The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts
We investigate the potential of submm-mm and submm-mm-radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500μm by the SPIRE instrument on Herschel. From a sample of 63 previously identified mm sources with reliable radio identifications in the Great Observatori...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2012-02, Vol.419 (4), p.2758-2773 |
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| creator | Roseboom, I. G. Ivison, R. J. Greve, T. R. Amblard, A. Arumugam, V. Auld, R. Aussel, H. Bethermin, M. Blain, A. Bock, J. Boselli, A. Brisbin, D. Buat, V. Burgarella, D. Castro-Rodríguez, N. Cava, A. Chanial, P. Chapin, E. Chapman, S. Clements, D. L. Conley, A. Conversi, L. Cooray, A. Dowell, C. D. Dunlop, J. S. Dwek, E. Eales, S. Elbaz, D. Farrah, D. Franceschini, A. Glenn, J. Griffin, M. Halpern, M. Hatziminaoglou, E. Ibar, E. Isaak, K. Lagache, G. Levenson, L. Lu, N. Madden, S. Maffei, B. Mainetti, G. Marchetti, L. Marsden, G. Morrison, G. Mortier, A. M. J. Nguyen, H. T. O'Halloran, B. Oliver, S. J. Omont, A. Page, M. J. Panuzzo, P. Papageorgiou, A. Pearson, C. P. Pérez-Fournon, I. Pohlen, M. Rawlings, J. I. Raymond, G. Rigopoulou, D. Rizzo, D. Rodighiero, G. Rowan-Robinson, M. Schulz, B. Scott, Douglas Seymour, N. Shupe, D. L. Smith, A. J. Stevens, J. A. Symeonidis, M. Trichas, M. Tugwell, K. E. Vaccari, M. Valtchanov, I. Vieira, J. D. Viero, M. P. Vigroux, L. Wardlow, J. Wang, L. Wright, G. Xu, C. K. Zemcov, M. |
| description | We investigate the potential of submm-mm and submm-mm-radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500μm by the SPIRE instrument on Herschel. From a sample of 63 previously identified mm sources with reliable radio identifications in the Great Observatories Origins Deep Survey North and Lockman Hole North fields, 46 (73 per cent) are found to have detections in at least one SPIRE band. We explore the observed submm/mm colour evolution with redshift, finding that the colours of mm sources are adequately described by a modified blackbody with constant optical depth τ= (ν/nu
0)β, where β=+1.8 and ν0=c/100 μm. We find a tight correlation between dust temperature and IR luminosity. Using a single model of the dust temperature and IR luminosity relation, we derive photometric redshift estimates for the 46 SPIRE-detected mm sources. Testing against the 22 sources with known spectroscopic or good quality optical/near-IR photometric redshifts, we find submm/mm photometric redshifts offer a redshift accuracy of |Δz|/(1 +z) = 0.16 (〈|Δz|〉= 0.51). Including constraints from the radio-far-IR correlation, the accuracy is improved to |Δz|/(1 +z) = 0.15 (〈|Δz|〉= 0.45). We estimate the redshift distribution of mm-selected sources finding a significant excess at z > 3 when compared to ∼ 850 μm selected samples. |
| doi_str_mv | 10.1111/j.1365-2966.2011.19827.x |
| format | Article |
