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Journal articles
Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10 11 solar masses
Alexandre Amblard
1
Asantha Cooray
1, 2, *
Paolo Serra
1
B. Altieri
3
V. Arumugam
4
H. Aussel
5
A. Blain
2
J. Bock
2, 6
A. Boselli
7
V. Buat
7
N. Castro-Rodríguez
8
A. Cava
8
P. Chanial
9
E. Chapin
10
D. L. Clements
9
A. Conley
11
L. Conversi
12
C. D. Dowell
6
E. Dwek
13
S. Eales
14
D. Elbaz
5
D. Farrah
15
A. Franceschini
16
W. Gear
14
J. Glenn
11
M. Griffin
14
M. Halpern
10
E. Hatziminaoglou
6
E. Ibar
17
K. Isaak
14
R. J. Ivison
17
A. A. Khostovan
1
Guilaine Lagache
18
L. Levenson
2
N. Lu
19
S. Madden
5
B. Maffei
20
G. Mainetti
16
L. Marchetti
16
G. Marsden
10
K. Mitchell-Wynne
1
H. T. Nguyen
21
B. O'Halloran
9
S. J. Oliver
15
A. Omont
22
M. J. Page
9
P. Panuzzo
5
A. Papageorgiou
6
C. P. Pearson
23
I. Pérez-Fournon
8
M. Pohlen
14
N. Rangwala
11
I. G. Roseboom
24
M. Rowan-Robinson
9
M. Sánchez Portal
3
B. Schulz
19
Douglas Scott
10
N. Seymour
25
D. L. Shupe
6
A. J. Smith
24
J. A. Stevens
26
M. Symeonidis
25
M. Trichas
9
K. Tugwell
27
M. Vaccari
16
E. Valiante
10
I. Valtchanov
3
J. D. Vieira
6
L. Vigroux
22
L. Wang
28
R. Ward
24
Gavin Wright
17
C. K. Xu
6
M. Zemcov
19
*
Corresponding author
28
MOTIVATE - Imagerie et modélisation Vasculaires, Thoraciques et Cérébrales
CREATIS - Centre de Recherche en Acquisition et Traitement de l'Image pour la Santé : 139739
Alexandre Amblard 1
Author
Asantha Cooray 1, 2
Correspondent author
Paolo Serra 1
Author
B. Altieri 3
Author
Guilaine Lagache 18
Author IdHAL : guilaine-lagache
L. Levenson 2
Author
N. Lu 19
Author
S. Madden 5
Author
1
Department of Physics and Astronomy [Irvine] (4129 Frederick Reines Hall, Irvine, CA 92697-4575 - United States)
- UCI - University of California [Irvine] (Irvine, CA 92697 - United States)
- University of California (United States)
2
Department of Astronomy (United States)
- CALTECH - California Institute of Technology (1200 East California Blvd, Pasadena, California 91125 - United States)
3
Herschel Science Centre (Herschel Science Centre, European Space Astronomy Centre, European Space Agency (ESA), Post Office Box 78, 28691 Villanueva de la Cañada, Madrid, Spain - Spain)
- ESA - European Space Agency (France)
4
IfA - Institute for Astronomy [Edinburgh] ( Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ - United Kingdom)
- University of Edinburgh (Old College South Bridge Edinburgh EH8 9YL - United Kingdom)
5
AIM (UMR_7158 / UMR_E_9005 / UM_112) - Astrophysique Interprétation Modélisation (AIM - UMR 7158 - UMR E 9005,
ex "Astrophysique Interactions Multi-échelles",
Service d'astrophysique,
CEA/Saclay,
Orme des Merisiers
F-91191 GIF SUR YVETTE CEDEX - France)
- CNRS - Centre National de la Recherche Scientifique : UMR_7158 (France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- CEA - Commissariat à l'énergie atomique et aux énergies alternatives : UMR_E_9005 (Centre de Saclay Centre de Grenoble Centre de Cadarache etc - France)
- UPD7 - Université Paris Diderot - Paris 7 : UMR_7158 (5 rue Thomas-Mann - 75205 Paris cedex 13 - France)
6
Computing and Mathematical Sciences [Pasadena]] (1200 E California Blvd. MC 305-16, Pasadena, CA 91125 - United States)
- CALTECH - California Institute of Technology (1200 East California Blvd, Pasadena, California 91125 - United States)
7
LAM - Laboratoire d'Astrophysique de Marseille (Pôle de l'Étoile Site de Château-Gombert 38, rue Frédéric Joliot-Curie 13388 Marseille cedex 13 - France)
- AMU - Aix Marseille Université : UMR7326 (Aix-Marseille Université Jardins du Pharo 58 Boulevard Charles Livon 13284 Marseille cedex 7 - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- CNES - Centre National d'Études Spatiales [Toulouse] : UMR7326 (18 avenue Edouard Belin 31401 Toulouse - France)
- CNRS - Centre National de la Recherche Scientifique : UMR7326 (France)
8
