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-Rodriguez; A. Cava; J. Cepa; P. Chanial; E. Chapin; R. -R. Chary; A. Cimatti; D. L. 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. Foerster 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. Perez-Fournon; A. M. Perez Garcia; 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. Sanchez 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-RodriguezA. Cava, J. Cepa, P. Chanial, E. Chapin, R. -R. Chary, A. Cimatti, D. L. 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. Foerster 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. Perez-Fournon, A. M. Perez Garcia, 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. Sanchez 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

School of Physics and Astronomy

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Abstract / Description of output

We study the dust properties of galaxies in the redshift range 0.1 less than or similar to z less than or similar to 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 (L-IR) and dust temperature (T-dust) 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 L-IR-T-dust relation between the two samples and find that the median T-dust of Herschel-selected galaxies at z greater than or similar to 0.5 with L-IR greater than or similar to 5 x 10(10) L-circle dot appears to be 2-5 K colder than that of AKARI-selected local galaxies with similar luminosities, and the dispersion in T-dust for high-z galaxies increases with L-IR due to the existence of cold galaxies that are not seen among local galaxies. We show that this large dispersion of the L-IR-T-dust 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 T-dust (less than or similar to 20 K) covered in this study have close neighbouring sources with similar 24-mu m brightness, which could lead to an overestimation of FIR/(sub) millimetre fluxes of the SMGs.

Original language	English
Pages (from-to)	75-82
Number of pages	8
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

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10.1111/j.1365-2966.2010.17645.x

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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{9c2e46af4f9d4bcca6fd9ab744bcad73,

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 less than or similar to z less than or similar to 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 (L-IR) and dust temperature (T-dust) 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 L-IR-T-dust relation between the two samples and find that the median T-dust of Herschel-selected galaxies at z greater than or similar to 0.5 with L-IR greater than or similar to 5 x 10(10) L-circle dot appears to be 2-5 K colder than that of AKARI-selected local galaxies with similar luminosities, and the dispersion in T-dust for high-z galaxies increases with L-IR due to the existence of cold galaxies that are not seen among local galaxies. We show that this large dispersion of the L-IR-T-dust 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 T-dust (less than or similar to 20 K) covered in this study have close neighbouring sources with similar 24-mu m brightness, which could lead to an overestimation of FIR/(sub) millimetre fluxes of the SMGs.",

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-Rodriguez and A. Cava and J. Cepa and P. Chanial and E. Chapin and Chary, {R. -R.} and A. Cimatti and Clements, {D. L.} 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. Foerster} 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. Perez-Fournon and {Perez Garcia}, {A. M.} 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 {Sanchez Portal}, M. 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",

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 = "0035-8711",

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-Rodriguez, N, Cava, A, Cepa, J, Chanial, P, Chapin, E, Chary, R-R, Cimatti, A, Clements, DL, 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, W-S, 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, Perez-Fournon, I, Perez Garcia, AM, 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, Sanchez Portal, M, 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-Rodriguez, N.

AU - Cava, A.

AU - Cepa, J.

AU - Chanial, P.

AU - Chapin, E.

AU - Chary, R. -R.

AU - Cimatti, A.

AU - Clements, D. L.

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. Foerster

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 - Perez-Fournon, I.

AU - Perez Garcia, A. M.

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 - Sanchez Portal, M.

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.

PY - 2010/11

Y1 - 2010/11

N2 - We study the dust properties of galaxies in the redshift range 0.1 less than or similar to z less than or similar to 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 (L-IR) and dust temperature (T-dust) 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 L-IR-T-dust relation between the two samples and find that the median T-dust of Herschel-selected galaxies at z greater than or similar to 0.5 with L-IR greater than or similar to 5 x 10(10) L-circle dot appears to be 2-5 K colder than that of AKARI-selected local galaxies with similar luminosities, and the dispersion in T-dust for high-z galaxies increases with L-IR due to the existence of cold galaxies that are not seen among local galaxies. We show that this large dispersion of the L-IR-T-dust 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 T-dust (less than or similar to 20 K) covered in this study have close neighbouring sources with similar 24-mu m brightness, which could lead to an overestimation of FIR/(sub) millimetre fluxes of the SMGs.

AB - We study the dust properties of galaxies in the redshift range 0.1 less than or similar to z less than or similar to 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 (L-IR) and dust temperature (T-dust) 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 L-IR-T-dust relation between the two samples and find that the median T-dust of Herschel-selected galaxies at z greater than or similar to 0.5 with L-IR greater than or similar to 5 x 10(10) L-circle dot appears to be 2-5 K colder than that of AKARI-selected local galaxies with similar luminosities, and the dispersion in T-dust for high-z galaxies increases with L-IR due to the existence of cold galaxies that are not seen among local galaxies. We show that this large dispersion of the L-IR-T-dust 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 T-dust (less than or similar to 20 K) covered in this study have close neighbouring sources with similar 24-mu m brightness, which could lead to an overestimation of FIR/(sub) millimetre fluxes of the SMGs.

UR - http://www.scopus.com/inward/record.url?scp=78149393207&partnerID=8YFLogxK

U2 - 10.1111/j.1365-2966.2010.17645.x

DO - 10.1111/j.1365-2966.2010.17645.x

M3 - Article

SN - 0035-8711

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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