First results from HerMES on the evolution of the submillimetre luminosity function

S. A. Eales; G. Raymond; I. G. Roseboom; B. Altieri; A. Amblard; V. Arumugam; R. Auld; H. Aussel; T. Babbedge; A. Blain; J. Bock; A. Boselli; D. Brisbin; V. Buat; D. Burgarella; N. Castro-Rodríguez; A. Cava; P. Chanial; D. L. Clements; A. Conley; L. Conversi; A. Cooray; C. D. Dowell; E. Dwek; S. Dye; D. Elbaz; D. Farrah; M. Fox; A. Franceschini; W. Gear; J. Glenn; E. A. González Solares; M. Griffin; M. Harwit; E. Hatziminaoglou; J. Huang; E. Ibar; K. Isaak; R. J. Ivison; G. Lagache; L. Levenson; C. J. Lonsdale; N. Lu; S. Madden; B. Maffei; G. Mainetti; L. Marchetti; G. E. Morrison; A. M J Mortier; H. T. Nguyen; B. O'Halloran; S. J. Oliver; A. Omont; F. N. Owen; M. J. Page; M. Pannella; P. Panuzzo; A. Papageorgiou; C. P. Pearson; I. Pérez-Fournon; M. Pohlen; J. I. Rawlings; D. Rigopoulou; D. Rizzo; M. Rowan-Robinson; M. Sánchez Portal; B. Schulz; D. Scott; N. Seymour; D. L. Shupe; A. J. Smith; J. A. Stevens; V. Strazzullo; M. Symeonidis; M. Trichas; K. E. Tugwell; M. Vaccari; I. Valtchanov; L. Vigroux; L. Wang; R. Ward; G. Wright; C. K. Xu; M. Zemcov

doi:10.1051/0004-6361/201014675

First results from HerMES on the evolution of the submillimetre luminosity function

S. A. Eales, G. Raymond, I. G. Roseboom, B. Altieri, A. Amblard, V. Arumugam, R. Auld, H. Aussel, T. Babbedge, A. Blain, J. Bock, A. Boselli, D. Brisbin, V. Buat, D. Burgarella, N. Castro-Rodríguez, A. Cava, P. Chanial, D. L. Clements, A. ConleyL. Conversi, A. Cooray, C. D. Dowell, E. Dwek, S. Dye, D. Elbaz, D. Farrah, M. Fox, A. Franceschini, W. Gear, J. Glenn, E. A. González Solares, M. Griffin, M. Harwit, E. Hatziminaoglou, J. Huang, E. Ibar, K. Isaak, R. J. Ivison, G. Lagache, L. Levenson, C. J. Lonsdale, N. Lu, S. Madden, B. Maffei, G. Mainetti, L. Marchetti, G. E. Morrison, A. M J Mortier, H. T. Nguyen, B. O'Halloran, S. J. Oliver, A. Omont, F. N. Owen, M. J. Page, M. Pannella, P. Panuzzo, A. Papageorgiou, C. P. Pearson, I. Pérez-Fournon, M. Pohlen, J. I. Rawlings, D. Rigopoulou, D. Rizzo, M. Rowan-Robinson, M. Sánchez Portal, B. Schulz, D. Scott, N. Seymour, D. L. Shupe, A. J. Smith, J. A. Stevens, V. Strazzullo, M. Symeonidis, M. Trichas, K. E. Tugwell, M. Vaccari, I. Valtchanov, L. Vigroux, L. Wang, R. Ward, G. Wright, C. K. Xu, M. Zemcov

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

Abstract

We have carried out two extremely deep surveys with SPIRE, one of the two cameras on Herschel, at 250 μm, close to the peak of the far-infrared background. We have used the results to investigate the evolution of the rest-frame 250-μm luminosity function out to z = 2. We find evidence for strong evolution out to z $\simeq$ 1 but evidence for at most weak evolution beyond this redshift. Our results suggest that a significant part of the stars and metals in the universe today were formed at z 1.4 in spiral galaxies. © 2010 ESO.

