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  • The SCUBA HAlf Degree Extragalactic Survey (SHADES) - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies 

    Ivison, R. J.; Greve, T. R.; Dunlop, J. S.; Peacock, J. A.; Egami, E.; Smail, Ian; Ibar, E.; van Kampen, E.; Aretxaga, I.; Babbedge, T.; Biggs, A. D.; Blain, A. W.; Chapman, S. C.; Clements, D. L.; Coppin, K.; Farrah, D.; Halpern, M.; Hughes, D. H.; Jarvis, M. J.; Jenness, T.; Jones, J. R.; Mortier, A. M. J.; Oliver, S.; Papovich, C.; Perez-Gonzalez, P. G.; Pope, A.; Rawlings, S.; Rieke, G. H.; Rowan-Robinson, M.; Savage, R. S.; Scott, D.; Seigar, M.; Serjeant, S.; Simpson, C.; Stevens, J. A.; Vaccari, M.; Wagg, J.; Willott, C. J. (2007-07-27)
    Determining an accurate position for a submm galaxy (SMG) is the crucial step that enables us to move from the basic properties of an SMG sample - source counts and 2-D clustering - to an assessment of their detailed, ...