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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Main Authors:	Roseboom, I., Ivison, R., Greve, T., 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., Conley, A., Conversi, L., Cooray, A., Dowell, C., Dunlop, J., 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., Nguyen, H., O'Halloran, B., Oliver, S., Omont, A., Page, M., Panuzzo, P., Papageorgiou, A., Pearson, C., Pérez-Fournon, I., Pohlen, M., Rawlings, J., Raymond, G., Rigopoulou, D., Rizzo, D., Rodighiero, G., Rowan-Robinson, M., Schulz, B., Scott, D., Seymour, Nick, Shupe, D., Smith, A., Stevens, J., Symeonidis, M., Trichas, M., Tugwell, K., Vaccari, M., Valtchanov, I., Vieira, J., Viero, M., Vigroux, L., Wardlow, J., Wang, L., Wright, G., Xu, C., Zemcov, M.
Format:	Journal Article
Published:	2012
Online Access:	http://hdl.handle.net/20.500.11937/25797

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author	Roseboom, I. Ivison, R. Greve, T. 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. Conley, A. Conversi, L. Cooray, A. Dowell, C. Dunlop, J. 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. Nguyen, H. O'Halloran, B. Oliver, S. Omont, A. Page, M. Panuzzo, P. Papageorgiou, A. Pearson, C. Pérez-Fournon, I. Pohlen, M. Rawlings, J. Raymond, G. Rigopoulou, D. Rizzo, D. Rodighiero, G. Rowan-Robinson, M. Schulz, B. Scott, D. Seymour, Nick Shupe, D. Smith, A. Stevens, J. Symeonidis, M. Trichas, M. Tugwell, K. Vaccari, M. Valtchanov, I. Vieira, J. Viero, M. Vigroux, L. Wardlow, J. Wang, L. Wright, G. Xu, C. Zemcov, M.
author_facet	Roseboom, I. Ivison, R. Greve, T. 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. Conley, A. Conversi, L. Cooray, A. Dowell, C. Dunlop, J. 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. Nguyen, H. O'Halloran, B. Oliver, S. Omont, A. Page, M. Panuzzo, P. Papageorgiou, A. Pearson, C. Pérez-Fournon, I. Pohlen, M. Rawlings, J. Raymond, G. Rigopoulou, D. Rizzo, D. Rodighiero, G. Rowan-Robinson, M. Schulz, B. Scott, D. Seymour, Nick Shupe, D. Smith, A. Stevens, J. Symeonidis, M. Trichas, M. Tugwell, K. Vaccari, M. Valtchanov, I. Vieira, J. Viero, M. Vigroux, L. Wardlow, J. Wang, L. Wright, G. Xu, C. Zemcov, M.
author_sort	Roseboom, I.
building	Curtin Institutional Repository
collection	Online Access
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/nu0)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.
first_indexed	2025-11-14T07:58:36Z
format	Journal Article
id	curtin-20.500.11937-25797
institution	Curtin University Malaysia
institution_category	Local University
last_indexed	2025-11-14T07:58:36Z
publishDate	2012
recordtype	eprints
repository_type	Digital Repository
spelling	curtin-20.500.11937-257972017-09-13T15:23:05Z The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts Roseboom, I. Ivison, R. Greve, T. 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. Conley, A. Conversi, L. Cooray, A. Dowell, C. Dunlop, J. 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. Nguyen, H. O'Halloran, B. Oliver, S. Omont, A. Page, M. Panuzzo, P. Papageorgiou, A. Pearson, C. Pérez-Fournon, I. Pohlen, M. Rawlings, J. Raymond, G. Rigopoulou, D. Rizzo, D. Rodighiero, G. Rowan-Robinson, M. Schulz, B. Scott, D. Seymour, Nick Shupe, D. Smith, A. Stevens, J. Symeonidis, M. Trichas, M. Tugwell, K. Vaccari, M. Valtchanov, I. Vieira, J. Viero, M. Vigroux, L. Wardlow, J. Wang, L. Wright, G. Xu, C. Zemcov, M. 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/nu0)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. 2012 Journal Article http://hdl.handle.net/20.500.11937/25797 10.1111/j.1365-2966.2011.19827.x fulltext
spellingShingle	Roseboom, I. Ivison, R. Greve, T. 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. Conley, A. Conversi, L. Cooray, A. Dowell, C. Dunlop, J. 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. Nguyen, H. O'Halloran, B. Oliver, S. Omont, A. Page, M. Panuzzo, P. Papageorgiou, A. Pearson, C. Pérez-Fournon, I. Pohlen, M. Rawlings, J. Raymond, G. Rigopoulou, D. Rizzo, D. Rodighiero, G. Rowan-Robinson, M. Schulz, B. Scott, D. Seymour, Nick Shupe, D. Smith, A. Stevens, J. Symeonidis, M. Trichas, M. Tugwell, K. Vaccari, M. Valtchanov, I. Vieira, J. Viero, M. Vigroux, L. Wardlow, J. Wang, L. Wright, G. Xu, C. Zemcov, M. The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts
title	The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts
title_full	The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts
title_fullStr	The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts
title_full_unstemmed	The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts
title_short	The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts
title_sort	herschel multi-tiered extragalactic survey: spire-mm photometric redshifts
url	http://hdl.handle.net/20.500.11937/25797

The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts

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