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0)β, where β=+1.8 and ν0=c/100 μm. We find a tight correlation between dust temperature and IR luminosity. Using a single model of the dust temperature and IR luminosity relation, we derive photometric redshift estimates for the 46 SPIRE-detected mm sources. Testing against the 22 sources with known spectroscopic or good quality optical/near-IR photometric redshifts, we find submm/mm photometric redshifts offer a redshift accuracy of |Δz|/(1 +z) = 0.16 (〈|Δz|〉= 0.51). Including constraints from the radio-far-IR correlation, the accuracy is improved to |Δz|/(1 +z) = 0.15 (〈|Δz|〉= 0.45). 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K.</creatorcontrib><creatorcontrib>Zemcov, M.</creatorcontrib><title>The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts</title><title>Monthly notices of the Royal Astronomical Society</title><addtitle>Monthly Notices of the Royal Astronomical Society</addtitle><description>We investigate the potential of submm-mm and submm-mm-radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500μm by the SPIRE instrument on Herschel. From a sample of 63 previously identified mm sources with reliable radio identifications in the Great Observatories Origins Deep Survey North and Lockman Hole North fields, 46 (73 per cent) are found to have detections in at least one SPIRE band. We explore the observed submm/mm colour evolution with redshift, finding that the colours of mm sources are adequately described by a modified blackbody with constant optical depth τ= (ν/nu
0)β, where β=+1.8 and ν0=c/100 μm. We find a tight correlation between dust temperature and IR luminosity. Using a single model of the dust temperature and IR luminosity relation, we derive photometric redshift estimates for the 46 SPIRE-detected mm sources. Testing against the 22 sources with known spectroscopic or good quality optical/near-IR photometric redshifts, we find submm/mm photometric redshifts offer a redshift accuracy of |Δz|/(1 +z) = 0.16 (〈|Δz|〉= 0.51). Including constraints from the radio-far-IR correlation, the accuracy is improved to |Δz|/(1 +z) = 0.15 (〈|Δz|〉= 0.45). We estimate the redshift distribution of mm-selected sources finding a significant excess at z > 3 when compared to ∼ 850 μm selected samples.</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Cosmology</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>galaxies: high‐redshift – galaxies: statistics – submillimetre: galaxies</subject><subject>Luminosity</subject><subject>Sciences of the Universe</subject><subject>Stars & galaxies</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><recordid>eNqNkV9v0zAUxS0EEmXwHSIkhHhIuP4TJ-EBaZoKndQNtPXdcp0b4sppip2M9tvjLFMfQEj4xZbv75xr30NIQiGjcX3cZZTLPGWVlBkDSjNalazIjs_I4lx4ThYAPE_LgtKX5FUIOwAQnMkFud20mKzQB9OiS25GN9h0sOixTpbHwesf2mkzWJPcj_4BT5-S--_Xd8u065JD2w99h4OPxYiH1jZDeE1eNNoFfPO0X5DNl-XmapWuv329vrpcpybntEgrFJAjqwvkXACWpqFGcym1QS2gqmELKClui5zJui6butga1oDRbCupFvyCfJhtW-3UwdtO-5PqtVWry7Wa7oAKwXjJH2hk38_swfc_RwyD6mww6JzeYz8GVTEoIQdZRvLtH-SuH_0-_kNVVFSCA4UIlTNkfB-Cx-bcn4KaElE7NQ1eTYNXUyLqMRF1jNJ3T_46GO0ar_fGhrOe5VxyTlnkPs_cL-vw9N_-6ub27vEYDfhs0I-Hf8jTv5_3G0mcrJ0</recordid><startdate>201202</startdate><enddate>201202</enddate><creator>Roseboom, I. 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K.</creator><creator>Zemcov, M.</creator><general>Blackwell Publishing Ltd</general><general>Wiley-Blackwell</general><general>Oxford University Press</general><general>Oxford University Press (OUP): Policy P - Oxford Open Option A</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7TG</scope><scope>KL.