Hintze Centre for Astrophysical Surveys

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Herschel-ATLAS: rapid evolution of dust in galaxies over the last 5 billion years

\mnras 417 (2011) 1510-1533-1510-1533

Authors:

L Dunne, HL Gomez, E da Cunha, S Charlot, S Dye, S Eales, SJ Maddox, K Rowlands, DJB Smith, R Auld, M Baes, DG Bonfield, N Bourne, S Buttiglione, A Cava, DL Clements, KEK Coppin, A Cooray, A Dariush, G de Zotti, S Driver, J Fritz, J Geach, R Hopwood, E Ibar, RJ Ivison, MJ Jarvis, L Kelvin, E Pascale, M Pohlen, C Popescu, EE Rigby, A Robotham, G Rodighiero, AE Sansom, S Serjeant, P Temi, M Thompson, R Tuffs, P van der Werf, C Vlahakis
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New views of old galaxies

Astronomy & Geophysics Oxford University Press (OUP) 52:5 (2011) 5.18-5.24
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The VLT-FLAMES survey of massive stars: Nitrogen abundances for Be-type stars in the Magellanic Clouds

(2011)

Authors:

PR Dunstall, I Brott, PL Dufton, DJ Lennon, CJ Evans, SJ Smartt, I Hunter
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On the association of ULXs with young superclusters: M82 X-1 and a new candidate in NGC 7479

(2011)

Authors:

R Voss, MTB Nielsen, G Nelemans, M Fraser, SJ Smartt
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FRATs: A search for Fast Radio Transients with LOFAR

AIP Conference Proceedings 1357 (2011) 331-334

Authors:

S Ter Veen, H Falcke, R Fender, JR Hörandel, CW James, S Rawlings, P Schellart, B Stappers, R Wijers, M Wise, P Zarka

Abstract:

The FRATs project aims to detect single dispersed pulses from Fast Radio Transients with LOFAR in real-time. These pulses can originate from pulsars, RRATS and other classes of known or unknown objects. To detect these pulses a detection algorithm is being run on an incoherent beam from the different LOFAR stations. This incoherent beam has a wide field of view and can be formed parallel to other observations, such that both can run at the same time. A precise localisation is done by storing the data from each dipole. This gives an all-sky coverage with a spatial resolution of order arc seconds. The source is identified by making high time-resolution images. This is explained in more detail with preliminary results illustrating the methods. © 2011 American Institute of Physics.
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