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

S Dye; L Dunne; S Eales; D Smith; A Amblard; R Auld; M Baes; Ivan Baldry; Steven Bamford; A Blain; D Bonfield; M Bremer; D Burgarella; S Buttiglione; Ewan Cameron; A Cava; D Clements; Asantha Cooray; Scott Croom; A Dariush; G De Zotti; Simon Driver; James Dunlop; D Frayer; J Fritz; Jonathon P Gardner; H Gomez; J Gonzalez-Nuevo; D Herranz; D Hill; Andrew Hopkins; E Ibar; R Ivison; M Jarvis; David Jones; L Kelvin; G Lagache; L Leeuw; J Liske; M Lopez-Caniego; J Loveday; S Maddox; M Michalowski; M Negrello; Peder Norberg; M Page; H Parkinson; E Pascale; John Peacock; M Pohlen; Cristina Popescu; Matthew Prescott; D Rigopoulou; A Robotham; E Rigby; G Rodighiero; S Samui; Douglas Scott; S Serjeant; Robert Sharp; B Sibthorpe; P Temi; M 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 microm luminosity function out to z = 0.5

S Dye, L Dunne, S Eales, D Smith, A Amblard, R Auld, M Baes, Ivan Baldry, Steven Bamford, A Blain, D Bonfield, M Bremer, D Burgarella, S Buttiglione, Ewan Cameron, A Cava, D Clements, Asantha Cooray, Scott Croom, A DariushG De Zotti, Simon Driver, James Dunlop, D Frayer, J Fritz, Jonathon P Gardner, H Gomez, J Gonzalez-Nuevo, D Herranz, D Hill, Andrew Hopkins, E Ibar, R Ivison, M Jarvis, David Jones, L Kelvin, G Lagache, L Leeuw, J Liske, M Lopez-Caniego, J Loveday, S Maddox, M Michalowski, M Negrello, Peder Norberg, M Page, H Parkinson, E Pascale, John Peacock, M Pohlen, Cristina Popescu, Matthew Prescott, D Rigopoulou, A Robotham, E Rigby, G Rodighiero, S Samui, Douglas Scott, S Serjeant, Robert Sharp, B Sibthorpe, P Temi, M Thompson, R Tuffs, I Valtchanov, P van der Werf, E van Kampen, A Verma

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

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Abstract

We have determined the luminosity function of 250 I?m-selected galaxies detected in the a??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 I?m 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
Pages (from-to)	1 - 5
Number of pages	5
Journal	Astronomy & Astrophysics
Volume	518
Issue number	1
DOIs	https://doi.org/10.1051/0004-6361/201014614
Publication status	Published - 2010
Externally published	Yes

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Dye, S., Dunne, L., Eales, S., Smith, D., Amblard, A., Auld, R., Baes, M., Baldry, I., Bamford, S., Blain, A., 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 microm luminosity function out to z = 0.5. Astronomy & Astrophysics, 518(1), 1 - 5. https://doi.org/10.1051/0004-6361/201014614

@article{57051151dc454edab3faaa191c872446,

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

abstract = "We have determined the luminosity function of 250 I?m-selected galaxies detected in the a??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 I?m 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 D Smith and A Amblard and R Auld and M Baes and Ivan Baldry and Steven Bamford and A Blain and D Bonfield and M Bremer and D Burgarella and S Buttiglione and Ewan Cameron and A Cava and D Clements and Asantha Cooray and Scott Croom and A Dariush and {De Zotti}, G and Simon Driver and James Dunlop and D Frayer and J Fritz and Gardner, {Jonathon P} and H Gomez and J Gonzalez-Nuevo and D Herranz and D Hill and Andrew Hopkins and E Ibar and R Ivison and M Jarvis and David 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 Peder Norberg and M Page and H Parkinson and E Pascale and John Peacock and M Pohlen and Cristina Popescu and Matthew Prescott and D Rigopoulou and A Robotham and E Rigby and G Rodighiero and S Samui and Douglas Scott and S Serjeant and Robert Sharp and B Sibthorpe and P Temi and M Thompson and R Tuffs and I Valtchanov and {van der Werf}, P and {van Kampen}, E and A Verma",

year = "2010",

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

language = "English",

volume = "518",

pages = "1 -- 5",

journal = "Astronomy & Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

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Dye, S, Dunne, L, Eales, S, Smith, D, Amblard, A, Auld, R, Baes, M, Baldry, I, Bamford, S, Blain, A, 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, J, Frayer, D, Fritz, J, Gardner, JP, Gomez, H, Gonzalez-Nuevo, J, Herranz, D, Hill, D, Hopkins, A, Ibar, E, Ivison, R, Jarvis, M, Jones, D, Kelvin, L, Lagache, G, Leeuw, L, Liske, J, Lopez-Caniego, M, Loveday, J, Maddox, S, Michalowski, M, Negrello, M, Norberg, P, Page, M, Parkinson, H, Pascale, E, Peacock, J, 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, M, Tuffs, R, Valtchanov, I, van der Werf, P, van Kampen, E & Verma, A 2010, 'Herschel-ATLAS: Evolution of the 250 microm luminosity function out to z = 0.5', Astronomy & Astrophysics, vol. 518, no. 1, pp. 1 - 5. https://doi.org/10.1051/0004-6361/201014614

TY - JOUR

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

AU - Dye, S

AU - Dunne, L

AU - Eales, S

AU - Smith, D

AU - Amblard, A

AU - Auld, R

AU - Baes, M

AU - Baldry, Ivan

AU - Bamford, Steven

AU - Blain, A

AU - Bonfield, D

AU - Bremer, M

AU - Burgarella, D

AU - Buttiglione, S

AU - Cameron, Ewan

AU - Cava, A

AU - Clements, D

AU - Cooray, Asantha

AU - Croom, Scott

AU - Dariush, A

AU - De Zotti, G

AU - Driver, Simon

AU - Dunlop, James

AU - Frayer, D

AU - Fritz, J

AU - Gardner, Jonathon P

AU - Gomez, H

AU - Gonzalez-Nuevo, J

AU - Herranz, D

AU - Hill, D

AU - Hopkins, Andrew

AU - Ibar, E

AU - Ivison, R

AU - Jarvis, M

AU - Jones, David

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, Peder

AU - Page, M

AU - Parkinson, H

AU - Pascale, E

AU - Peacock, John

AU - Pohlen, M

AU - Popescu, Cristina

AU - Prescott, Matthew

AU - Rigopoulou, D

AU - Robotham, A

AU - Rigby, E

AU - Rodighiero, G

AU - Samui, S

AU - Scott, Douglas

AU - Serjeant, S

AU - Sharp, Robert

AU - Sibthorpe, B

AU - Temi, P

AU - Thompson, M

AU - Tuffs, R

AU - Valtchanov, I

AU - van der Werf, P

AU - van Kampen, E

AU - Verma, A

PY - 2010

Y1 - 2010

N2 - We have determined the luminosity function of 250 I?m-selected galaxies detected in the a??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 I?m 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 I?m-selected galaxies detected in the a??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 I?m luminosity density out to z = 0.2 where it is 3.6 +1.4-0.9 times higher than the local value

UR - http://arxiv.org/abs/1005.2411

U2 - 10.1051/0004-6361/201014614

DO - 10.1051/0004-6361/201014614

M3 - Article

SN - 0004-6361

VL - 518

SP - 1

EP - 5

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

IS - 1

ER -

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

Abstract

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