| Issue |
A&A
Volume 558, October 2013
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 3 | |
| Section | Cosmology (including clusters of galaxies) | |
| DOI | https://doi.org/10.1051/0004-6361/201220040e | |
| Published online | 17 October 2013 | |
Planck intermediate results (Corrigendum)
V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect
1 APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10 rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
2 Aalto University Metsähovi Radio Observatory, Metsähovintie 114, 02540 Kylmälä, Finland
3 Academy of Sciences of Tatarstan, Bauman Str. 20, Kazan 420111, Republic of Tatarstan, Russia
4 Agenzia Spaziale Italiana Science Data Center, c/o ESRIN, via Galileo Galilei, Frascati, Italy
5 Agenzia Spaziale Italiana, Viale Liegi 26, Roma, Italy
6 Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge CB3 0HE, UK
7 Atacama Large Millimeter/submillimeter Array, ALMA Santiago Central Offices, Alonso de Cordova 3107, Vitacura, Casilla 763 0355, Santiago, Chile
8 CITA, University of Toronto, 60 St. George St., Toronto, ON M5S 3H8, Canada
9 CNRS, IRAP, 9 Av. colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France
10 California Institute of Technology, Pasadena, California, USA
11 Centre of Mathematics for Applications, University of Oslo, Blindern, Oslo, Norway
12 Centro de Astrofísica, Universidade doPorto, Rua das Estrelas, 4150-762 Porto, Portugal
13 Centro de Estudios de Física del Cosmos de Aragón (CEFCA), Plaza San Juan, 1 planta 2, 44001 Teruel, Spain
14 Computational Cosmology Center, Lawrence Berkeley National Laboratory, Berkeley, California, USA
15 Consejo Superior de Investigaciones Científicas (CSIC), Madrid, Spain
16 DSM/Irfu/SPP, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
17 DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark
18 Département de Physique Théorique, Université de Genève, 24 Quai E. Ansermet, 1211 Genève 4, Switzerland
19 Departamento de Física Fundamental, Facultad de Ciencias, Universidad de Salamanca, 37008 Salamanca, Spain
20 Departamento de Física, Universidad de Oviedo, Avda. Calvo Sotelo s/n, Oviedo, Spain
21 Department of Astronomy and Geodesy, Kazan Federal University, Kremlevskaya Str. 18, 420008 Kazan, Russia
22 Department of Astrophysics, IMAPP, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands
23 Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada
24 Department of Physics and Astronomy, Dana and David Dornsife College of Letter, Arts and Sciences, University of Southern California, Los Angeles, CA 90089, USA
25 Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UK
26 Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, Helsinki, Finland
27 Department of Physics, Princeton University, Princeton, New Jersey, USA
28 Department of Physics, University of California, Berkeley, California, USA
29 Department of Physics, University of California, One Shields Avenue, Davis, California, USA
30 Department of Physics, University of California, Santa Barbara, California, USA
31 Department of Physics, University of Illinois at Urbana-Champaign, 1110 West Green Street, Urbana, Illinois, USA
32 Department of Statistics, Purdue University, 250 N. University Street, West Lafayette, Indiana, USA
33 Dipartimento di Fisica e Astronomia G. Galilei, Università degli Studi di Padova, via Marzolo 8, 35131 Padova, Italy
34 Dipartimento di Fisica, Università La Sapienza, P. le A. Moro 2, Roma, Italy
35 Dipartimento di Fisica, Università degli Studi di Milano, via Celoria 16, Milano, Italy
36 Dipartimento di Fisica, Università degli Studi di Trieste, via A. Valerio 2, Trieste, Italy
37 Dipartimento di Fisica, Università di Ferrara, via Saragat 1, 44122 Ferrara, Italy
38 Dipartimento di Fisica, Università di Roma Tor Vergata, via della Ricerca Scientifica 1, Roma, Italy
39 Dipartimento di Matematica, Università di Roma Tor Vergata, via della Ricerca Scientifica 1, Roma, Italy
40 Discovery Center, Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
41 Dpto. Astrofísica, Universidad de La Laguna (ULL), 38206 La Laguna, Tenerife, Spain
42 European Southern Observatory, ESO Vitacura, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile
43 European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la Cañada, Madrid, Spain
44 European Space Agency, ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
45 GEPI, Observatoire de Paris, Section de Meudon, 5 Place J. Janssen, 92195 Meudon Cedex, France
46 Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland
47 INAF – Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, Padova, Italy
48 INAF – Osservatorio Astronomico di Roma, via di Frascati 33, Monte Porzio Catone, Italy
49 INAF – Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, Trieste, Italy
50 INAF Istituto di Radioastronomia, via P. Gobetti 101, 40129 Bologna, Italy
