Evolution of dust temperature of galaxies through cosmic time as seen by Herschel

H. S. Hwang; D. Elbaz; G. Magdis; E. Daddi; M. Symeonidis; B. Altieri; A. Amblard; P. Andreani; V. Arumugam; R. Auld; H. Aussel; T. Babbedge; S. Berta; A. Blain; J. Bock; A. Bongiovanni; A. Boselli; V. Buat; D. Burgarella; N. Castro-Rodríguez; A. Cava; J. Cepa; P. Chanial; E. Chapin; R. R. Chary; A. Cimatti; D. L Z Clements; A. Conley; L. Conversi; A. Cooray; H. Dannerbauer; M. Dickinson; H. Dominguez; C. D. Dowell; J. S. Dunlop; E. Dwek; S. Eales; D. Farrah; N. Förster Schreiber; M. Fox; A. Franceschini; W. Gear; R. Genzel; J. Glenn; M. Griffin; C. Gruppioni; M. Halpern; E. Hatziminaoglou; E. Ibar; K. Isaak; R. J. Ivison; W. S. Jeong; G. Lagache; D. Le Borgne; E. Le Floc'h; H. M. Lee; J. C. Lee; M. G. Lee; L. Levenson; N. Lu; D. Lutz; S. Madden; B. Maffei; B. Magnelli; G. Mainetti; R. Maiolino; L. Marchetti; A. M J Mortier; H. T. Nguyen; R. Nordon; B. O'Halloran; K. Okumura; S. J. Oliver; A. Omont; M. J. Page; P. Panuzzo; A. Papageorgiou; C. P. Pearson; I. Pérez-Fournon; A. M Pérez García; A. Poglitsch; M. Pohlen; P. Popesso; F. Pozzi; J. I. Rawlings; D. Rigopoulou; L. Riguccini; D. Rizzo; G. Rodighiero; I. G. Roseboom; M. Rowan-Robinson; A. Saintonge; M. Sánchez Portal; P. Santini; M. Sauvage; B. Schulz; D. Scott; N. Seymour; L. Shao; D. L. Shupe; A. J. Smith; J. A. Stevens; E. Sturm; L. Tacconi; M. Trichas; K. E. Tugwell; M. Vaccari; I. Valtchanov; J. D. Vieira; L. Vigroux; L. Wang; R. Ward; G. Wright; C. K. Xu; M. Zemcov

doi:10.1111/j.1365-2966.2010.17645.x

Evolution of dust temperature of galaxies through cosmic time as seen by Herschel

H. S. Hwang, D. Elbaz, G. Magdis, E. Daddi, M. Symeonidis, B. Altieri, A. Amblard, P. Andreani, V. Arumugam, R. Auld, H. Aussel, T. Babbedge, S. Berta, A. Blain, J. Bock, A. Bongiovanni, A. Boselli, V. Buat, D. Burgarella, N. Castro-RodríguezA. Cava, J. Cepa, P. Chanial, E. Chapin, R. R. Chary, A. Cimatti, D. L Z Clements, A. Conley, L. Conversi, A. Cooray, H. Dannerbauer, M. Dickinson, H. Dominguez, C. D. Dowell, J. S. Dunlop, E. Dwek, S. Eales, D. Farrah, N. Förster Schreiber, M. Fox, A. Franceschini, W. Gear, R. Genzel, J. Glenn, M. Griffin, C. Gruppioni, M. Halpern, E. Hatziminaoglou, E. Ibar, K. Isaak, R. J. Ivison, W. S. Jeong, G. Lagache, D. Le Borgne, E. Le Floc'h, H. M. Lee, J. C. Lee, M. G. Lee, L. Levenson, N. Lu, D. Lutz, S. Madden, B. Maffei, B. Magnelli, G. Mainetti, R. Maiolino, L. Marchetti, A. M J Mortier, H. T. Nguyen, R. Nordon, B. O'Halloran, K. Okumura, S. J. Oliver, A. Omont, M. J. Page, P. Panuzzo, A. Papageorgiou, C. P. Pearson, I. Pérez-Fournon, A. M Pérez García, A. Poglitsch, M. Pohlen, P. Popesso, F. Pozzi, J. I. Rawlings, D. Rigopoulou, L. Riguccini, D. Rizzo, G. Rodighiero, I. G. Roseboom, M. Rowan-Robinson, A. Saintonge, M. Sánchez Portal, P. Santini, M. Sauvage, B. Schulz, D. Scott, N. Seymour, L. Shao, D. L. Shupe, A. J. Smith, J. A. Stevens, E. Sturm, L. Tacconi, M. Trichas, K. E. Tugwell, M. Vaccari, I. Valtchanov, J. D. Vieira, L. Vigroux, L. Wang, R. Ward, G. Wright, C. K. Xu, M. Zemcov

