Browsing by Author "Smith, M.W.L."

Now showing items 1-2 of 2

    • 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: properties of dusty massive galaxies at low and high redshifts 

      Rowlands, K.; Dunne, L.; Dye, S.; Aragón-Salamanca, A.; Maddox, S.; da Cunha, E.; Smith, Daniel; Bourne, N.; Eales, S.; Gomez, H.L.; Smail, I.; Alpaslan, M.; Clark, C.J.R.; Driver, S.; Ibar, E.; Ivison, Rob J.; Robotham, A.; Smith, M.W.L.; Valiante, E. (2014-06-21)
      We present a comparison of the physical properties of a rest-frame 250-μm-selected sample of massive, dusty galaxies from 0 < z < 5.3. Our sample comprises 29 high-redshift submillimetre galaxies (SMGs) from the literature ...