescu, M Prescott, E Rigby, A Robotham, G Rodighiero, M Seibert, DJB Smith, P Temi, RJ Tuffs, PP van der Werf

A weak compact jet in a soft state of Cygnus X-1

(2011)

Authors:

A Rushton, JCA Miller-Jones, R Campana, Y Evangelista, Z Paragi, TJ Maccarone, GG Pooley, V Tudose, RP Fender, RE Spencer, V Dhawan

Goonhilly Sparklers

ArXiv 1110.4044 (2011)

Authors:

Aris Karastergiou, Mark Walker

Abstract:

Flux monitoring of compact radio quasars has revealed dramatic radio-wave lensing events which challenge our understanding of the interstellar medium. However, the data on these events remain very sparse. Here we consider how the Goonhilly radio astronomical facility can make an impact on this problem by dedicating one or more dishes to flux monitoring for a period of one year. Such an experiment would be able to identify \sim6 new events and study them in detail.