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

S. Dye; L. Dunne; S. Eales; Daniel Smith; A. Amblard; R. Auld; M. Baes; I.K. Baldry; S. Bamford; A.W. Blain; D. Bonfield; M. Bremer; D. Burgarella; S. Buttiglione; E. Cameron; A. Cava; D. Clements; A. Cooray; S. Croom; A. Dariush; G. de Zotti; S. Driver; J.S. Dunlop; D. Frayer; J. Fritz; J.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. Michalowski; 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.G. Sharp; B. Sibthorpe; P. Temi; M.A. Thompson; R. Tuffs; I. Valtchanov; P. van der Werf; E. van Kampen; A. Verma

doi:10.1051/0004-6361/201014614

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

S. Dye
, L. Dunne
, S. Eales
, Daniel Smith
, A. Amblard
, R. Auld
, M. Baes
, I.K. Baldry
, S. Bamford
, A.W. Blain
, D. Bonfield
, M. Bremer
, D. Burgarella
, S. Buttiglione
, E. Cameron
, A. Cava
, D. Clements
, A. Cooray
, S. Croom
, A. Dariush

G. de Zotti, S. Driver, J.S. Dunlop, D. Frayer, J. Fritz, J.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. Michalowski, 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.G. Sharp, B. Sibthorpe, P. Temi, M.A. Thompson, R. Tuffs, I. Valtchanov, P. van der Werf, E. van Kampen, A. Verma

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Abstract

We have determined the luminosity function of 250 μm-selected galaxies detected in the ~14 deg2 science demonstration region of the Herschel-ATLAS project out to a redshift of z = 0.5. Our findings very clearly show that the luminosity function evolves steadily out to this redshift. By selecting a sub-group of sources within a fixed luminosity interval where incompleteness effects are minimal, we have measured a smooth increase in the comoving 250 μm luminosity density out to z = 0.2 where it is 3.6+1.4-0.9 times higher than the local value.

Original language	English
Article number	L10
Journal	Astronomy & Astrophysics
Volume	518
DOIs	https://doi.org/10.1051/0004-6361/201014614
Publication status	Published - 2010

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Dye, S., Dunne, L., Eales, S., Smith, D., Amblard, A., Auld, R., Baes, M., Baldry, I. K., Bamford, S., Blain, A. W., Bonfield, D., Bremer, M., Burgarella, D., Buttiglione, S., Cameron, E., Cava, A., Clements, D., Cooray, A., Croom, S., ... Verma, A. (2010). Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5. Astronomy & Astrophysics, 518, Article L10. https://doi.org/10.1051/0004-6361/201014614

@article{1acfad5b0c254a31baf4f413475e59c3,

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

abstract = "We have determined the luminosity function of 250 μm-selected galaxies detected in the \textasciitilde{}14 deg2 science demonstration region of the Herschel-ATLAS project out to a redshift of z = 0.5. Our findings very clearly show that the luminosity function evolves steadily out to this redshift. By selecting a sub-group of sources within a fixed luminosity interval where incompleteness effects are minimal, we have measured a smooth increase in the comoving 250 μm luminosity density out to z = 0.2 where it is 3.6+1.4-0.9 times higher than the local value.",

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

note = "Original article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory",

