GAMA/H-ATLAS: the ultraviolet spectral slope and obscuration in galaxies

\mnras 415 (2011) 1002-1012-1002-1012

Authors:

DB Wijesinghe, E da Cunha, AM Hopkins, L Dunne, R Sharp, M Gunawardhana, S Brough, EM Sadler, S Driver, I Baldry, S Bamford, J Liske, J Loveday, P Norberg, J Peacock, CC Popescu, R Tuffs, E Andrae, R Auld, M Baes, J Bland-Hawthorn, S Buttiglione, A Cava, E Cameron, CJ Conselice, A Cooray, S Croom, A Dariush, G Dezotti, S Dye, S Eales, C Frenk, J Fritz, D Hill, R Hopwood, E Ibar, R Ivison, M Jarvis, DH Jones, E van Kampen, L Kelvin, K Kuijken, SJ Maddox, B Madore, MJ Micha lowski, B Nichol, H Parkinson, E Pascale, KA Pimbblet, M Pohlen, M Prescott, G Rhodighiero, ASG Robotham, EE Rigby, M Seibert, S Sergeant, DJB Smith, P Temi, W Sutherland, E Taylor, D Thomas, P van der Werf

Herschel-ATLAS: first data release of the Science Demonstration Phase source catalogues

\mnras 415 (2011) 2336-2348-2336-2348

Authors:

EE Rigby, SJ Maddox, L Dunne, M Negrello, DJB Smith, J González-Nuevo, D Herranz, M López-Caniego, R Auld, S Buttiglione, M Baes, A Cava, A Cooray, DL Clements, A Dariush, G de Zotti, S Dye, S Eales, D Frayer, J Fritz, R Hopwood, E Ibar, RJ Ivison, M Jarvis, P Panuzzo, E Pascale, M Pohlen, G Rodighiero, S Serjeant, P Temi, MA Thompson

The unusual radio transient in M82: an SS 433 analogue?

(2011)

Authors:

Tana Joseph, Thomas Maccarone, Robert Fender

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

ArXiv 1107.2516 (2011)

Authors:

Alessio Magro, Aris Karastergiou, Stefano Salvini, Benjamin Mort, Fred Dulwich, Kristian Zarb Adami

Abstract:

The identification, and subsequent discovery, of fast radio transients through blind-search surveys requires a large amount of processing power, in worst cases scaling as $\mathcal{O}(N^3)$. For this reason, survey data are generally processed offline, using high-performance computing architectures or hardware-based designs. In recent years, graphics processing units 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.

Dust-correlated cm wavelength continuum emission from translucent clouds ζ Oph and LDN 1780

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 414:3 (2011) 2424-2435

Authors:

M Vidal, S Casassus, C Dickinson, AN Witt, P Castellanos, RD Davies, RJ Davis, G Cabrera, K Cleary, JR Allison, JR Bond, L Bronfman, R Bustos, ME Jones, R Paladini, TJ Pearson, ACS Readhead, R Reeves, JL Sievers, AC Taylor