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

Abstract

We study the dust properties of galaxies in the redshift range 0.1 ≲z≲ 2.8 observed by the Herschel Space Observatory in the field of the Great Observatories Origins Deep Survey-North as part of the PACS Extragalactic Probe (PEP) and Herschel Multi-tiered Extragalactic Survey (HerMES) key programmes. Infrared (IR) luminosity (LIR) and dust temperature (Tdust) of galaxies are derived from the spectral energy distribution fit of the far-IR (FIR) flux densities obtained with the PACS and SPIRE instruments onboard Herschel. As a reference sample, we also obtain IR luminosities and dust temperatures of local galaxies at z <0.1 using AKARI and IRAS data in the field of the Sloan Digital Sky Survey. We compare the LIR-Tdust relation between the two samples and find that the median Tdust of Herschel-selected galaxies at z<0.5 with LIR≲ 5 × 1010L· appears to be 2-5 K colder than that of AKARI-selected local galaxies with similar luminosities, and the dispersion in Tdust for high-z galaxies increases with LIR due to the existence of cold galaxies that are not seen among local galaxies. We show that this large dispersion of the LIR-Tdust relation can bridge the gap between local star-forming galaxies and high-z submillimetre galaxies (SMGs). We also find that three SMGs with very low Tdust (≲20 K) covered in this study have close neighbouring sources with similar 24-μm brightness, which could lead to an overestimation of FIR/(sub)millimetre fluxes of the SMGs. © 2010 The Authors. Journal compilation © 2010 RAS.

Original language	English
Pages (from-to)	75-82
Number of pages	7
Journal	Monthly Notices of the Royal Astronomical Society
Volume	409
Issue number	1
DOIs	https://doi.org/10.1111/j.1365-2966.2010.17645.x
Publication status	Published - Nov 2010

Keywords

Galaxies: evolution
Galaxies: formation
Galaxies: general
Galaxies: high-redshift
Galaxies: starburst
Infrared: galaxies

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10.1111/j.1365-2966.2010.17645.x

http://adsabs.harvard.edu/abs/2010MNRAS.409...75H

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Hwang, H. S., Elbaz, D., Magdis, G., Daddi, E., Symeonidis, M., Altieri, B., Amblard, A., Andreani, P., Arumugam, V., Auld, R., Aussel, H., Babbedge, T., Berta, S., Blain, A., Bock, J., Bongiovanni, A., Boselli, A., Buat, V., Burgarella, D., ... Zemcov, M. (2010). Evolution of dust temperature of galaxies through cosmic time as seen by Herschel. Monthly Notices of the Royal Astronomical Society, 409(1), 75-82. https://doi.org/10.1111/j.1365-2966.2010.17645.x

@article{9cda2c87fff64fe3aee174b91a5790f1,

title = "Evolution of dust temperature of galaxies through cosmic time as seen by Herschel",

abstract = "We study the dust properties of galaxies in the redshift range 0.1 ≲z≲ 2.8 observed by the Herschel Space Observatory in the field of the Great Observatories Origins Deep Survey-North as part of the PACS Extragalactic Probe (PEP) and Herschel Multi-tiered Extragalactic Survey (HerMES) key programmes. Infrared (IR) luminosity (LIR) and dust temperature (Tdust) of galaxies are derived from the spectral energy distribution fit of the far-IR (FIR) flux densities obtained with the PACS and SPIRE instruments onboard Herschel. As a reference sample, we also obtain IR luminosities and dust temperatures of local galaxies at z <0.1 using AKARI and IRAS data in the field of the Sloan Digital Sky Survey. We compare the LIR-Tdust relation between the two samples and find that the median Tdust of Herschel-selected galaxies at z<0.5 with LIR≲ 5 × 1010L· appears to be 2-5 K colder than that of AKARI-selected local galaxies with similar luminosities, and the dispersion in Tdust for high-z galaxies increases with LIR due to the existence of cold galaxies that are not seen among local galaxies. We show that this large dispersion of the LIR-Tdust relation can bridge the gap between local star-forming galaxies and high-z submillimetre galaxies (SMGs). We also find that three SMGs with very low Tdust (≲20 K) covered in this study have close neighbouring sources with similar 24-μm brightness, which could lead to an overestimation of FIR/(sub)millimetre fluxes of the SMGs. {\textcopyright} 2010 The Authors. Journal compilation {\textcopyright} 2010 RAS.",

