The Herschel ATLAS
S. Eales, L. Dunne, D. Clements, A. Cooray, G. De Zotti, S. Dye, R., Ivison, M. Jarvis, G. Lagache, S. Maddox, M. Negrello, S. Serjeant, M.A., Thompson, E. Van Kampen, A. Amblard, P. Andreani, M. Baes, A. Beelen, G.J., Bendo, D. Benford, F. Bertoldi, J. Bock, D. Bonfield
TL;DR
The Herschel ATLAS is a large-scale survey of 510 square degrees in the far-infrared and submillimetre, combining multi-wavelength data to study galaxy properties and evolution.
Contribution
This paper details the design, scope, and scientific goals of the Herschel ATLAS, including new models predicting source properties across wavebands.
Findings
Survey covers 510 sq. degrees, four times larger than previous Herschel surveys.
Predictions of galaxy source properties in multiple wavebands.
Description of six major science programs enabled by the survey.
Abstract
The Herschel ATLAS is the largest open-time key project that will be carried out on the Herschel Space Observatory. It will survey 510 square degrees of the extragalactic sky, four times larger than all the other Herschel surveys combined, in five far-infrared and submillimetre bands. We describe the survey, the complementary multi-wavelength datasets that will be combined with the Herschel data, and the six major science programmes we are undertaking. Using new models based on a previous submillimetre survey of galaxies, we present predictions of the properties of the ATLAS sources in other wavebands.
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