http://www.cnr.it/ontology/cnr/individuo/prodotto/ID226316
Planck intermediate results II : comparison of Sunyaev-Zeldovich measurements from Planck and from the Arcminute Microkelvin Imager for 11 galaxy clusters (Articolo in rivista)
- Type
- Label
- Planck intermediate results II : comparison of Sunyaev-Zeldovich measurements from Planck and from the Arcminute Microkelvin Imager for 11 galaxy clusters (Articolo in rivista) (literal)
- Anno
- 2013-01-01T00:00:00+01:00 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
- 10.1051/0004-6361/201219361 (literal)
- Alternative label
P. A. R. Ade (82); N. Aghanim (56); M. Arnaud (72); M. Ashdown (69); 6; J. Aumont (56); C. Baccigalupi (81); A. Balbi (35); A. J. Banday (90; 9); R. B. Barreiro (65); E. Battaner (92); R. Battye (68); K. Benabed (57; 89); A. Benoît (54); J.-P. Bernard (9); M. Bersanelli (32; 48); R. Bhatia (7); I. Bikmaev (20; 3); H. Böhringer (77); A. Bonaldi (68); J. R. Bond (8); J. Borrill (14; 85); F. R. Bouchet (57; 89); H. Bourdin (35); M. L. Brown (68); M. Bucher (1); R. Burenin (83); C. Burigana (47; 34); R. C. Butler (47); P. Cabella (36); P. Carvalho (6); A. Catalano (73; 71); L. Cayón (29); A. Chamballu (52); R.-R. Chary (53); L.-Y. Chiang (61); G. Chon (77); D. L. Clements (52); S. Colafrancesco (44); S. Colombi (57; 89); A. Coulais (71); B. P. Crill (67; 79); F. Cuttaia (47); A. Da Silva (12); H. Dahle (63); 11; R. D. Davies (68); R. J. Davis (68); P. de Bernardis (31); G. de Gasperis (35); A. de Rosa (47); G. de Zotti (43; 81); J. Delabrouille (1); J. Démoclès (72); C. Dickinson (68); J. M. Diego (65); K. Dolag (91; 76); H. Dole (56; 55); S. Donzelli (48); O. Doré (67; 10); M. Douspis (56); X. Dupac (40); G. Efstathiou (62); T. A. Enßlin (76); H. K. Eriksen (63); F. Feroz (6); F. Finelli (47); I. Flores-Cacho (9; 90); O. Forni (90; 9); P. Fosalba (58); M. Frailis (45); E. Franceschi (47); S. Fromenteau (1; 56); S. Galeotta (45); K. Ganga (1); R. T. Génova-Santos (64); M. Giard (90; 9); Y. Giraud-Héraud (1); J. González-Nuevo (65; 81); K. M. Górski (67; 94); K. J. B. Grainge (6; 69); A. Gregorio (33; 45); A. Gruppuso (47); F. K. Hansen (63); D. Harrison (62; 69); S. Henrot-Versillé (70); C. Hernández-Monteagudo (13;76); D. Herranz (65); S. R. Hildebrandt (10); E. Hivon (57;89); M. Hobson (6); W. A. Holmes (67); K. M. Huffenberger (93); G. Hurier (73); N. Hurley-Walker (6); T. Jagemann (40); M. Juvela (25); E. Keihänen (25); I. Khamitov (88); R. Kneissl (39;7); J. Knoche (76); M. Kunz (18;56); H. Kurki-Suonio (25;42); G. Lagache (56); J.-M. Lamarre (71); A. Lasenby (6;69); C. R. Lawrence (67); M. Le Jeune (1); S. Leach (81); R. Leonardi (40); A. Liddle (24); P. B. Lilje (63;11); M. Linden-Vørnle (17); M. López-Caniego (65); G. Luzzi (70); J. F. Macías-Pérez (73); C. J. MacTavish (69); D. Maino (32;48); N. Mandolesi (47;5); M. Maris (45); F. Marleau (60); D. J. Marshall (72); E. Martínez-González (65); S. Masi (31); M. Massardi (46); S. Matarrese (30); F. Matthai (76); P. Mazzotta (35); P. R. Meinhold (27); A. Melchiorri (31;49); J.-B. Melin (16); L. Mendes (40); A. Mennella (32;48); S. Mitra (51;67); M.-A. Miville-Deschênes (56;8); L. Montier (90;9); G. Morgante (47); D. Munshi (82); P. Naselsky (78;37); P. Natoli (34;4;47); H. U. Nørgaard-Nielsen (17); F. Noviello (68); D. Novikov (52); I. Novikov (78); M. Olamaie (6); S. Osborne (87); F. Pajot (56); D. Paoletti (47); F. Pasian (45); G. Patanchon (1); T. J. Pearson (10;53); O. Perdereau (70); Y. C. Perrott (6); F. Perrotta (81); F. Piacentini (31); E. Pierpaoli (23); P. Platania (66); E. Pointecouteau (90;9); G. Polenta (4;44); L. Popa (59); T. Poutanen (42;25;2); G. W. Pratt (72); J.