</scope><scope>1XC</scope><scope>VOOES</scope><orcidid>https://orcid.org/0000-0002-6878-9840</orcidid><orcidid>https://orcid.org/0000-0002-3915-2015</orcidid><orcidid>https://orcid.org/0000-0002-9795-6433</orcidid><orcidid>https://orcid.org/0000-0002-2214-5329</orcidid><orcidid>https://orcid.org/0000-0002-4193-2539</orcidid><orcidid>https://orcid.org/0000-0003-3229-2899</orcidid><orcidid>https://orcid.org/0000-0002-0016-8271</orcidid><orcidid>https://orcid.org/0000-0003-3441-903X</orcidid><orcidid>https://orcid.org/0000-0002-1371-5705</orcidid></search><sort><creationdate>201202</creationdate><title>The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts</title><author>Roseboom, I. G. ; Ivison, R. J. ; Greve, T. R. ; Amblard, A. ; Arumugam, V. ; Auld, R. ; Aussel, H. ; Bethermin, M. ; Blain, A. ; Bock, J. ; Boselli, A. ; Brisbin, D. ; Buat, V. ; Burgarella, D. ; Castro-Rodríguez, N. ; Cava, A. ; Chanial, P. ; Chapin, E. ; Chapman, S. ; Clements, D. L. ; Conley, A. ; Conversi, L. ; Cooray, A. ; Dowell, C. D. ; Dunlop, J. S. ; Dwek, E. ; Eales, S. ; Elbaz, D. ; Farrah, D. ; Franceschini, A. ; Glenn, J. ; Griffin, M. ; Halpern, M. ; Hatziminaoglou, E. ; Ibar, E. ; Isaak, K. ; Lagache, G. ; Levenson, L. ; Lu, N. ; Madden, S. ; Maffei, B. ; Mainetti, G. ; Marchetti, L. ; Marsden, G. ; Morrison, G. ; Mortier, A. M. J. ; Nguyen, H. T. ; O'Halloran, B. ; Oliver, S. J. ; Omont, A. ; Page, M. J. ; Panuzzo, P. ; Papageorgiou, A. ; Pearson, C. P. ; Pérez-Fournon, I. ; Pohlen, M. ; Rawlings, J. I. ; Raymond, G. ; Rigopoulou, D. ; Rizzo, D. ; Rodighiero, G. ; Rowan-Robinson, M. ; Schulz, B. ; Scott, Douglas ; Seymour, N. ; Shupe, D. L. ; Smith, A. J. ; Stevens, J. A. ; Symeonidis, M. ; Trichas, M. ; Tugwell, K. E. ; Vaccari, M. ; Valtchanov, I. ; Vieira, J. D. ; Viero, M. P. ; Vigroux, L. ; Wardlow, J. ; Wang, L. ; Wright, G. ; Xu, C. K. ; Zemcov, M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c5317-9e405e2d7e3340e8cf1ca366acea409d0b0e61eb7526dd8fd7bc2f0ca2b61a43</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Cosmology</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>galaxies: high‐redshift – galaxies: statistics – submillimetre: galaxies</topic><topic>Luminosity</topic><topic>Sciences of the Universe</topic><topic>Stars & galaxies</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Roseboom, I. G.</creatorcontrib><creatorcontrib>Ivison, R. J.</creatorcontrib><creatorcontrib>Greve, T. R.</creatorcontrib><creatorcontrib>Amblard, A.</creatorcontrib><creatorcontrib>Arumugam, V.</creatorcontrib><creatorcontrib>Auld, R.</creatorcontrib><creatorcontrib>Aussel, H.</creatorcontrib><creatorcontrib>Bethermin, M.</creatorcontrib><creatorcontrib>Blain, A.</creatorcontrib><creatorcontrib>Bock, J.</creatorcontrib><creatorcontrib>Boselli, A.</creatorcontrib><creatorcontrib>Brisbin, D.</creatorcontrib><creatorcontrib>Buat, V.</creatorcontrib><creatorcontrib>Burgarella, D.</creatorcontrib><creatorcontrib>Castro-Rodríguez, N.</creatorcontrib><creatorcontrib>Cava, A.</creatorcontrib><creatorcontrib>Chanial, P.</creatorcontrib><creatorcontrib>Chapin, E.</creatorcontrib><creatorcontrib>Chapman, S.</creatorcontrib><creatorcontrib>Clements, D. L.</creatorcontrib><creatorcontrib>Conley, A.</creatorcontrib><creatorcontrib>Conversi, L.</creatorcontrib><creatorcontrib>Cooray, A.</creatorcontrib><creatorcontrib>Dowell, C. D.</creatorcontrib><creatorcontrib>Dunlop, J. S.</creatorcontrib><creatorcontrib>Dwek, E.</creatorcontrib><creatorcontrib>Eales, S.</creatorcontrib><creatorcontrib>Elbaz, D.</creatorcontrib><creatorcontrib>Farrah, D.</creatorcontrib><creatorcontrib>Franceschini, A.</creatorcontrib><creatorcontrib>Glenn, J.</creatorcontrib><creatorcontrib>Griffin, M.</creatorcontrib><creatorcontrib>Halpern, M.