Now showing items 1-4 of 4

    • Colour matters : the effects of lensing on the positional offsets between optical and submillimetre galaxies in Herschel-ATLAS 

      Bourne, N.; Maddox, S.J.; Dunne, L.; Dye, S.; Eales, S.; Hoyos, C.; González-Nuevo, J.; Smith, Daniel; Valiante, E.; de Zotti, G.; Ivison, Rob J.; Rowlands, K. (2014-10-21)
      We report an unexpected variation in the positional offset distributions between Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) submillimetre (submm) sources and their optical associations, depending on both ...
    • Far-infrared observations of an unbiased sample of gamma-ray burst host galaxies 

      Kohn, S.A.; Michalowski, M. J.; Bourne, N.; Baes, M.; Fritz, J.; Cooray, A.; De Looze, I.; De Zotti, G.; Dannerbauer, H.; Dunne, L.; Dye, S.; Eales, S.; Furlanetto, C.; Gonzalez-Nuevo, J.; Ibar, E.; Ivison, Rob J.; Maddox, S.J.; Scott, D.; Smith, Daniel; Smith, M.W.L.; Symeonidis, M.; Valiante, E. (2015-04-01)
      Gamma-ray bursts (GRBs) are the most energetic phenomena in the Universe; believed to result from the collapse and subsequent explosion of massive stars. Even though it has profound consequences for our understanding of ...
    • Herschel-ATLAS : Multi-wavelength SEDs and physical properties of 250 μm selected galaxies at z <0.5 

      Smith, Daniel; Dunne, L.; Rowlands, K.; Maddox, S.J.; Bourne, N.; Dye, S.; Rigby, E.E.; Bonfield, D.G.; Jarvis, M.J.; da Cunha, E.; Eales, S.; Gomez, H.L.; Auld, R.; Dariush, A.; Pohlen, M.; Charlot, S.; Driver, S.P.; Kelvin, L.; Robotham, A.; Popescu, C.C.; Tuffs, R.J.; Andrae, E.; Dunlop, J.S.; Ivison, R.J.; Seymour, N.; Symeonidis, M.; Baes, M.; Fritz, J.; Clements, D.L.; Cooray, A.; De Zotti, G.; Buttiglione, S.; Scott, D.; Verma, A.; van der Werf, P.; Cava, A.; Hopwood, R.; Ibar, E.; Madore, B.F.; Seibert, M.; Temi, P. (2012-11-21)
      We present a pan-chromatic analysis of an unprecedented sample of 1402 250 μm selected galaxies at z < 0.5 (z-=0.24) from the Herschel-ATLAS survey. We complement our Herschel 100-500μm data with UV-K-band photometry from ...
    • Isothermal dust models of Herschel-ATLAS galaxies 

      Smith, Daniel; Hardcastle, M.J.; Jarvis, M.J.; Maddox, S.J.; Dunne, L.; Bonfield, D.G.; Eales, S.; Serjeant, S.; Thompson, M.A.; Baes, M.; Clements, D. L.; Cooray, A.; de Zotti, G.; Gonzalez-Nuevo, J.; van der Werf, P.; Virdee, J.; Bourne, N.; Dariush, A.; Hopwood, R.; Ibar, E.; Valiante, E. (2013-12)
      We use galaxies from the Herschel-ATLAS (H-ATLAS) survey, and a suite of ancillary simulations based on an isothermal dust model, to study our ability to determine the effective dust temperature, luminosity and emissivity ...