Herschel-ATLAS : extragalactic number counts from 250 to 500 microns Journal Item

@inproceedings{Clements2010HerschelATLASE,
  title={Herschel-ATLAS : extragalactic number counts from 250 to 500 microns Journal Item},
  author={D. L. Clements and Elyse Rigby and Steve J. Maddox and Loretta Dunne and Augustin Mortier and Christine Pearson and Alexandre Amblard and Robbie Auld and Maarten Baes and David G. Bonfield and Denis Burgarella and Sara Buttiglione and Antonio La Cava and Asantha Cooray and Ali A. Dariush and G. de Zotti and Simon Dye and Stephen A. Eales and D. Frayer and Jacopo Fritz and Jonathan P. A. Gardner and Joaqu{\'i}n Gonz{\'a}lez-Nuevo and Diego Herranz and Eduardo Ibar and R J Ivison and Matt J. Jarvis and Guilaine Lagache and Lerothodi L. Leeuw and Marcos L{\'o}pez-Caniego and Mattia Negrello and Enzo Pascale and Michael Pohlen and Giulia Rodighiero and S. Samui and Stephen Serjeant and Bruce Sibthorpe and Douglas Scott and Daniel J. B. Smith and Pasquale Temi and Mark A. Thompson and Ivan Valtchanov and Paul P. van der Werf and Aprajita Verma},
  year={2010}
}
Aims. The Herschel-ATLAS survey (H-ATLAS) will be the largest area survey to be undertaken by the Herschel Space Observatory. It will cover 550 sq. deg. of extragalactic sky at wavelengths of 100, 160, 250, 350 and 500 μm when completed, reaching flux limits (5σ) from 32 to 145 mJy. We here present galaxy number counts obtained for SPIRE observations of the first ∼14 sq. deg. observed at 250, 350 and 500 μm. Methods. Number counts are a fundamental tool in constraining models of galaxy… CONTINUE READING

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