Original language	English
Journal	Astronomy and Astrophysics
Volume	518
Issue number	2
DOIs	https://doi.org/10.1051/0004-6361/201014675
Publication status	Published - 16 Jul 2010

Keywords

Galaxies: evoluton
Galaxies: formation
Galaxies: high-redshift
Submillimeter: galaxies

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10.1051/0004-6361/201014675

http://adsabs.harvard.edu/abs/2010A%26A...518L..23E

Cite this

Eales, S. A., Raymond, G., Roseboom, I. G., Altieri, B., Amblard, A., Arumugam, V., Auld, R., Aussel, H., Babbedge, T., Blain, A., Bock, J., Boselli, A., Brisbin, D., Buat, V., Burgarella, D., Castro-Rodríguez, N., Cava, A., Chanial, P., Clements, D. L., ... Zemcov, M. (2010). First results from HerMES on the evolution of the submillimetre luminosity function. Astronomy and Astrophysics, 518(2). https://doi.org/10.1051/0004-6361/201014675

@article{29a1f6a262f74d97b2b0ee59f10fb023,

title = "First results from HerMES on the evolution of the submillimetre luminosity function",

abstract = "We have carried out two extremely deep surveys with SPIRE, one of the two cameras on Herschel, at 250 μm, close to the peak of the far-infrared background. We have used the results to investigate the evolution of the rest-frame 250-μm luminosity function out to z = 2. We find evidence for strong evolution out to z $\simeq$ 1 but evidence for at most weak evolution beyond this redshift. Our results suggest that a significant part of the stars and metals in the universe today were formed at z 1.4 in spiral galaxies. {\textcopyright} 2010 ESO.",

keywords = "Galaxies: evoluton, Galaxies: formation, Galaxies: high-redshift, Submillimeter: galaxies",

author = "Eales, {S. A.} and G. Raymond and Roseboom, {I. G.} and B. Altieri and A. Amblard and V. Arumugam and R. Auld and H. Aussel and T. Babbedge and A. Blain and J. Bock and A. Boselli and D. Brisbin and V. Buat and D. Burgarella and N. Castro-Rodr{\'i}guez and A. Cava and P. Chanial and Clements, {D. L.} and A. Conley and L. Conversi and A. Cooray and Dowell, {C. D.} and E. Dwek and S. Dye and D. Elbaz and D. Farrah and M. Fox and A. Franceschini and W. Gear and J. Glenn and {Gonz{\'a}lez Solares}, {E. A.} and M. Griffin and M. Harwit and E. Hatziminaoglou and J. Huang and E. Ibar and K. Isaak and Ivison, {R. J.} and G. Lagache and L. Levenson and Lonsdale, {C. J.} and N. Lu and S. Madden and B. Maffei and G. Mainetti and L. Marchetti and Morrison, {G. E.} and Mortier, {A. M J} and Nguyen, {H. T.} and B. O'Halloran and Oliver, {S. J.} and A. Omont and Owen, {F. N.} and Page, {M. J.} and M. Pannella and P. Panuzzo and A. Papageorgiou and Pearson, {C. P.} and I. P{\'e}rez-Fournon and M. Pohlen and Rawlings, {J. I.} and D. Rigopoulou and D. Rizzo and M. Rowan-Robinson and {S{\'a}nchez Portal}, M. and B. Schulz and D. Scott and N. Seymour and Shupe, {D. L.} and Smith, {A. J.} and Stevens, {J. A.} and V. Strazzullo and M. Symeonidis and M. Trichas and Tugwell, {K. E.} and M. Vaccari and I. Valtchanov and L. Vigroux and L. Wang and R. Ward and G. Wright and Xu, {C. K.} and M. Zemcov",

note = "DOI: 10.1051/0004-6361/201014675; eprintid: arXiv:1005.2189",

year = "2010",

month = jul,

day = "16",

doi = "10.1051/0004-6361/201014675",

language = "English",

volume = "518",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

number = "2",

}

Eales, SA, Raymond, G, Roseboom, IG, Altieri, B, Amblard, A, Arumugam, V, Auld, R, Aussel, H, Babbedge, T, Blain, A, Bock, J, Boselli, A, Brisbin, D, Buat, V, Burgarella, D, Castro-Rodríguez, N, Cava, A, Chanial, P, Clements, DL, Conley, A, Conversi, L, Cooray, A, Dowell, CD, Dwek, E, Dye, S, Elbaz, D, Farrah, D, Fox, M, Franceschini, A, Gear, W, Glenn, J, González Solares, EA, Griffin, M, Harwit, M, Hatziminaoglou, E, Huang, J, Ibar, E, Isaak, K, Ivison, RJ, Lagache, G, Levenson, L, Lonsdale, CJ, Lu, N, Madden, S, Maffei, B, Mainetti, G, Marchetti, L, Morrison, GE, Mortier, AMJ, Nguyen, HT, O'Halloran, B, Oliver, SJ, Omont, A, Owen, FN, Page, MJ, Pannella, M, Panuzzo, P, Papageorgiou, A, Pearson, CP, Pérez-Fournon, I, Pohlen, M, Rawlings, JI, Rigopoulou, D, Rizzo, D, Rowan-Robinson, M, Sánchez Portal, M, Schulz, B, Scott, D, Seymour, N, Shupe, DL, Smith, AJ, Stevens, JA, Strazzullo, V, Symeonidis, M, Trichas, M, Tugwell, KE, Vaccari, M, Valtchanov, I, Vigroux, L, Wang, L, Ward, R, Wright, G, Xu, CK & Zemcov, M 2010, 'First results from HerMES on the evolution of the submillimetre luminosity function', Astronomy and Astrophysics, vol. 518, no. 2. https://doi.org/10.1051/0004-6361/201014675

TY - JOUR

T1 - First results from HerMES on the evolution of the submillimetre luminosity function

AU - Eales, S. A.