IAC - Instituto de Astrofisica de Canarias (Calle Vía Láctea, s/n, 38205 San Cristóbal de La Laguna, Santa Cruz de Tenerife - Spain)
9
Astrophysics Group (Blackett Laboratory, Prince Consort Road, London SW7 2AZ, UK - United Kingdom)
- Blackett Laboratory (Prince Consort Road, South Kensington, London SW7 2AZ - United Kingdom)
- Imperial College London (South Kensington Campus, London SW7 2AZ - United Kingdom)
10
Department of Physics and Astronomy [Vancouver] (6224 Agricultural Road, Vancouver, BC V6T 1Z1 - Canada)
- UBC - University of British Columbia (Vancouver Campus, , 2329 West Mall, Vancouver, BC, V6T 1Z4 / Okanagan Campus, 3333 University Way, Kelowna, BC, V1V 1V7 - Canada)
11
CASA - Center for Astrophysics and Space Astronomy [Boulder] (University of Colorado, 389 UCB, Boulder, CO 80309-0839 - United States)
- University of Colorado [Boulder] (Boulder, Colorado 80309 - United States)
12
Herschel Science Center [Madrid] (Villanueva de la Cañada, E-28691 Madrid - Spain)
- ESAC - European Space Astronomy Centre (Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo,, Villanueva de la Cañada, E-28692 Madrid
- Spain)
- ESA - European Space Agency (France)
13
Observational Cosmology Lab (Code 665, Greenbelt, Maryland 20771, USA - United States)
- GSFC - NASA Goddard Space Flight Center (Greenbelt, MD 20771 - United States)
14
School of Physics and Astronomy [Cardiff] (Queens Buildings The Parade, Cardiff CF24 3AA - United Kingdom)
- Cardiff University (Cardiff Wales CF10 3AT - United Kingdom)
16
Dipartimento di Astronomia [Padova] (Italy)
- Universita degli Studi di Padova (Via 8 Febbraio 2, 35122 Padova - Italy)
17
UK ATC - UK Astronomy Technology Centre (Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ - United Kingdom)
- STFC - Science and Technology Facilities Council (Polaris House, North Star Avenue, Swindon SN2 1SZ - United Kingdom)
18
IAS - Institut d'astrophysique spatiale (bat. 121 91405 ORSAY CEDEX - France)
- UP11 - Université Paris-Sud - Paris 11 (Bâtiment 300 - 91405 Orsay cedex - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8617 (France)
19
CALTECH - California Institute of Technology (1200 East California Blvd, Pasadena, California 91125 - United States)
20
School of Physics and Astronomy (Alan Turing Building, Oxford Road, Manchester M13 9PL, UK - United Kingdom)
- University of Manchester [Manchester] (Oxford Rd, Manchester M13 9PL - United Kingdom)
21
JPL - Jet Propulsion Laboratory (4800 Oak Grove Drive, Pasadena, CA 91109-8099, USA - United States)
- NASA (www.nasa.gov - United States)
- CALTECH - California Institute of Technology (1200 East California Blvd, Pasadena, California 91125 - United States)
22
IAP - Institut d'Astrophysique de Paris (98bis, bd Arago - 75014 Paris France - France)
- CNRS - Centre National de la Recherche Scientifique : UMR7095 (France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- UPMC - Université Pierre et Marie Curie - Paris 6 (4 place Jussieu - 75005 Paris - France)
23
RAL Space - Space Science and Technology Department [Didcot] (Chilton, Didcot OX11 0QX, UK - United Kingdom)
- RAL - STFC Rutherford Appleton Laboratory (Harwell Campus, Didcot OX11 0FA - United Kingdom)
- STFC - Science and Technology Facilities Council (Polaris House, North Star Avenue, Swindon SN2 1SZ - United Kingdom)
25
Space Science & Technology Department (Rutherford Appleton Laboratory, Chilton, Didcot OX11 0QX, UK - United Kingdom)
- Rutheford Appleton Laboratory (France)
26
Centre for Astrophysics Research [Hatfield] (College Lane, Hatfield AL10 9AB, UK - United Kingdom)
- UH - University of Hertfordshire [Hatfield] (De Havilland Campus, Mosquito Way, Hatfield AL10 9EU, UK - United Kingdom)
27
MSSL - Mullard Space Science Laboratory (Holmbury Hill Rd, Dorking RH5 6NT - United Kingdom)
- UCL - University College of London [London] (Gower Street, London WC1E 6BT - United Kingdom)