-L. Puget (56); J. P. Rachen (21;76); R. Rebolo (64;15;38); M. Reinecke (76); M. Remazeilles (56;1); C. Renault (73); S. Ricciardi (47); I. Ristorcelli (90;9); G. Rocha (67;10); C. Rodríguez-Gonzálvez (6); C. Rosset (1); M. Rossetti (32;48); J. A. Rubiño-Martín (64;38); C. Rumsey (6); B. Rusholme (53); M. Sandri (47); R. D. E. Saunders (6;69); G. Savini (80); M. P. Schammel (6); D. Scott (22); T. W. Shimwell (6); G. F. Smoot (26;75;1); J.-L. Starck (72); F. Stivoli (50); V. Stolyarov (6;69;86); R. Sudiwala (82); R. Sunyaev (76;84); D. Sutton (62;69); A.-S. Suur-Uski (25;42); J.-F. Sygnet (57); J. A. Tauber (41); L. Terenzi (47); L. Toffolatti (19;65); M. Tomasi (48); M. Tristram (70); L. Valenziano (47); B. Van Tent (74); P. Vielva (65); F. Villa (47); N. Vittorio (35); L. A. Wade (67); B. D. Wandelt (57;89;28); D. Yvon (16); A. Zacchei (45); and A. Zonca (27) (2013)
Planck intermediate results II : comparison of Sunyaev-Zeldovich measurements from Planck and from the Arcminute Microkelvin Imager for 11 galaxy clusters
in Astronomy & astrophysics (Print); EDP Sciences, Les Ulis Cedex (Francia)
(literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- P. A. R. Ade (82); N. Aghanim (56); M. Arnaud (72); M. Ashdown (69); 6; J. Aumont (56); C. Baccigalupi (81); A. Balbi (35); A. J. Banday (90; 9); R. B. Barreiro (65); E. Battaner (92); R. Battye (68); K. Benabed (57; 89); A. Benoît (54); J.-P. Bernard (9); M. Bersanelli (32; 48); R. Bhatia (7); I. Bikmaev (20; 3); H. Böhringer (77); A. Bonaldi (68); J. R. Bond (8); J. Borrill (14; 85); F. R. Bouchet (57; 89); H. Bourdin (35); M. L. Brown (68); M. Bucher (1); R. Burenin (83); C. Burigana (47; 34); R. C. Butler (47); P. Cabella (36); P. Carvalho (6); A. Catalano (73; 71); L. Cayón (29); A. Chamballu (52); R.-R. Chary (53); L.-Y. Chiang (61); G. Chon (77); D. L. Clements (52); S. Colafrancesco (44); S. Colombi (57; 89); A. Coulais (71); B. P. Crill (67; 79); F. Cuttaia (47); A. Da Silva (12); H. Dahle (63); 11; R. D. Davies (68); R. J. Davis (68); P. de Bernardis (31); G. de Gasperis (35); A. de Rosa (47); G. de Zotti (43; 81); J. Delabrouille (1); J. Démoclès (72); C. Dickinson (68); J. M. Diego (65); K. Dolag (91; 76); H. Dole (56; 55); S. Donzelli (48); O. Doré (67; 10); M. Douspis (56); X. Dupac (40); G. Efstathiou (62); T. A. Enßlin (76); H. K. Eriksen (63); F. Feroz (6); F. Finelli (47); I. Flores-Cacho (9; 90); O. Forni (90; 9); P. Fosalba (58); M. Frailis (45); E. Franceschi (47); S. Fromenteau (1; 56); S. Galeotta (45); K. Ganga (1); R. T. Génova-Santos (64); M. Giard (90; 9); Y. Giraud-Héraud (1); J. González-Nuevo (65; 81); K. M. Górski (67; 94); K. J. B. Grainge (6; 69); A. Gregorio (33; 45); A. Gruppuso (47); F. K. Hansen (63); D. Harrison (62; 69); S. Henrot-Versillé (70); C. Hernández-Monteagudo (13;76); D. Herranz (65); S. R. Hildebrandt (10); E. Hivon (57;89); M. Hobson (6); W. A. Holmes (67); K. M. Huffenberger (93); G. Hurier (73); N. Hurley-Walker (6); T. Jagemann (40); M. Juvela (25); E. Keihänen (25); I. Khamitov (88); R. Kneissl (39;7); J. Knoche (76); M. Kunz (18;56); H. Kurki-Suonio (25;42); G. Lagache (56); J.