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Journal articles
Comparison of Sunyaev-Zel’dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters
Y. C. Perrott
1
M. Olamaie
1
C. Rumsey
1
M. L. Brown
F. Feroz
1
K. J. B. Grainge
1
M. P. Hobson
1
A. N. Lasenby
1
C. J. Mactavish
G. G. Pooley
1
R. D. E. Saunders
1
M. P. Schammel
1
P. F. Scott
1
T. W. Shimwell
1
D. J. Titterington
1
E. M. Waldram
1
N. Aghanim
2
M. Arnaud
3
M. Ashdown
1
H. Aussel
3
R. Barrena
I. Bikmaev
H. Böhringer
R. Burenin
P. Carvalho
G. Chon
B. Comis
4
H. Dahle
J. Democles
3
M. Douspis
2
D. Harrison
A. Hempel
G. Hurier
2
I. Khamitov
R. Kneissl
5
J.F. Macías-Pérez
4
J.-B. Melin
6
E. Pointecouteau
7
G. W. Pratt
3
J. A. Rubiño-Martín
V. Stolyarov
1
D. Sutton
J.-B. Melin 6
Author
E. Pointecouteau 7
Author IdHAL : etienne-pointecouteau ORCID : https://orcid.org/0000-0001-8488-3645
G. W. Pratt 3
Author
J. A. Rubiño-Martín
Author
V. Stolyarov 1
Author
D. Sutton
Author
1
Cavendish Laboratory (JJ Thomson Ave, Cambridge CB3 0HE - United Kingdom)
- CAM - University of Cambridge [UK] (The Old Schools, Trinity Lane, Cambridge CB2 1TN - United Kingdom)
2
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)
3
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)
4
LPSC - Laboratoire de Physique Subatomique et de Cosmologie (53 avenue des Martyrs - 38026 Grenoble Cedex - France)
- Grenoble INP - Institut polytechnique de Grenoble - Grenoble Institute of Technology (46 avenue Félix Viallet 38031 Grenoble Cedex 1 - France)
- Institut Polytechnique de Grenoble - Grenoble Institute of Technology (France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- UJF - Université Joseph Fourier - Grenoble 1 (BP 53 - 38041 Grenoble Cedex 9 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR5821 (France)
5
ALMA - Atacama Large Millimeter/submillimeter Array (Santiago - Chile)
- ESO - European Southern Observatory (Karl-Schwarzchild Str. 2 D-85748 Garching bei Munchen - Germany)
6
DPP - Département de Physique des Particules (ex SPP) (France)
- IRFU - Institut de Recherches sur les lois Fondamentales de l'Univers : DRF/IRFU/DPP (CEA Saclay
F-91191 Gif sur Yvette cedex - France)
- CEA - Commissariat à l'énergie atomique et aux énergies alternatives : DRF/IRFU (Centre de Saclay Centre de Grenoble Centre de Cadarache etc - France)
- Université Paris-Saclay (Espace Technologique, Bat. Discovery - RD 128 - 2e ét., 91190 Saint-Aubin - France)
7
IRAP - Institut de recherche en astrophysique et planétologie (9 avenue Colonel Roche 31028 Toulouse - France)
- CNRS - Centre National de la Recherche Scientifique : UMR5277 (France)
- OMP - Observatoire Midi-Pyrénées (14 avenue Edouard Belin, 31400 TOULOUSE - France)
- Météo France (Direction interrégionale - Sud-Est, 2 boulevard Château Double, Aix-en-Provence - France)
- CNES - Centre National d'Études Spatiales [Toulouse] (18 avenue Edouard Belin 31401 Toulouse - France)
- Université Fédérale Toulouse Midi-Pyrénées (41 Allée Jules Guesde, 31000 Toulouse - France)
- CNRS - Centre National de la Recherche Scientifique : UAR 831 (France)
- IRD - Institut de Recherche pour le Développement (Siège Le Sextant 44, bd de Dunkerque CS 90009 13572 Marseille cedex 02 - France)
- UT3 - Université Toulouse III - Paul Sabatier (118 route de Narbonne - 31062 Toulouse - France)
- Université Fédérale Toulouse Midi-Pyrénées (41 Allée Jules Guesde, 31000 Toulouse - France)
- INSU - CNRS - Institut national des sciences de l'Univers : UMR5277 (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
Abstract : We present observations and analysis of a sample of 123 galaxy clusters from the 2013 Planck catalogue of Sunyaev-Zel’dovich sources with the Arcminute Microkelvin Imager (AMI), a ground-based radio interferometer. AMI provides an independent measurement with higher angular resolution, 3 arcmin compared to the Planck beams of 5–10 arcmin. The AMI observations thus provide validation of the cluster detections, improved positional estimates, and a consistency check on the fitted size (θs) and flux (Ytot) parameters in the generalised Navarro, Frenk and White (GNFW) model. We detect 99 of the clusters. We use the AMI positional estimates to check the positional estimates and error-bars produced by the Planck algorithms PowellSnakes and MMF3. We find that Ytot values as measured by AMI are biased downwards with respect to the Planck constraints, especially for high Planck-S/N clusters. We perform simulations to show that this can be explained by deviation from the universal pressure profile shape used to model the clusters. We show that AMI data can constrain the α and β parameters describing the shape of the profile in the GNFW model for individual clusters provided careful attention is paid to the degeneracies between parameters, but one requires information on a wider range of angular scales than are present in AMI data alone to correctly constrain all parameters simultaneously.
Document type :
Journal articles
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https://hal-cea.archives-ouvertes.fr/cea-01383653
Contributor : Edp Sciences <>
Submitted on : Wednesday, October 19, 2016 - 10:08:48 AM
Last modification on : Thursday, September 9, 2021 - 5:33:27 PM
Contributor : Edp Sciences <>
Submitted on : Wednesday, October 19, 2016 - 10:08:48 AM
Last modification on : Thursday, September 9, 2021 - 5:33:27 PM
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aa24188-14.pdf
Publication funded by an institution
Identifiers
- HAL Id : cea-01383653, version 1
- ARXIV : 1405.5013
- DOI : 10.1051/0004-6361/201424188
Collections
CEA | LPSC | CNRS | UNIV-PARIS7 | OMP-IRAP | DSM-IRFU | IRFU-AIM | IN2P3 | OMP | INSU | USPC | CEA-UPSAY | CEA-DRF | UNIV-TLSE3 | UNIV-PARIS | GEPI | UP-SCIENCES | METEO | IRD | UGA | INSTITUT-SCIENCES-LUMIERE
Citation
Y. C. Perrott, M. Olamaie, C. Rumsey, M. L. Brown, F. Feroz, et al.. Comparison of Sunyaev-Zel’dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters. Astronomy and Astrophysics - A&A, EDP Sciences, 2015, 580, pp.A95. ⟨10.1051/0004-6361/201424188⟩. ⟨cea-01383653⟩
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