28
MOTIVATE - Imagerie et modélisation Vasculaires, Thoraciques et Cérébrales (France)
- CREATIS - Centre de Recherche en Acquisition et Traitement de l'Image pour la Santé : 139739 (7 avenue Jean Capelle, Bat Blaise Pascal, 69621 Villeurbanne Cedex - France)
- UCBL - Université Claude Bernard Lyon 1 (43, boulevard du 11 novembre 1918, 69622 Villeurbanne cedex - France)
- Université de Lyon (92 rue Pasteur - CS 30122, 69361 Lyon Cedex 07 - France)
- INSA Lyon - Institut National des Sciences Appliquées de Lyon (20 Avenue Albert Einstein,
69621 Villeurbanne cedex - France)
- Université de Lyon (92 rue Pasteur - CS 30122, 69361 Lyon Cedex 07 - France)
- INSA - Institut National des Sciences Appliquées (France)
- HCL - Hospices Civils de Lyon (3 Quai des Célestins 69002 Lyon - France)
- UJM - Université Jean Monnet [Saint-Étienne] (10 rue Tréfilerie - 42100 Saint-Étienne - France)
- INSERM - Institut National de la Santé et de la Recherche Médicale : U1206 (101, rue de Tolbiac, 75013 Paris - France)
- CNRS - Centre National de la Recherche Scientifique : UMR5220 (France)
- UCBL - Université Claude Bernard Lyon 1 (43, boulevard du 11 novembre 1918, 69622 Villeurbanne cedex - France)
Abstract : The extragalactic background light at far-infrared wavelengths comes from optically faint, dusty, star-forming galaxies in the Universe with star formation rates of a few hundred solar masses per year. These faint, submillimetre galaxies are challenging to study individually because of the relatively poor spatial resolution of far-infrared telescopes. Instead, their average properties can be studied using statistics such as the angular power spectrum of the background intensity variations. A previous attempt at measuring this power spectrum resulted in the suggestion that the clustering amplitude is below the level computed with a simple ansatz based on a halo model. Here we report excess clustering over the linear prediction at arcminute angular scales in the power spectrum of brightness fluctuations at 250, 350 and 500 μm. From this excess, we find that submillimetre galaxies are located in dark matter haloes with a minimum mass, Mmin, such that log10[Mmin/M⊙] = at 350 μm, where M⊙ is the solar mass. This minimum dark matter halo mass corresponds to the most efficient mass scale for star formation in the Universe, and is lower than that predicted by semi-analytical models for galaxy formation
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Journal articles
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https://hal-cea.archives-ouvertes.fr/cea-00904021
Contributor : Bruno Savelli Connect in order to contact the contributor
Submitted on : Tuesday, February 9, 2021 - 2:48:59 PM
Last modification on : Thursday, October 21, 2021 - 5:10:30 AM
Long-term archiving on: : Monday, May 10, 2021 - 6:50:03 PM
Contributor : Bruno Savelli Connect in order to contact the contributor
Submitted on : Tuesday, February 9, 2021 - 2:48:59 PM
Last modification on : Thursday, October 21, 2021 - 5:10:30 AM
Long-term archiving on: : Monday, May 10, 2021 - 6:50:03 PM
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- HAL Id : cea-00904021, version 1
- DOI : 10.1038/nature09771
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CEA | CNRS | UNIV-LYON1 | CEA-DRF | UNIV-ST-ETIENNE | INSA-GROUPE | SORBONNE-UNIVERSITE | SU-SCIENCES | UDL | UNIV-PARIS | IRISA_UBS | UBS | UP-SCIENCES | SU-TI | INSA-LYON | IRFU-AIM | DSM-IRFU | CREATIS | HCL | IAP | INSU | LAM | OSU-INSTITUT-PYTHEAS | UNIV-PARIS7 | UPMC | UNIV-AMU | USPC | INSERM
Citation
Alexandre Amblard, Asantha Cooray, Paolo Serra, B. Altieri, V. Arumugam, et al.. Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10 11 solar masses. Nature, Nature Publishing Group, 2011, 470 (7335), pp.510-512. ⟨10.1038/nature09771⟩. ⟨cea-00904021⟩
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