Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS 
detected sources using submillimetre colours

Amblard, A.; Cooray, A.; Serra, P.; Temi, P.; Barton, E.; Negrello, M.; Auld, R.; Baes, M.; Baldry, I. K.; Bamford, S.; Blain, A.; Bock, J.; Bonfield, D.; Burgarella, D.; Buttiglione, S.; Cameron, E.; Cava, A.; Clements, D.; Croom, S.; Dariush, A.; de Zotti, G.; Driver, S.; Dunlop, J.; Dunne, L.; Dye, S.; Eales, S.; Frayer, D.; Fritz, J.; Gardner, J. P.; Gonzalez-Nuevo, J.; Herranz, D.; Hill, D.; Hopkins, A.; Hughes, D. H.; Ibar, E.; Ivison, R. J.; Jarvis, M.; Jones, D. H.; Kelvin, L.; Lagache, G.; Leeuw, L.; Liske, J.; Lopez-Caniego, M.; Loveday, J.; Maddox, S.; Michalowski, M.; Norberg, P.; Parkinson, H.; Peacock, J. A.; Pearson, C.; Pascale, E.; Pohlen, M.; Popescu, C.; Prescott, M.; Robotham, A.; Rigby, E.; Rodighiero, G.; Samui, S.; Sansom, A.; Scott, D.; Serjeant, S.; Sharp, R.; Sibthorpe, B.; Smith, D. J. B.; Thompson, M. A.; Tuffs, R.; Valtchanov, I.; Van Kampen, E.; van der Werf, P.; Verma, A.; Vieira, J.; Vlahakis, C.

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Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours

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Baldry, I. K.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Tuffs, R.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Amblard, A., Cooray, A., Serra, P., Temi, P., Barton, E., Negrello, M., et al. (2010). Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours. Astronomy & Astrophysics, 518: L9.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-70ED-9

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