-M. Lamarre (71); A. Lasenby (6;69); C. R. Lawrence (67); M. Le Jeune (1); S. Leach (81); R. Leonardi (40); A. Liddle (24); P. B. Lilje (63;11); M. Linden-Vørnle (17); M. López-Caniego (65); G. Luzzi (70); J. F. Macías-Pérez (73); C. J. MacTavish (69); D. Maino (32;48); N. Mandolesi (47;5); M. Maris (45); F. Marleau (60); D. J. Marshall (72); E. Martínez-González (65); S. Masi (31); M. Massardi (46); S. Matarrese (30); F. Matthai (76); P. Mazzotta (35); P. R. Meinhold (27); A. Melchiorri (31;49); J.-B. Melin (16); L. Mendes (40); A. Mennella (32;48); S. Mitra (51;67); M.-A. Miville-Deschênes (56;8); L. Montier (90;9); G. Morgante (47); D. Munshi (82); P. Naselsky (78;37); P. Natoli (34;4;47); H. U. Nørgaard-Nielsen (17); F. Noviello (68); D. Novikov (52); I. Novikov (78); M. Olamaie (6); S. Osborne (87); F. Pajot (56); D. Paoletti (47); F. Pasian (45); G. Patanchon (1); T. J. Pearson (10;53); O. Perdereau (70); Y. C. Perrott (6); F. Perrotta (81); F. Piacentini (31); E. Pierpaoli (23); P. Platania (66); E. Pointecouteau (90;9); G. Polenta (4;44); L. Popa (59); T. Poutanen (42;25;2); G. W. Pratt (72); J.-L. Puget (56); J. P. Rachen (21;76); R. Rebolo (64;15;38); M. Reinecke (76); M. Remazeilles (56;1); C. Renault (73); S. Ricciardi (47); I. Ristorcelli (90;9); G. Rocha (67;10); C. Rodríguez-Gonzálvez (6); C. Rosset (1); M. Rossetti (32;48); J. A. Rubiño-Martín (64;38); C. Rumsey (6); B. Rusholme (53); M. Sandri (47); R. D. E. Saunders (6;69); G. Savini (80); M. P. Schammel (6); D. Scott (22); T. W. Shimwell (6); G. F. Smoot (26;75;1); J.-L. Starck (72); F. Stivoli (50); V. Stolyarov (6;69;86); R. Sudiwala (82); R. Sunyaev (76;84); D. Sutton (62;69); A.-S. Suur-Uski (25;42); J.-F. Sygnet (57); J. A. Tauber (41); L. Terenzi (47); L. Toffolatti (19;65); M. Tomasi (48); M. Tristram (70); L. Valenziano (47); B. Van Tent (74); P. Vielva (65); F. Villa (47); N. Vittorio (35); L. A. Wade (67); B. D. Wandelt (57;89;28); D. Yvon (16); A. Zacchei (45); and A. Zonca (27) (literal)
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(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
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(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
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(13) Centro de Estudios de Física del Cosmos de Aragón (CEFCA), Plaza San Juan, 1, planta 2, 44001 Teruel, Spain
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(21) Department of Astrophysics, IMAPP, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands
(22) Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada
(23) Department of Physics and Astronomy, Dana and David Dornsife College of Letter, Arts and Sciences, University of SouthernCalifornia, Los Angeles, CA 90089, USA
(24) Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UK
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(37) Discovery Center, Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
(38) Dpto. Astrofísica, Universidad de La Laguna (ULL), 38206, La Laguna, Tenerife, Spain
(39) European Southern Observatory, ESO Vitacura, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile
(40) European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la Cañada, Madrid, Spain
(41) European Space Agency, ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
(42) Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland
(43) INAF - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, Italy