</creatorcontrib><creatorcontrib>Hatziminaoglou, E.</creatorcontrib><creatorcontrib>Ibar, E.</creatorcontrib><creatorcontrib>Isaak, K.</creatorcontrib><creatorcontrib>Lagache, G.</creatorcontrib><creatorcontrib>Levenson, L.</creatorcontrib><creatorcontrib>Lu, N.</creatorcontrib><creatorcontrib>Madden, S.</creatorcontrib><creatorcontrib>Maffei, B.</creatorcontrib><creatorcontrib>Mainetti, G.</creatorcontrib><creatorcontrib>Marchetti, L.</creatorcontrib><creatorcontrib>Marsden, G.</creatorcontrib><creatorcontrib>Morrison, G.</creatorcontrib><creatorcontrib>Mortier, A. M. J.</creatorcontrib><creatorcontrib>Nguyen, H. T.</creatorcontrib><creatorcontrib>O'Halloran, B.</creatorcontrib><creatorcontrib>Oliver, S. J.</creatorcontrib><creatorcontrib>Omont, A.</creatorcontrib><creatorcontrib>Page, M. J.</creatorcontrib><creatorcontrib>Panuzzo, P.</creatorcontrib><creatorcontrib>Papageorgiou, A.</creatorcontrib><creatorcontrib>Pearson, C. P.</creatorcontrib><creatorcontrib>Pérez-Fournon, I.</creatorcontrib><creatorcontrib>Pohlen, M.</creatorcontrib><creatorcontrib>Rawlings, J. I.</creatorcontrib><creatorcontrib>Raymond, G.</creatorcontrib><creatorcontrib>Rigopoulou, D.</creatorcontrib><creatorcontrib>Rizzo, D.</creatorcontrib><creatorcontrib>Rodighiero, G.</creatorcontrib><creatorcontrib>Rowan-Robinson, M.</creatorcontrib><creatorcontrib>Schulz, B.</creatorcontrib><creatorcontrib>Scott, Douglas</creatorcontrib><creatorcontrib>Seymour, N.</creatorcontrib><creatorcontrib>Shupe, D. L.</creatorcontrib><creatorcontrib>Smith, A. J.</creatorcontrib><creatorcontrib>Stevens, J. A.</creatorcontrib><creatorcontrib>Symeonidis, M.</creatorcontrib><creatorcontrib>Trichas, M.</creatorcontrib><creatorcontrib>Tugwell, K. E.</creatorcontrib><creatorcontrib>Vaccari, M.</creatorcontrib><creatorcontrib>Valtchanov, I.</creatorcontrib><creatorcontrib>Vieira, J. D.</creatorcontrib><creatorcontrib>Viero, M. P.</creatorcontrib><creatorcontrib>Vigroux, L.</creatorcontrib><creatorcontrib>Wardlow, J.</creatorcontrib><creatorcontrib>Wang, L.</creatorcontrib><creatorcontrib>Wright, G.</creatorcontrib><creatorcontrib>Xu, C. K.</creatorcontrib><creatorcontrib>Zemcov, M.</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Roseboom, I. G.</au><au>Ivison, R. J.</au><au>Greve, T. R.</au><au>Amblard, A.</au><au>Arumugam, V.</au><au>Auld, R.</au><au>Aussel, H.</au><au>Bethermin, M.</au><au>Blain, A.</au><au>Bock, J.</au><au>Boselli, A.</au><au>Brisbin, D.</au><au>Buat, V.</au><au>Burgarella, D.</au><au>Castro-Rodríguez, N.</au><au>Cava, A.</au><au>Chanial, P.</au><au>Chapin, E.</au><au>Chapman, S.</au><au>Clements, D. L.</au><au>Conley, A.</au><au>Conversi, L.</au><au>Cooray, A.</au><au>Dowell, C. D.</au><au>Dunlop, J. S.</au><au>Dwek, E.</au><au>Eales, S.</au><au>Elbaz, D.</au><au>Farrah, D.</au><au>Franceschini, A.</au><au>Glenn, J.</au><au>Griffin, M.</au><au>Halpern, M.</au><au>Hatziminaoglou, E.</au><au>Ibar, E.</au><au>Isaak, K.</au><au>Lagache, G.</au><au>Levenson, L.</au><au>Lu, N.</au><au>Madden, S.</au><au>Maffei, B.</au><au>Mainetti, G.</au><au>Marchetti, L.</au><au>Marsden, G.</au><au>Morrison, G.</au><au>Mortier, A. M. J.</au><au>Nguyen, H. T.</au><au>O'Halloran, B.</au><au>Oliver, S. J.</au><au>Omont, A.</au><au>Page, M. J.</au><au>Panuzzo, P.</au><au>Papageorgiou, A.</au><au>Pearson, C. P.</au><au>Pérez-Fournon, I.</au><au>Pohlen, M.</au><au>Rawlings, J. I.</au><au>Raymond, G.</au><au>Rigopoulou, D.</au><au>Rizzo, D.