51 INAF/IASF Bologna, via Gobetti 101, Bologna, Italy
52 INAF/IASF Milano, via E. Bassini 15, Milano, Italy
53 INFN, Sezione di Roma 1, Universit‘a di Roma Sapienza, Piazzale Aldo Moro 2, 00185, Roma, Italy
54 IPAG: Institut de Planétologie et d’Astrophysique de Grenoble, Université Joseph Fourier, Grenoble 1/CNRS-INSU, UMR 5274, 38041 Grenoble, France
55 IUCAA, Post Bag 4, Ganeshkhind, Pune University Campus, Pune 411 007, India
56 Imperial College London, Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, UK
57 Infrared Processing and Analysis Center,California Institute of Technology, Pasadena, CA 91125, USA
58 Institut Néel, CNRS, Université Joseph Fourier Grenoble I, 25 rue des Martyrs, Grenoble, France
59 Institut Universitaire de France, 103 bd Saint-Michel, 75005 Paris, France
60 Institut d’Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
61 Institut d’Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, 75014 Paris, France
62 Institut de Ciències de l’Espai, CSIC/IEEC, Facultat de Ciències, Campus UAB, Torre C5 par-2, Bellaterra 08193, Spain
63 Institute for Space Sciences, Bucharest-Magurale, Romania
64 Institute of Astro and Particle Physics, Technikerstrasse 25/8, University of Innsbruck, 6020 Innsbruck, Austria
65 Institute of Astronomy and Astrophysics, Academia Sinica, Taipei, Taiwan
66 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
67 Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
68 Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, La Laguna, Tenerife, Spain
69 Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avda. de los Castros s/n, Santander, Spain
70 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
71 Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, UK
72 Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
73 LAL, Université Paris-Sud, CNRS/IN2P3, Orsay, France
74 LERMA, CNRS, Observatoire de Paris, 61 avenue de l’Observatoire, Paris, France
75 Laboratoire AIM, IRFU/Service d’Astrophysique – CEA/DSM – CNRS – Université Paris Diderot, Bât. 709, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
76 Laboratoire Traitement et Communication de l’Information, CNRS (UMR 5141) and Télécom ParisTech, 46 rue Barrault, 75634 Paris Cedex 13, France
77 Laboratoire de Physique Subatomique et de Cosmologie, Université Joseph Fourier Grenoble I, CNRS/IN2P3, Institut National Polytechnique de Grenoble, 53 rue des Martyrs, 38026 Grenoble Cedex, France
78 Laboratoire de Physique Théorique, Université Paris-Sud 11 & CNRS, Bâtiment 210, 91405 Orsay, France
79 Lawrence Berkeley National Laboratory, Berkeley, California, USA
80 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
81 Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstraße, 85748 Garching, Germany
82 MilliLab, VTT Technical Research Centre of Finland, Tietotie 3, Espoo, Finland
83 National University of Ireland, Department of Experimental Physics, Maynooth, Co. Kildare, Ireland
84 Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
85 Observational Cosmology, Mail Stop 367-17, California Institute of Technology, Pasadena, CA 91125, USA
86 Optical Science Laboratory, University College London, Gower Street, London, UK
87 SISSA, Astrophysics Sector, via Bonomea 265, 34136 Trieste, Italy
88 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
89 Space Research Institute (IKI), Profsoyuznaya 84/32, Moscow, Russia
90 Space Research Institute (IKI), Russian Academy of Sciences, Profsoyuznaya Str 84/32, Moscow 117997, Russia
91 Space Sciences Laboratory, University of California, Berkeley, California, USA
92 Stanford University, Dept of Physics, Varian Physics Bldg, 382 via Pueblo Mall, Stanford, California, USA
93 TÜBİTAK National Observatory, Akdeniz University Campus, 07058, Antalya, Turkey
94 UPMC Univ Paris 06, UMR7095, 98 bis Boulevard Arago, 75014 Paris, France
95 Université Denis Diderot (Paris 7), 75205 Paris Cedex 13, France
96 Université de Toulouse, UPS-OMP, IRAP, 31028 Toulouse Cedex 4, France
97 Universities Space Research Association, Stratospheric Observatory for Infrared Astronomy, MS 211-3, Moffett Field, CA 94035, USA
98 University Observatory, Ludwig Maximilian University of Munich, Scheinerstrasse 1, 81679 Munich, Germany
99 University of Granada, Departamento de Física Teórica y del Cosmos, Facultad de Ciencias, Granada, Spain
100 Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland
Key words: cosmology: observations / galaxies: clusters: general / galaxies: clusters: intracluster medium / submillimeter: general / X-rays: general / errata, addenda
Figure 7 of our original publication (Planck Collaboration 2013) is flawed. The correct figure is presented here and we stress that our original conclusion on the radial distribution of the gas fraction remains unchanged.