keywords = "Galaxies: evolution, Galaxies: formation, Galaxies: general, Galaxies: high-redshift, Galaxies: starburst, Infrared: galaxies",

author = "Hwang, \{H. S.\} and D. Elbaz and G. Magdis and E. Daddi and M. Symeonidis and B. Altieri and A. Amblard and P. Andreani and V. Arumugam and R. Auld and H. Aussel and T. Babbedge and S. Berta and A. Blain and J. Bock and A. Bongiovanni and A. Boselli and V. Buat and D. Burgarella and N. Castro-Rodr{\'i}guez and A. Cava and J. Cepa and P. Chanial and E. Chapin and Chary, \{R. R.\} and A. Cimatti and Clements, \{D. L Z\} and A. Conley and L. Conversi and A. Cooray and H. Dannerbauer and M. Dickinson and H. Dominguez and Dowell, \{C. D.\} and Dunlop, \{J. S.\} and E. Dwek and S. Eales and D. Farrah and Schreiber, \{N. F{\"o}rster\} and M. Fox and A. Franceschini and W. Gear and R. Genzel and J. Glenn and M. Griffin and C. Gruppioni and M. Halpern and E. Hatziminaoglou and E. Ibar and K. Isaak and Ivison, \{R. J.\} and Jeong, \{W. S.\} and G. Lagache and \{Le Borgne\}, D. and \{Le Floc'h\}, E. and Lee, \{H. M.\} and Lee, \{J. C.\} and Lee, \{M. G.\} and L. Levenson and N. Lu and D. Lutz and S. Madden and B. Maffei and B. Magnelli and G. Mainetti and R. Maiolino and L. Marchetti and Mortier, \{A. M J\} and Nguyen, \{H. T.\} and R. Nordon and B. O'Halloran and K. Okumura and Oliver, \{S. J.\} and A. Omont and Page, \{M. J.\} and P. Panuzzo and A. Papageorgiou and Pearson, \{C. P.\} and I. P{\'e}rez-Fournon and Garc{\'i}a, \{A. M P{\'e}rez\} and A. Poglitsch and M. Pohlen and P. Popesso and F. Pozzi and Rawlings, \{J. I.\} and D. Rigopoulou and L. Riguccini and D. Rizzo and G. Rodighiero and Roseboom, \{I. G.\} and M. Rowan-Robinson and A. Saintonge and Portal, \{M. S{\'a}nchez\} and P. Santini and M. Sauvage and B. Schulz and D. Scott and N. Seymour and L. Shao and Shupe, \{D. L.\} and Smith, \{A. J.\} and Stevens, \{J. A.\} and E. Sturm and L. Tacconi and M. Trichas and Tugwell, \{K. E.\} and M. Vaccari and I. Valtchanov and Vieira, \{J. D.\} and L. Vigroux and L. Wang and R. Ward and G. Wright and Xu, \{C. K.\} and M. Zemcov",

note = "DOI: 10.1111/j.1365-2966.2010.17645.x; eprintid: arXiv:1009.1058",

year = "2010",

month = nov,

doi = "10.1111/j.1365-2966.2010.17645.x",

language = "English",

volume = "409",

pages = "75--82",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "1365-2966",

