Cold dust and young starbursts: Spectral energy distributions of Herschel SPIRE sources from the HerMES survey

M. Rowan-Robinson; I. G. Roseboom; M. Vaccari; A. Amblard; V. Arumugam; R. Auld; H. Aussel; T. Babbedge; A. Blain; J. Bock; A. Boselli; D. Brisbin; V. Buat; D. Burgarella; N. Castro-Rodriguez; A. Cava; P. Chanial; D. L. Clements; A. Conley; L. Conversi; A. Cooray; C. D. Dowell; E. Dwek; S. Dye; S. Eales; D. Elbaz; D. Farrah; M. Fox; A. Franceschini; W. Gear; J. Glenn; E. A.G. Solares; M. Griffin; M. Halpern; E. Hatziminaoglou; J. Huang; E. Ibar; K. Isaak; R. J. Ivison; G. Lagache; L. Levenson; N. Lu; S. Madden; B. Maffei; G. Mainetti; L. Marchetti; A. M.J. Mortier; H. T. Nguyen; B. O'Halloran; S. J. Oliver; A. Omont; M. J. Page; P. Panuzzo; A. Papageorgiou; H. Patel; C. P. Pearson; I. Perez Fournon; M. Pohlen; J. I. Rawlings; G. Raymond; D. Rigopoulou; D. Rizzo; B. Schulz; Douglas Scott; N. Seymour; D. L. Shupe; A. J. Smith; J. A. Stevens; M. Symeonidis; M. Trichas; K. E. Tugwell; I. Valtchanov; L. Vigroux; L. Wang; R. Ward; G. Wright; C. K. Xu; M. Zemcov

doi:10.1111/j.1365-2966.2010.17041.x

Cold dust and young starbursts: Spectral energy distributions of Herschel SPIRE sources from the HerMES survey

M. Rowan-Robinson
, I. G. Roseboom
, M. Vaccari
, A. Amblard
, V. Arumugam
, R. Auld
, H. Aussel
, T. Babbedge
, A. Blain
, J. Bock
, A. Boselli
, D. Brisbin
, V. Buat
, D. Burgarella
, N. Castro-Rodriguez
, A. Cava
, P. Chanial
, D. L. Clements
, A. Conley
, L. Conversi

A. Cooray, C. D. Dowell, E. Dwek, S. Dye, S. Eales, D. Elbaz, D. Farrah, M. Fox, A. Franceschini, W. Gear, J. Glenn, E. A.G. Solares, M. Griffin, M. Halpern, E. Hatziminaoglou, J. Huang, E. Ibar, K. Isaak, R. J. Ivison, G. Lagache, L. Levenson, N. Lu, S. Madden, B. Maffei, G. Mainetti, L. Marchetti, A. M.J. Mortier, H. T. Nguyen, B. O'Halloran, S. J. Oliver, A. Omont, M. J. Page, P. Panuzzo, A. Papageorgiou, H. Patel, C. P. Pearson, I. Perez Fournon, M. Pohlen, J. I. Rawlings, G. Raymond, D. Rigopoulou, D. Rizzo, B. Schulz, Douglas Scott, N. Seymour, D. L. Shupe, A. J. Smith, J. A. Stevens, M. Symeonidis, M. Trichas, K. E. Tugwell, I. Valtchanov, L. Vigroux, L. Wang, R. Ward, G. Wright, C. K. Xu, M. Zemcov

Imperial College London
University of Sussex
University of Padova
University of California, Irvine
University of Edinburgh, Institute for Astronomy
Cardiff University
Université Paris Diderot
California Institute of Technology
Jet Propulsion Laboratory
Aix-Marseille Université
Cornell University
GTC Project
Universidad de la Laguna
University of Colorado Boulder
European Space Astronomy Centre
NASA Goddard Space Flight Center
Institute of Astronomy
University of British Columbia
ESO
Harvard & Smithsonian
Royal Observatory
Institut d'Astrophysique Spatiale
California Institute of Technology
University of Manchester
UPMC Univ. Paris 06
University College London
Rutherford Appleton Laboratory
University of Lethbridge
University of Oxford
University of Hertfordshire