There was an error in the reconstruction of the temperature profiles used to derive the gas mass distribution from the joint Planck and XMM-Newton pressure profile, and thereby a prediction for the gas fraction profiles. The error in the temperature profile reconstruction applies to this paper only. The predicted gas fraction profiles for both hypothesis on the temperature profiles, i.e., from hypothesis H1 and H2, were affected similarly. Now corrected, they are in better agreement at R500 with the measurement by Pratt et al. (2009) on the REXCESS sample and with the expectations from the CMB. The Perseus profile (Simionescu et al. 2011) is still marginally compatible with our prediction within our large dispersion (shaded blue and red area on the figure).
 |
Fig. 7 Gas mass fraction profile derived from the combined Planck and XMM-Newton pressure profile, assuming for the temperature profile: (H1) the average best fit model across the sample from X-ray spectroscopy (red line and striped area); or (H2) the same but extrapolating beyond R500 to a constant value equal to the average temperature measured in the last radial bin across the sample (blue line and striped area). The green dashed curve marks the expected gas fraction profile assuming the A10 pressure profile and kT(r) as in hypothesis (1). The star gives fgas(r = R500) for REXCESS clusters with M500 > 5 × 1014 M⊙ (Pratt et al. 2009). In maroon we reproduce the gas mass fraction profile derived from Suzaku measurements for the Perseus cluster (Simionescu et al. 2011). The solid and dashed black lines mark the cosmic baryon fraction expected from CMB measurements (Komatsu et al. 2011) and the expected gas fraction, assuming that 12% of baryons are in stars, respectively. The shaded blue and red areas translate the dispersion in the pressure profile across the ESZ–XMM sample as shown on Fig. 4 in our original paper, assuming hypothesis (H1) for kT(r). See Sect. 7.3 in Planck Collaboration (2013) |
References
- Komatsu, E., Smith, K. M., Dunkley, J., et al. 2011, ApJS, 192, 18 [NASA ADS] [CrossRef] [Google Scholar]
- Planck Collaboration 2013, A&A, 550, A131 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Pratt, G. W., Croston, J. H., Arnaud, M., & Böhringer, H. 2009, A&A, 498, 361 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Simionescu, A., Allen, S. W., Mantz, A., et al. 2011, Science, 331, 1576 [NASA ADS] [CrossRef] [Google Scholar]
© ESO, 2013
All Figures
|
Fig. 7 Gas mass fraction profile derived from the combined Planck and XMM-Newton pressure profile, assuming for the temperature profile: (H1) the average best fit model across the sample from X-ray spectroscopy (red line and striped area); or (H2) the same but extrapolating beyond R500 to a constant value equal to the average temperature measured in the last radial bin across the sample (blue line and striped area). The green dashed curve marks the expected gas fraction profile assuming the A10 pressure profile and kT(r) as in hypothesis (1). The star gives fgas(r = R500) for REXCESS clusters with M500 > 5 × 1014 M⊙ (Pratt et al. 2009). In maroon we reproduce the gas mass fraction profile derived from Suzaku measurements for the Perseus cluster (Simionescu et al. 2011). The solid and dashed black lines mark the cosmic baryon fraction expected from CMB measurements (Komatsu et al. 2011) and the expected gas fraction, assuming that 12% of baryons are in stars, respectively. The shaded blue and red areas translate the dispersion in the pressure profile across the ESZ–XMM sample as shown on Fig. 4 in our original paper, assuming hypothesis (H1) for kT(r). See Sect. 7.3 in Planck Collaboration (2013) |
| In the text | |
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.