Herschel-ATLAS: Evolution of the 250 mu m 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. 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. 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

Herschel-ATLAS: Evolution of the 250 mu m 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. DariushG. 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. 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. Sharp, B. Sibthorpe, P. Temi, M. A. Thompson, R. Tuffs, I. Valtchanov, P. P. van der Werf, E. van Kampen, A. Verma

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

We have determined the luminosity function of 250 mu m-selected galaxies detected in the similar to 14 deg(2) 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 mu m luminosity density out to z = 0.2 where it is 3.6(-0.9)(+1.4) times higher than the local value.

Original language	English
Article number	L10
Pages (from-to)	-
Number of pages	5
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. J. B., Amblard, A., Auld, R., Baes, M., Baldry, I. K., Bamford, S., Blain, A. W., Bonfield, D. G., Bremer, M., Burgarella, D., Buttiglione, S., Cameron, E., Cava, A., Clements, D. L., Cooray, A., Croom, S., ... Verma, A. (2010). Herschel-ATLAS: Evolution of the 250 mu m luminosity function out to z = 0.5. Astronomy & Astrophysics, 518, -. Article L10. https://doi.org/10.1051/0004-6361/201014614

@article{1e4eb0514da24b2a8cc10d97fa0b2933,

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

abstract = "We have determined the luminosity function of 250 mu m-selected galaxies detected in the similar to 14 deg(2) 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 mu m luminosity density out to z = 0.2 where it is 3.6(-0.9)(+1.4) times higher than the local value.",

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

year = "2010",

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

language = "English",

volume = "518",

pages = "--",

journal = "Astronomy \& Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Dye, S, Dunne, L, Eales, S, Smith, DJB, Amblard, A, Auld, R, Baes, M, Baldry, IK, Bamford, S, Blain, AW, Bonfield, DG, Bremer, M, Burgarella, D, Buttiglione, S, Cameron, E, Cava, A, Clements, DL, 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, MJ, 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, R, Sibthorpe, B, Temi, P, Thompson, MA, Tuffs, R, Valtchanov, I, van der Werf, PP, van Kampen, E & Verma, A 2010, 'Herschel-ATLAS: Evolution of the 250 mu m luminosity function out to z = 0.5', Astronomy & Astrophysics, vol. 518, L10, pp. -. https://doi.org/10.1051/0004-6361/201014614

TY - JOUR

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

AU - Dye, S.

AU - Dunne, L.

AU - Eales, S.

AU - Smith, D. J. B.

AU - Amblard, A.

AU - Auld, R.

AU - Baes, M.

AU - Baldry, I. K.

AU - Bamford, S.

AU - Blain, A. W.

AU - Bonfield, D. G.

AU - Bremer, M.

AU - Burgarella, D.

AU - Buttiglione, S.

AU - Cameron, E.

AU - Cava, A.

AU - Clements, D. L.

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, Jonathan 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. J.

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.

AU - Sibthorpe, B.

AU - Temi, P.

AU - Thompson, M. A.

AU - Tuffs, R.

AU - Valtchanov, I.

AU - van der Werf, P. P.

AU - van Kampen, E.

AU - Verma, A.

PY - 2010

Y1 - 2010

N2 - We have determined the luminosity function of 250 mu m-selected galaxies detected in the similar to 14 deg(2) 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 mu m luminosity density out to z = 0.2 where it is 3.6(-0.9)(+1.4) times higher than the local value.

AB - We have determined the luminosity function of 250 mu m-selected galaxies detected in the similar to 14 deg(2) 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 mu m luminosity density out to z = 0.2 where it is 3.6(-0.9)(+1.4) times higher than the local value.

UR - https://www.scopus.com/pages/publications/77954767657

U2 - 10.1051/0004-6361/201014614

DO - 10.1051/0004-6361/201014614

M3 - Article

SN - 0004-6361

VL - 518

SP - -

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - L10

ER -

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

Abstract

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