Research output: Contribution to a Journal (Peer & Non Peer) › Article › peer-review

43 Citations (Scopus)

Abstract

We present spectral energy distributions (SEDs) for 68 Herschel sources detected at 5σ at 250, 350 and 500 μm in the HerMES SWIRE-Lockman field. We explore whether existing models for starbursts, quiescent star-forming galaxies and active galactic nucleus dust tori are able to model the full range of SEDs measured with Herschel. We find that while many galaxies ( 56 per cent) are well fitted with the templates used to fit IRAS, Infrared Space Observatory (ISO) and Spitzer sources, for about half the galaxies two new templates are required: quiescent ('cirrus') models with colder (10-20 K) dust and a young starburst model with higher optical depth than Arp 220. Predictions of submillimetre fluxes based on model fits to 4.5-24 μm data agree rather poorly with the observed fluxes, but the agreement is better for fits to 4.5-70 μm data. Herschel galaxies detected at 500 μm tend to be those with the highest dust masses.

Original language	English
Pages (from-to)	2-11
Number of pages	10
Journal	Monthly Notices of the Royal Astronomical Society
Volume	409
Issue number	1
DOIs	https://doi.org/10.1111/j.1365-2966.2010.17041.x
Publication status	Published - Nov 2010
Externally published	Yes

Keywords

Cosmology: observations
Galaxies: evolution
Galaxies: star formation
Galaxies: starburst
Infrared: galaxies

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10.1111/j.1365-2966.2010.17041.x

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Rowan-Robinson, M., Roseboom, I. G., Vaccari, M., Amblard, A., Arumugam, V., Auld, R., Aussel, H., Babbedge, T., Blain, A., Bock, J., Boselli, A., Brisbin, D., Buat, V., Burgarella, D., Castro-Rodriguez, N., Cava, A., Chanial, P., Clements, D. L., Conley, A., ... Zemcov, M. (2010). Cold dust and young starbursts: Spectral energy distributions of Herschel SPIRE sources from the HerMES survey. Monthly Notices of the Royal Astronomical Society, 409(1), 2-11. https://doi.org/10.1111/j.1365-2966.2010.17041.x

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title = "Cold dust and young starbursts: Spectral energy distributions of Herschel SPIRE sources from the HerMES survey",

abstract = "We present spectral energy distributions (SEDs) for 68 Herschel sources detected at 5σ at 250, 350 and 500 μm in the HerMES SWIRE-Lockman field. We explore whether existing models for starbursts, quiescent star-forming galaxies and active galactic nucleus dust tori are able to model the full range of SEDs measured with Herschel. We find that while many galaxies ( 56 per cent) are well fitted with the templates used to fit IRAS, Infrared Space Observatory (ISO) and Spitzer sources, for about half the galaxies two new templates are required: quiescent ('cirrus') models with colder (10-20 K) dust and a young starburst model with higher optical depth than Arp 220. Predictions of submillimetre fluxes based on model fits to 4.5-24 μm data agree rather poorly with the observed fluxes, but the agreement is better for fits to 4.5-70 μm data. Herschel galaxies detected at 500 μm tend to be those with the highest dust masses.",

keywords = "Cosmology: observations, Galaxies: evolution, Galaxies: star formation, Galaxies: starburst, Infrared: galaxies",

