Herschel-ATLAS: Evolution of the 250 μm luminosity function out to z =  0.5

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

doi:10.1051/0004-6361/201014614

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Volume 518 (July-August 2010)

A&A, 518 (2010) L10

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Herschel: the first science highlights

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Fig. 4

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Evolution of comoving rest-frame 250 μm luminosity density out to z ≃ 0.2 for sources with luminosity in the range 10⁹ < L₂₅₀/L_⊙ < 5 × 10⁹. Errors were determined using a Monte Carlo simulation which randomised redshifts and photometry and account for Poisson noise. The line is the fit (1 + z)^7.1.

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