publisher = "Oxford University Press",

number = "1",

}

Hwang, HS, Elbaz, D, Magdis, G, Daddi, E, Symeonidis, M, Altieri, B, Amblard, A, Andreani, P, Arumugam, V, Auld, R, Aussel, H, Babbedge, T, Berta, S, Blain, A, Bock, J, Bongiovanni, A, Boselli, A, Buat, V, Burgarella, D, Castro-Rodríguez, N, Cava, A, Cepa, J, Chanial, P, Chapin, E, Chary, RR, Cimatti, A, Clements, DLZ, Conley, A, Conversi, L, Cooray, A, Dannerbauer, H, Dickinson, M, Dominguez, H, Dowell, CD, Dunlop, JS, Dwek, E, Eales, S, Farrah, D, Schreiber, NF, Fox, M, Franceschini, A, Gear, W, Genzel, R, Glenn, J, Griffin, M, Gruppioni, C, Halpern, M, Hatziminaoglou, E, Ibar, E, Isaak, K, Ivison, RJ, Jeong, WS, Lagache, G, Le Borgne, D, Le Floc'h, E, Lee, HM, Lee, JC, Lee, MG, Levenson, L, Lu, N, Lutz, D, Madden, S, Maffei, B, Magnelli, B, Mainetti, G, Maiolino, R, Marchetti, L, Mortier, AMJ, Nguyen, HT, Nordon, R, O'Halloran, B, Okumura, K, Oliver, SJ, Omont, A, Page, MJ, Panuzzo, P, Papageorgiou, A, Pearson, CP, Pérez-Fournon, I, García, AMP, Poglitsch, A, Pohlen, M, Popesso, P, Pozzi, F, Rawlings, JI, Rigopoulou, D, Riguccini, L, Rizzo, D, Rodighiero, G, Roseboom, IG, Rowan-Robinson, M, Saintonge, A, Portal, MS, Santini, P, Sauvage, M, Schulz, B, Scott, D, Seymour, N, Shao, L, Shupe, DL, Smith, AJ, Stevens, JA, Sturm, E, Tacconi, L, Trichas, M, Tugwell, KE, Vaccari, M, Valtchanov, I, Vieira, JD, Vigroux, L, Wang, L, Ward, R, Wright, G, Xu, CK & Zemcov, M 2010, 'Evolution of dust temperature of galaxies through cosmic time as seen by Herschel', Monthly Notices of the Royal Astronomical Society, vol. 409, no. 1, pp. 75-82. https://doi.org/10.1111/j.1365-2966.2010.17645.x

TY - JOUR

T1 - Evolution of dust temperature of galaxies through cosmic time as seen by Herschel

AU - Hwang, H. S.

AU - Elbaz, D.

AU - Magdis, G.

AU - Daddi, E.

AU - Symeonidis, M.

AU - Altieri, B.

AU - Amblard, A.

AU - Andreani, P.

AU - Arumugam, V.

AU - Auld, R.

AU - Aussel, H.

AU - Babbedge, T.

AU - Berta, S.

AU - Blain, A.

AU - Bock, J.

AU - Bongiovanni, A.

AU - Boselli, A.

AU - Buat, V.

AU - Burgarella, D.

AU - Castro-Rodríguez, N.

AU - Cava, A.

AU - Cepa, J.

AU - Chanial, P.

AU - Chapin, E.

AU - Chary, R. R.

AU - Cimatti, A.

AU - Clements, D. L Z

AU - Conley, A.

AU - Conversi, L.

AU - Cooray, A.

AU - Dannerbauer, H.

AU - Dickinson, M.

AU - Dominguez, H.

AU - Dowell, C. D.

AU - Dunlop, J. S.

AU - Dwek, E.

AU - Eales, S.

AU - Farrah, D.

AU - Schreiber, N. Förster

AU - Fox, M.

AU - Franceschini, A.

AU - Gear, W.

AU - Genzel, R.

AU - Glenn, J.

AU - Griffin, M.

AU - Gruppioni, C.

AU - Halpern, M.

AU - Hatziminaoglou, E.

AU - Ibar, E.

AU - Isaak, K.

AU - Ivison, R. J.

AU - Jeong, W. S.

AU - Lagache, G.

AU - Le Borgne, D.

AU - Le Floc'h, E.

AU - Lee, H. M.

AU - Lee, J. C.

AU - Lee, M. G.

AU - Levenson, L.

AU - Lu, N.

AU - Lutz, D.

AU - Madden, S.

AU - Maffei, B.

AU - Magnelli, B.

AU - Mainetti, G.

AU - Maiolino, R.

AU - Marchetti, L.

AU - Mortier, A. M J

AU - Nguyen, H. T.

AU - Nordon, R.

AU - O'Halloran, B.

AU - Okumura, K.

AU - Oliver, S. J.

AU - Omont, A.

AU - Page, M. J.

AU - Panuzzo, P.

AU - Papageorgiou, A.

AU - Pearson, C. P.

AU - Pérez-Fournon, I.

AU - García, A. M Pérez

AU - Poglitsch, A.

AU - Pohlen, M.

AU - Popesso, P.

AU - Pozzi, F.

AU - Rawlings, J. I.

AU - Rigopoulou, D.

AU - Riguccini, L.

AU - Rizzo, D.

AU - Rodighiero, G.

AU - Roseboom, I. G.

AU - Rowan-Robinson, M.