author = "M. Rowan-Robinson and Roseboom, \{I. G.\} and M. Vaccari and A. Amblard and V. Arumugam and R. Auld and H. Aussel and T. Babbedge and A. Blain and J. Bock and A. Boselli and D. Brisbin and V. Buat and D. Burgarella and N. Castro-Rodriguez and A. Cava and P. Chanial and Clements, \{D. L.\} and A. Conley and L. Conversi and A. Cooray and Dowell, \{C. D.\} and E. Dwek and S. Dye and S. Eales and D. Elbaz and D. Farrah and M. Fox and A. Franceschini and W. Gear and J. Glenn and Solares, \{E. A.G.\} and M. Griffin and M. Halpern and E. Hatziminaoglou and J. Huang and E. Ibar and K. Isaak and Ivison, \{R. J.\} and G. Lagache and L. Levenson and N. Lu and S. Madden and B. Maffei and G. Mainetti and L. Marchetti and Mortier, \{A. M.J.\} and Nguyen, \{H. T.\} and B. O'Halloran and Oliver, \{S. J.\} and A. Omont and Page, \{M. J.\} and P. Panuzzo and A. Papageorgiou and H. Patel and Pearson, \{C. P.\} and Fournon, \{I. Perez\} and M. Pohlen and Rawlings, \{J. I.\} and G. Raymond and D. Rigopoulou and D. Rizzo and B. Schulz and Douglas Scott and N. Seymour and Shupe, \{D. L.\} and Smith, \{A. J.\} and Stevens, \{J. A.\} and M. Symeonidis and M. Trichas and Tugwell, \{K. E.\} and I. Valtchanov 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.1365-2966.2010.17041.x",

language = "English",

volume = "409",

pages = "2--11",

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

issn = "0035-8711",

publisher = "Oxford University Press",

number = "1",

}

Rowan-Robinson, M, Roseboom, IG, Vaccari, M, Amblard, A, Arumugam, V, Auld, R, Aussel, H, Babbedge, T, Blain, A, Bock, J, Boselli, A, Brisbin, D, Buat, V, Burgarella, D, Castro-Rodriguez, N, Cava, A, Chanial, P, Clements, DL, Conley, A, Conversi, L, Cooray, A, Dowell, CD, Dwek, E, Dye, S, Eales, S, Elbaz, D, Farrah, D, Fox, M, Franceschini, A, Gear, W, Glenn, J, Solares, EAG, Griffin, M, Halpern, M, Hatziminaoglou, E, Huang, J, Ibar, E, Isaak, K, Ivison, RJ, Lagache, G, Levenson, L, Lu, N, Madden, S, Maffei, B, Mainetti, G, Marchetti, L, Mortier, AMJ, Nguyen, HT, O'Halloran, B, Oliver, SJ, Omont, A, Page, MJ, Panuzzo, P, Papageorgiou, A, Patel, H, Pearson, CP, Fournon, IP, Pohlen, M, Rawlings, JI, Raymond, G, Rigopoulou, D, Rizzo, D, Schulz, B, Scott, D, Seymour, N, Shupe, DL, Smith, AJ, Stevens, JA, Symeonidis, M, Trichas, M, Tugwell, KE, Valtchanov, I, Vigroux, L, Wang, L, Ward, R, Wright, G, Xu, CK & Zemcov, M 2010, 'Cold dust and young starbursts: Spectral energy distributions of Herschel SPIRE sources from the HerMES survey', Monthly Notices of the Royal Astronomical Society, vol. 409, no. 1, pp. 2-11. https://doi.org/10.1111/j.1365-2966.2010.17041.x

TY - JOUR

T1 - Cold dust and young starbursts

T2 - Spectral energy distributions of Herschel SPIRE sources from the HerMES survey

AU - Rowan-Robinson, M.

AU - Roseboom, I. G.

AU - Vaccari, M.

AU - Amblard, A.

AU - Arumugam, V.

AU - Auld, R.

AU - Aussel, H.

AU - Babbedge, T.

AU - Blain, A.

AU - Bock, J.

AU - Boselli, A.

AU - Brisbin, D.

AU - Buat, V.

AU - Burgarella, D.

AU - Castro-Rodriguez, N.

AU - Cava, A.

AU - Chanial, P.

AU - Clements, D. L.

AU - Conley, A.