</au><au>Rodighiero, G.</au><au>Rowan-Robinson, M.</au><au>Schulz, B.</au><au>Scott, Douglas</au><au>Seymour, N.</au><au>Shupe, D. L.</au><au>Smith, A. J.</au><au>Stevens, J. A.</au><au>Symeonidis, M.</au><au>Trichas, M.</au><au>Tugwell, K. E.</au><au>Vaccari, M.</au><au>Valtchanov, I.</au><au>Vieira, J. D.</au><au>Viero, M. P.</au><au>Vigroux, L.</au><au>Wardlow, J.</au><au>Wang, L.</au><au>Wright, G.</au><au>Xu, C. K.</au><au>Zemcov, M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><stitle>Monthly Notices of the Royal Astronomical Society</stitle><date>2012-02</date><risdate>2012</risdate><volume>419</volume><issue>4</issue><spage>2758</spage><epage>2773</epage><pages>2758-2773</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><coden>MNRAA4</coden><abstract>We investigate the potential of submm-mm and submm-mm-radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500μm by the SPIRE instrument on Herschel. From a sample of 63 previously identified mm sources with reliable radio identifications in the Great Observatories Origins Deep Survey North and Lockman Hole North fields, 46 (73 per cent) are found to have detections in at least one SPIRE band. We explore the observed submm/mm colour evolution with redshift, finding that the colours of mm sources are adequately described by a modified blackbody with constant optical depth τ= (ν/nu
0)β, where β=+1.8 and ν0=c/100 μm. We find a tight correlation between dust temperature and IR luminosity. Using a single model of the dust temperature and IR luminosity relation, we derive photometric redshift estimates for the 46 SPIRE-detected mm sources. Testing against the 22 sources with known spectroscopic or good quality optical/near-IR photometric redshifts, we find submm/mm photometric redshifts offer a redshift accuracy of |Δz|/(1 +z) = 0.16 (〈|Δz|〉= 0.51). Including constraints from the radio-far-IR correlation, the accuracy is improved to |Δz|/(1 +z) = 0.15 (〈|Δz|〉= 0.45). We estimate the redshift distribution of mm-selected sources finding a significant excess at z > 3 when compared to ∼ 850 μm selected samples.</abstract><cop>Oxford, UK</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1111/j.1365-2966.2011.19827.x</doi><tpages>16</tpages><orcidid>https://orcid.org/0000-0002-6878-9840</orcidid><orcidid>https://orcid.org/0000-0002-3915-2015</orcidid><orcidid>https://orcid.org/0000-0002-9795-6433</orcidid><orcidid>https://orcid.org/0000-0002-2214-5329</orcidid><orcidid>https://orcid.org/0000-0002-4193-2539</orcidid><orcidid>https://orcid.org/0000-0003-3229-2899</orcidid><orcidid>https://orcid.org/0000-0002-0016-8271</orcidid><orcidid>https://orcid.org/0000-0003-3441-903X</orcidid><orcidid>https://orcid.org/0000-0002-1371-5705</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0035-8711 |
| ispartof | Monthly notices of the Royal Astronomical Society, 2012-02, Vol.419 (4), p.2758-2773 |
| issn | 0035-8711 1365-2966 |
| language | eng |
| recordid | cdi_hal_primary_oai_HAL_hal_01442383v1 |
| source | Wiley Online Library Journals Frontfile Complete; Oxford Journals Open Access Collection |
| subjects | Astronomy Astrophysics Cosmology Earth, ocean, space Exact sciences and technology galaxies: high‐redshift – galaxies: statistics – submillimetre: galaxies Luminosity Sciences of the Universe Stars & galaxies |
| title | The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts |
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