AU - Saintonge, A.

AU - Portal, M. Sánchez

AU - Santini, P.

AU - Sauvage, M.

AU - Schulz, B.

AU - Scott, D.

AU - Seymour, N.

AU - Shao, L.

AU - Shupe, D. L.

AU - Smith, A. J.

AU - Stevens, J. A.

AU - Sturm, E.

AU - Tacconi, L.

AU - Trichas, M.

AU - Tugwell, K. E.

AU - Vaccari, M.

AU - Valtchanov, I.

AU - Vieira, J. D.

AU - Vigroux, L.

AU - Wang, L.

AU - Ward, R.

AU - Wright, G.

AU - Xu, C. K.

AU - Zemcov, M.

N1 - DOI: 10.1111/j.1365-2966.2010.17645.x; eprintid: arXiv:1009.1058

PY - 2010/11

Y1 - 2010/11

N2 - We study the dust properties of galaxies in the redshift range 0.1 ≲z≲ 2.8 observed by the Herschel Space Observatory in the field of the Great Observatories Origins Deep Survey-North as part of the PACS Extragalactic Probe (PEP) and Herschel Multi-tiered Extragalactic Survey (HerMES) key programmes. Infrared (IR) luminosity (LIR) and dust temperature (Tdust) of galaxies are derived from the spectral energy distribution fit of the far-IR (FIR) flux densities obtained with the PACS and SPIRE instruments onboard Herschel. As a reference sample, we also obtain IR luminosities and dust temperatures of local galaxies at z <0.1 using AKARI and IRAS data in the field of the Sloan Digital Sky Survey. We compare the LIR-Tdust relation between the two samples and find that the median Tdust of Herschel-selected galaxies at z<0.5 with LIR≲ 5 × 1010L· appears to be 2-5 K colder than that of AKARI-selected local galaxies with similar luminosities, and the dispersion in Tdust for high-z galaxies increases with LIR due to the existence of cold galaxies that are not seen among local galaxies. We show that this large dispersion of the LIR-Tdust relation can bridge the gap between local star-forming galaxies and high-z submillimetre galaxies (SMGs). We also find that three SMGs with very low Tdust (≲20 K) covered in this study have close neighbouring sources with similar 24-μm brightness, which could lead to an overestimation of FIR/(sub)millimetre fluxes of the SMGs. © 2010 The Authors. Journal compilation © 2010 RAS.

AB - We study the dust properties of galaxies in the redshift range 0.1 ≲z≲ 2.8 observed by the Herschel Space Observatory in the field of the Great Observatories Origins Deep Survey-North as part of the PACS Extragalactic Probe (PEP) and Herschel Multi-tiered Extragalactic Survey (HerMES) key programmes. Infrared (IR) luminosity (LIR) and dust temperature (Tdust) of galaxies are derived from the spectral energy distribution fit of the far-IR (FIR) flux densities obtained with the PACS and SPIRE instruments onboard Herschel. As a reference sample, we also obtain IR luminosities and dust temperatures of local galaxies at z <0.1 using AKARI and IRAS data in the field of the Sloan Digital Sky Survey. We compare the LIR-Tdust relation between the two samples and find that the median Tdust of Herschel-selected galaxies at z<0.5 with LIR≲ 5 × 1010L· appears to be 2-5 K colder than that of AKARI-selected local galaxies with similar luminosities, and the dispersion in Tdust for high-z galaxies increases with LIR due to the existence of cold galaxies that are not seen among local galaxies. We show that this large dispersion of the LIR-Tdust relation can bridge the gap between local star-forming galaxies and high-z submillimetre galaxies (SMGs). We also find that three SMGs with very low Tdust (≲20 K) covered in this study have close neighbouring sources with similar 24-μm brightness, which could lead to an overestimation of FIR/(sub)millimetre fluxes of the SMGs. © 2010 The Authors. Journal compilation © 2010 RAS.

KW - Galaxies: evolution

KW - Galaxies: formation

KW - Galaxies: general

KW - Galaxies: high-redshift

KW - Galaxies: starburst

KW - Infrared: galaxies

UR - https://www.scopus.com/pages/publications/78149393207

U2 - 10.1111/j.1365-2966.2010.17645.x

DO - 10.1111/j.1365-2966.2010.17645.x

M3 - Article

SN - 1365-2966

VL - 409

SP - 75

EP - 82

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

Evolution of dust temperature of galaxies through cosmic time as seen by Herschel

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