year = "2010",

doi = "10.1051/0004-6361/201014614",

language = "English",

volume = "518",

journal = "Astronomy \& Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Dye, S, Dunne, L, Eales, S, Smith, D, Amblard, A, Auld, R, Baes, M, Baldry, IK, Bamford, S, Blain, AW, Bonfield, D, Bremer, M, Burgarella, D, Buttiglione, S, Cameron, E, Cava, A, Clements, D, Cooray, A, Croom, S, Dariush, A, de Zotti, G, Driver, S, Dunlop, JS, Frayer, D, Fritz, J, Gardner, JP, Gomez, HL, Gonzalez-Nuevo, J, Herranz, D, Hill, D, Hopkins, A, Ibar, E, Ivison, RJ, Jarvis, MJ, Jones, DH, Kelvin, L, Lagache, G, Leeuw, L, Liske, J, Lopez-Caniego, M, Loveday, J, Maddox, S, Michalowski, M, Negrello, M, Norberg, P, Page, MJ, Parkinson, H, Pascale, E, Peacock, JA, Pohlen, M, Popescu, C, Prescott, M, Rigopoulou, D, Robotham, A, Rigby, E, Rodighiero, G, Samui, S, Scott, D, Serjeant, S, Sharp, RG, Sibthorpe, B, Temi, P, Thompson, MA, Tuffs, R, Valtchanov, I, van der Werf, P, van Kampen, E & Verma, A 2010, 'Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5', Astronomy & Astrophysics, vol. 518, L10. https://doi.org/10.1051/0004-6361/201014614

TY - JOUR

T1 - Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5

AU - Dye, S.

AU - Dunne, L.

AU - Eales, S.

AU - Smith, Daniel

AU - Amblard, A.

AU - Auld, R.

AU - Baes, M.

AU - Baldry, I.K.

AU - Bamford, S.

AU - Blain, A.W.

AU - Bonfield, D.

AU - Bremer, M.

AU - Burgarella, D.

AU - Buttiglione, S.

AU - Cameron, E.

AU - Cava, A.

AU - Clements, D.

AU - Cooray, A.

AU - Croom, S.

AU - Dariush, A.

AU - de Zotti, G.

AU - Driver, S.

AU - Dunlop, J.S.

AU - Frayer, D.

AU - Fritz, J.

AU - Gardner, J.P.

AU - Gomez, H.L.

AU - Gonzalez-Nuevo, J.

AU - Herranz, D.

AU - Hill, D.

AU - Hopkins, A.

AU - Ibar, E.

AU - Ivison, R.J.

AU - Jarvis, M.J.

AU - Jones, D.H.

AU - Kelvin, L.

AU - Lagache, G.

AU - Leeuw, L.

AU - Liske, J.

AU - Lopez-Caniego, M.

AU - Loveday, J.

AU - Maddox, S.

AU - Michalowski, M.

AU - Negrello, M.

AU - Norberg, P.

AU - Page, M.J.

AU - Parkinson, H.

AU - Pascale, E.

AU - Peacock, J.A.

AU - Pohlen, M.

AU - Popescu, C.

AU - Prescott, M.

AU - Rigopoulou, D.

AU - Robotham, A.

AU - Rigby, E.

AU - Rodighiero, G.

AU - Samui, S.

AU - Scott, D.

AU - Serjeant, S.

AU - Sharp, R.G.

AU - Sibthorpe, B.

AU - Temi, P.

AU - Thompson, M.A.

AU - Tuffs, R.

AU - Valtchanov, I.

AU - van der Werf, P.

AU - van Kampen, E.

AU - Verma, A.

N1 - Original article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory

PY - 2010

Y1 - 2010

N2 - We have determined the luminosity function of 250 μm-selected galaxies detected in the ~14 deg2 science demonstration region of the Herschel-ATLAS project out to a redshift of z = 0.5. Our findings very clearly show that the luminosity function evolves steadily out to this redshift. By selecting a sub-group of sources within a fixed luminosity interval where incompleteness effects are minimal, we have measured a smooth increase in the comoving 250 μm luminosity density out to z = 0.2 where it is 3.6+1.4-0.9 times higher than the local value.

AB - We have determined the luminosity function of 250 μm-selected galaxies detected in the ~14 deg2 science demonstration region of the Herschel-ATLAS project out to a redshift of z = 0.5. Our findings very clearly show that the luminosity function evolves steadily out to this redshift. By selecting a sub-group of sources within a fixed luminosity interval where incompleteness effects are minimal, we have measured a smooth increase in the comoving 250 μm luminosity density out to z = 0.2 where it is 3.6+1.4-0.9 times higher than the local value.

U2 - 10.1051/0004-6361/201014614

DO - 10.1051/0004-6361/201014614

M3 - Article

SN - 0004-6361

VL - 518

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - L10

ER -

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

Abstract

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