AU - Raymond, G.

AU - Roseboom, I. G.

AU - Altieri, B.

AU - Amblard, A.

AU - Arumugam, V.

AU - Auld, R.

AU - Aussel, H.

AU - Babbedge, T.

AU - Blain, A.

AU - Bock, J.

AU - Boselli, A.

AU - Brisbin, D.

AU - Buat, V.

AU - Burgarella, D.

AU - Castro-Rodríguez, N.

AU - Cava, A.

AU - Chanial, P.

AU - Clements, D. L.

AU - Conley, A.

AU - Conversi, L.

AU - Cooray, A.

AU - Dowell, C. D.

AU - Dwek, E.

AU - Dye, S.

AU - Elbaz, D.

AU - Farrah, D.

AU - Fox, M.

AU - Franceschini, A.

AU - Gear, W.

AU - Glenn, J.

AU - González Solares, E. A.

AU - Griffin, M.

AU - Harwit, M.

AU - Hatziminaoglou, E.

AU - Huang, J.

AU - Ibar, E.

AU - Isaak, K.

AU - Ivison, R. J.

AU - Lagache, G.

AU - Levenson, L.

AU - Lonsdale, C. J.

AU - Lu, N.

AU - Madden, S.

AU - Maffei, B.

AU - Mainetti, G.

AU - Marchetti, L.

AU - Morrison, G. E.

AU - Mortier, A. M J

AU - Nguyen, H. T.

AU - O'Halloran, B.

AU - Oliver, S. J.

AU - Omont, A.

AU - Owen, F. N.

AU - Page, M. J.

AU - Pannella, M.

AU - Panuzzo, P.

AU - Papageorgiou, A.

AU - Pearson, C. P.

AU - Pérez-Fournon, I.

AU - Pohlen, M.

AU - Rawlings, J. I.

AU - Rigopoulou, D.

AU - Rizzo, D.

AU - Rowan-Robinson, M.

AU - Sánchez Portal, M.

AU - Schulz, B.

AU - Scott, D.

AU - Seymour, N.

AU - Shupe, D. L.

AU - Smith, A. J.

AU - Stevens, J. A.

AU - Strazzullo, V.

AU - Symeonidis, M.

AU - Trichas, M.

AU - Tugwell, K. E.

AU - Vaccari, M.

AU - Valtchanov, I.

AU - Vigroux, L.

AU - Wang, L.

AU - Ward, R.

AU - Wright, G.

AU - Xu, C. K.

AU - Zemcov, M.

N1 - DOI: 10.1051/0004-6361/201014675; eprintid: arXiv:1005.2189

PY - 2010/7/16

Y1 - 2010/7/16

N2 - We have carried out two extremely deep surveys with SPIRE, one of the two cameras on Herschel, at 250 μm, close to the peak of the far-infrared background. We have used the results to investigate the evolution of the rest-frame 250-μm luminosity function out to z = 2. We find evidence for strong evolution out to z $\simeq$ 1 but evidence for at most weak evolution beyond this redshift. Our results suggest that a significant part of the stars and metals in the universe today were formed at z 1.4 in spiral galaxies. © 2010 ESO.

AB - We have carried out two extremely deep surveys with SPIRE, one of the two cameras on Herschel, at 250 μm, close to the peak of the far-infrared background. We have used the results to investigate the evolution of the rest-frame 250-μm luminosity function out to z = 2. We find evidence for strong evolution out to z $\simeq$ 1 but evidence for at most weak evolution beyond this redshift. Our results suggest that a significant part of the stars and metals in the universe today were formed at z 1.4 in spiral galaxies. © 2010 ESO.

KW - Galaxies: evoluton

KW - Galaxies: formation

KW - Galaxies: high-redshift

KW - Submillimeter: galaxies

U2 - 10.1051/0004-6361/201014675

DO - 10.1051/0004-6361/201014675

M3 - Article

SN - 0004-6361

VL - 518

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 2

ER -

First results from HerMES on the evolution of the submillimetre luminosity function

Abstract

Keywords

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