First results from HerMES on the evolution of the submillimetre luminosity function
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 evo...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Journal Article |
| Published: |
EDP Sciences
2010
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| Online Access: | http://hdl.handle.net/20.500.11937/37367 |
| _version_ | 1848755027566395392 |
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| author | Eales, S. Raymond, G. Roseboom, I. 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. Conley, A. Conversi, L. Cooray, A. Dowell, C. Dwek, E. Dye, S. Elbaz, D. Farrah, D. Fox, M. Franceschini, A. Gear, W. Glenn, J. González Solares, E. Griffin, M. Harwit, M. Hatziminaoglou, E. Huang, J. Ibar, E. Isaak, K. Ivison, R. Lagache, G. Levenson, L. Lonsdale, C. Lu, N. Madden, S. Maffei, B. Mainetti, G. Marchetti, L. Morrison, G. Mortier, A. Nguyen, H. O'Halloran, B. Oliver, S. Omont, A. Owen, F. Page, M. Pannella, M. Panuzzo, P. Papageorgiou, A. Pearson, C. Pérez-Fournon, I. Pohlen, M. Rawlings, J. Rigopoulou, D. Rizzo, D. Rowan-Robinson, M. Sánchez Portal, M. Schulz, B. Scott, D. Seymour, Nick Shupe, D. Smith, A. Stevens, J. Strazzullo, V. Symeonidis, M. Trichas, M. Tugwell, K. Vaccari, M. Valtchanov, I. Vigroux, L. Wang, L. Ward, R. Wright, G. Xu, C. |
| author_facet | Eales, S. Raymond, G. Roseboom, I. 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. Conley, A. Conversi, L. Cooray, A. Dowell, C. Dwek, E. Dye, S. Elbaz, D. Farrah, D. Fox, M. Franceschini, A. Gear, W. Glenn, J. González Solares, E. Griffin, M. Harwit, M. Hatziminaoglou, E. Huang, J. Ibar, E. Isaak, K. Ivison, R. Lagache, G. Levenson, L. Lonsdale, C. Lu, N. Madden, S. Maffei, B. Mainetti, G. Marchetti, L. Morrison, G. Mortier, A. Nguyen, H. O'Halloran, B. Oliver, S. Omont, A. Owen, F. Page, M. Pannella, M. Panuzzo, P. Papageorgiou, A. Pearson, C. Pérez-Fournon, I. Pohlen, M. Rawlings, J. Rigopoulou, D. Rizzo, D. Rowan-Robinson, M. Sánchez Portal, M. Schulz, B. Scott, D. Seymour, Nick Shupe, D. Smith, A. Stevens, J. Strazzullo, V. Symeonidis, M. Trichas, M. Tugwell, K. Vaccari, M. Valtchanov, I. Vigroux, L. Wang, L. Ward, R. Wright, G. Xu, C. |
| author_sort | Eales, S. |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | 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. |
| first_indexed | 2025-11-14T08:49:47Z |
| format | Journal Article |
| id | curtin-20.500.11937-37367 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T08:49:47Z |
| publishDate | 2010 |
| publisher | EDP Sciences |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-373672017-09-13T13:38:14Z First results from HerMES on the evolution of the submillimetre luminosity function Eales, S. Raymond, G. Roseboom, I. 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. Conley, A. Conversi, L. Cooray, A. Dowell, C. Dwek, E. Dye, S. Elbaz, D. Farrah, D. Fox, M. Franceschini, A. Gear, W. Glenn, J. González Solares, E. Griffin, M. Harwit, M. Hatziminaoglou, E. Huang, J. Ibar, E. Isaak, K. Ivison, R. Lagache, G. Levenson, L. Lonsdale, C. Lu, N. Madden, S. Maffei, B. Mainetti, G. Marchetti, L. Morrison, G. Mortier, A. Nguyen, H. O'Halloran, B. Oliver, S. Omont, A. Owen, F. Page, M. Pannella, M. Panuzzo, P. Papageorgiou, A. Pearson, C. Pérez-Fournon, I. Pohlen, M. Rawlings, J. Rigopoulou, D. Rizzo, D. Rowan-Robinson, M. Sánchez Portal, M. Schulz, B. Scott, D. Seymour, Nick Shupe, D. Smith, A. Stevens, J. Strazzullo, V. Symeonidis, M. Trichas, M. Tugwell, K. Vaccari, M. Valtchanov, I. Vigroux, L. Wang, L. Ward, R. Wright, G. Xu, C. 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. 2010 Journal Article http://hdl.handle.net/20.500.11937/37367 10.1051/0004-6361/201014675 EDP Sciences unknown |
| spellingShingle | Eales, S. Raymond, G. Roseboom, I. 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. Conley, A. Conversi, L. Cooray, A. Dowell, C. Dwek, E. Dye, S. Elbaz, D. Farrah, D. Fox, M. Franceschini, A. Gear, W. Glenn, J. González Solares, E. Griffin, M. Harwit, M. Hatziminaoglou, E. Huang, J. Ibar, E. Isaak, K. Ivison, R. Lagache, G. Levenson, L. Lonsdale, C. Lu, N. Madden, S. Maffei, B. Mainetti, G. Marchetti, L. Morrison, G. Mortier, A. Nguyen, H. O'Halloran, B. Oliver, S. Omont, A. Owen, F. Page, M. Pannella, M. Panuzzo, P. Papageorgiou, A. Pearson, C. Pérez-Fournon, I. Pohlen, M. Rawlings, J. Rigopoulou, D. Rizzo, D. Rowan-Robinson, M. Sánchez Portal, M. Schulz, B. Scott, D. Seymour, Nick Shupe, D. Smith, A. Stevens, J. Strazzullo, V. Symeonidis, M. Trichas, M. Tugwell, K. Vaccari, M. Valtchanov, I. Vigroux, L. Wang, L. Ward, R. Wright, G. Xu, C. First results from HerMES on the evolution of the submillimetre luminosity function |
| title | First results from HerMES on the evolution of the submillimetre luminosity function |
| title_full | First results from HerMES on the evolution of the submillimetre luminosity function |
| title_fullStr | First results from HerMES on the evolution of the submillimetre luminosity function |
| title_full_unstemmed | First results from HerMES on the evolution of the submillimetre luminosity function |
| title_short | First results from HerMES on the evolution of the submillimetre luminosity function |
| title_sort | first results from hermes on the evolution of the submillimetre luminosity function |
| url | http://hdl.handle.net/20.500.11937/37367 |