AU - Conversi, L.

AU - Cooray, A.

AU - Dowell, C. D.

AU - Dwek, E.

AU - Dye, S.

AU - Eales, S.

AU - Elbaz, D.

AU - Farrah, D.

AU - Fox, M.

AU - Franceschini, A.

AU - Gear, W.

AU - Glenn, J.

AU - Solares, E. A.G.

AU - Griffin, M.

AU - Halpern, M.

AU - Hatziminaoglou, E.

AU - Huang, J.

AU - Ibar, E.

AU - Isaak, K.

AU - Ivison, R. J.

AU - Lagache, G.

AU - Levenson, L.

AU - Lu, N.

AU - Madden, S.

AU - Maffei, B.

AU - Mainetti, G.

AU - Marchetti, L.

AU - Mortier, A. M.J.

AU - Nguyen, H. T.

AU - O'Halloran, B.

AU - Oliver, S. J.

AU - Omont, A.

AU - Page, M. J.

AU - Panuzzo, P.

AU - Papageorgiou, A.

AU - Patel, H.

AU - Pearson, C. P.

AU - Fournon, I. Perez

AU - Pohlen, M.

AU - Rawlings, J. I.

AU - Raymond, G.

AU - Rigopoulou, D.

AU - Rizzo, D.

AU - Schulz, B.

AU - Scott, Douglas

AU - Seymour, N.

AU - Shupe, D. L.

AU - Smith, A. J.

AU - Stevens, J. A.

AU - Symeonidis, M.

AU - Trichas, M.

AU - Tugwell, K. E.

AU - Valtchanov, I.

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 present spectral energy distributions (SEDs) for 68 Herschel sources detected at 5σ at 250, 350 and 500 μm in the HerMES SWIRE-Lockman field. We explore whether existing models for starbursts, quiescent star-forming galaxies and active galactic nucleus dust tori are able to model the full range of SEDs measured with Herschel. We find that while many galaxies ( 56 per cent) are well fitted with the templates used to fit IRAS, Infrared Space Observatory (ISO) and Spitzer sources, for about half the galaxies two new templates are required: quiescent ('cirrus') models with colder (10-20 K) dust and a young starburst model with higher optical depth than Arp 220. Predictions of submillimetre fluxes based on model fits to 4.5-24 μm data agree rather poorly with the observed fluxes, but the agreement is better for fits to 4.5-70 μm data. Herschel galaxies detected at 500 μm tend to be those with the highest dust masses.

AB - We present spectral energy distributions (SEDs) for 68 Herschel sources detected at 5σ at 250, 350 and 500 μm in the HerMES SWIRE-Lockman field. We explore whether existing models for starbursts, quiescent star-forming galaxies and active galactic nucleus dust tori are able to model the full range of SEDs measured with Herschel. We find that while many galaxies ( 56 per cent) are well fitted with the templates used to fit IRAS, Infrared Space Observatory (ISO) and Spitzer sources, for about half the galaxies two new templates are required: quiescent ('cirrus') models with colder (10-20 K) dust and a young starburst model with higher optical depth than Arp 220. Predictions of submillimetre fluxes based on model fits to 4.5-24 μm data agree rather poorly with the observed fluxes, but the agreement is better for fits to 4.5-70 μm data. Herschel galaxies detected at 500 μm tend to be those with the highest dust masses.

KW - Cosmology: observations

KW - Galaxies: evolution

KW - Galaxies: star formation

KW - Galaxies: starburst

KW - Infrared: galaxies

UR - https://www.scopus.com/pages/publications/78149366397

U2 - 10.1111/j.1365-2966.2010.17041.x

DO - 10.1111/j.1365-2966.2010.17041.x

M3 - Article

SN - 0035-8711

VL - 409

SP - 2

EP - 11

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

Cold dust and young starbursts: Spectral energy distributions of Herschel SPIRE sources from the HerMES survey

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Keywords

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