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

57 Citations (Scopus)

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

Access to Document

10.1051/0004-6361/201014614

Cite this

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",

number = "1",

}

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

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 - 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

Access to Document

Other files and links

Cite this