Now showing items 1-4 of 4

    • Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release 

      Driver, S. P.; Hill, D. T.; Kelvin, L. S.; Robotham, A. S. G.; Liske, J.; Norberg, P.; Baldry, I.K.; Bamford, S. P.; Hopkins, A. M.; Loveday, J.; Peacock, J.A.; Andrae, E.; Bland-Hawthorn, J.; Brough, S.; Brown, M. J. I.; Cameron, E.; Ching, J. H. Y.; Colless, M.; Conselice, C. J.; Croom, S. M.; Cross, N.J.G.; De Propris, R.; Dye, S.; Drinkwater, M. J.; Ellis, S.; Graham, Alister W.; Grootes, M. W.; Gunawardhana, M.; Jones, D. H.; van Kampen, E.; Maraston, C.; Nichol, R.C.; Parkinson, H. R.; Phillipps, S.; Pimbblet, K.; Popescu, C. C.; Prescott, M.; Roseboom, I.G.; Sadler, E.M.; Sansom, A. E.; Sharp, R.G.; Smith, Daniel; Taylor, E.; Thomas, D.; Tuffs, R. J.; Wijesinghe, D.; Dunne, L.; Frenk, C. S.; Jarvis, M.J.; Madore, B. F.; Meyer, M. J.; Seibert, M.; Staveley-Smith, L.; Sutherland, W. J.; Warren, S.J. (2011-05)
      The Galaxy and Mass Assembly (GAMA) survey has been operating since 2008 February on the 3.9-m Anglo-Australian Telescope using the AAOmega fibre-fed spectrograph facility to acquire spectra with a resolution of R approximate ...
    • Herschel-ATLAS : Counterparts from the ultraviolet-near-infrared in the science demonstration phase catalogue 

      Smith, Daniel; Dunne, L.; Maddox, S. J.; Eales, S.; Bonfield, D. G.; Jarvis, M.J.; Sutherland, W.; Fleuren, S.; Rigby, E. E.; Thompson, Mark; Baldry, I.K.; Bamford, S.; Buttiglione, S.; Cava, A.; Clements, D. L.; Cooray, A.; Croom, S.; Dariush, A.; de Zotti, G.; Driver, S. P.; Dunlop, J.S.; Fritz, J.; Hill, D. T.; Hopkins, A.; Hopwood, R.; Ibar, E.; Ivison, R.J.; Jones, D. H.; Kelvin, L.; Leeuw, L.; Liske, J.; Loveday, J.; Madore, B. F.; Norberg, P.; Panuzzo, P.; Pascale, E.; Pohlen, M.; Popescu, C. C.; Prescott, M.; Robotham, A.; Rodighiero, G.; Scott, D.; Seibert, M.; Sharp, R.; Temi, P.; Tuffs, R. J.; van der Werf, P.; van Kampen, E. (2011-09)
      We present a technique to identify optical counterparts of 250-mu m-selected sources from the Herschel-ATLAS survey. Of the 6621 250 mu m > 32-mJy sources in our science demonstration catalogue we find that similar to 60 ...
    • Herschel-ATLAS: far-infrared properties of radio-selected galaxies 

      Hardcastle, M.J.; Virdee, J.S.; Jarvis, M.J.; Bonfield, D.; Dunne, L.; Rawlings, S.; Stevens, J. A.; Christopher, N. M.; Heywood, I.; Mauch, Tom; Rigopoulou, D.; Verma, A.; Baldry, Ivan K.; Bamford, S. P.; Buttiglione, S.; Cava, A.; Clements, D. L.; Cooray, A.; Croom, S. M.; Dariush, A.; de Zotti, G.; Eales, S.; Fritz, J.; Hill, D. T.; Hughes, D.; Hopwood, R.; Ibar, E.; Ivison, Rob J.; Jones, D.H.; Loveday, J.; Maddox, S. J.; Michalowski, M. J.; Negrello, M.; Norberg, P.; Pohlen, M.; Prescott, M.; Rigby, E. E.; Robotham, A. S. G.; Rodighiero, G.; Scott, D.; Sharp, R.; Smith, Daniel; Temi, P.; van Kampen, E. (2010)
      We use the Herschel-Astrophysical Terahertz Large Area Survey (ATLAS) science demonstration data to investigate the star formation properties of radio-selected galaxies in the GAMA-9h field as a function of radio luminosity ...
    • Herschel-ATLAS: the far-infrared-radio correlation at z <0.5 

      Jarvis, M.J.; Smith, Daniel; Bonfield, David G.; Hardcastle, M.J.; Falder, J. T.; Stevens, Jason; Ivison, R.J.; Auld, R.; Baes, M.; Baldry, I.K.; Bamford, S. P.; Bourne, N.; Buttiglione, S.; Cava, A.; Cooray, A.; Dariush, A.; de Zotti, G.; Dunlop, J. S.; Dunne, L.; Dye, S.; Eales, S.; Fritz, J.; Hill, D. T.; Hopwood, R.; Hughes, D.H.; Ibar, E.; Jones, D. H.; Kelvin, L.; Lawrence, A.; Leeuw, L.; Loveday, J.; Maddox, S. J.; Michalowski, M. J.; Negrello, M.; Norberg, P.; Pohlen, M.; Prescott, M.; Rigby, E. E.; Robotham, A.; Rodighiero, G.; Scott, D.; Sharp, R.; Temi, P.; Thompson, Mark; van der Werf, P.; van Kampen, E.; Vlahakis, C.; White, G. (2010)
      We use data from the Herschel-ATLAS to investigate the evolution of the far-infrared–radio correlation over the redshift range 0 < z < 0.5. Using the total far-infrared luminosity of all >5σ sources in the Herschel-ATLAS ...