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(50) INRIA, Laboratoire de Recherche en Informatique, Université Paris-Sud 11, Bâtiment 490, 91405 Orsay Cedex, France
(51) IUCAA, Post Bag 4, Ganeshkhind, Pune University Campus, 411 007 Pune, India
(52) Imperial College London, Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, UK
(53) Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA
(54) Institut Néel, CNRS, Université Joseph Fourier Grenoble I, 25 rue des Martyrs, Grenoble, France
(55) Institut Universitaire de France, 103 bd Saint-Michel, 75005 Paris, France
(56) Institut d'Astrophysique Spatiale, CNRS UMR8617 Université Paris-Sud 11, Bâtiment 121, Orsay, France
(57) Institut d'Astrophysique de Paris, CNRS UMR7095, 98 bis boulevard Arago, 75014 Paris, France
(58) Institut de Ciències de l'Espai, CSIC/IEEC, Facultat de Ciències, Campus UAB, Torre C5 par-2, 08193 Bellaterra, Spain
(59) Institute for Space Sciences, Bucharest-Magurale, Romania
(60) Institute of Astro and Particle Physics, Technikerstrasse 25/8, University of Innsbruck, 6020 Innsbruck, Austria
(61) Institute of Astronomy and Astrophysics, Academia Sinica, Taipei, Taiwan
(62) Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
(63) Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
(64) Instituto de Astrofísica de Canarias, C/vía Láctea s/n, La Laguna, Tenerife, Spain
(65) Instituto de Física de Cantabria, CSIC-Universidad de Cantabria, Avda. de los Castros s/n, Santander, Spain
(66) Istituto di Fisica del Plasma, CNR-ENEA-EURATOM Association, via R. Cozzi 53, Milano, Italy
(67) Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
(68) Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, UK
(69) Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
(70) LAL, Université Paris-Sud, CNRS/IN2P3, Orsay, France
(71) LERMA, CNRS, Observatoire de Paris, 61 Avenue de l'Observatoire, Paris, France
(72) Laboratoire AIM, IRFU/Service d'Astrophysique - CEA/DSM - CNRS - Université Paris Diderot, Bât. 709, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
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(74) Laboratoire de Physique Théorique, Université Paris-Sud 11 & CNRS, Bâtiment 210, 91405 Orsay, France
(75) Lawrence Berkeley National Laboratory, Berkeley, California, USA
(76) Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
(77) Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstraße, 85748 Garching, Germany
(78) Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
(79) Observational Cosmology, Mail Stop 367-17, California Institute of Technology, Pasadena, CA, 91125, USA
(80) Optical Science Laboratory, University College London, Gower Street, London, UK
(81) SISSA, Astrophysics Sector, via Bonomea 265, 34136 Trieste, Italy
(82) School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
(83) Space Research Institute (IKI), Profsoyuznaya 84/32, Moscow, Russia
(84) Space Research Institute (IKI), Russian Academy of Sciences, Profsoyuznaya Str, 84/32, 117997 Moscow, Russia
(85) Space Sciences Laboratory, University of California, Berkeley, California, USA
(86) Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnij Arkhyz, Zelenchukskiy region, 369167 Karachai-Cherkessian Republic, Russia
(87) Stanford University, Dept of Physics, Varian Physics Bldg, 382 via Pueblo Mall, Stanford, California, USA
(88) Tübitak National Observatory, Akdeniz University Campus, 07058 Antalya, Turkey
(89) UPMC Univ. Paris 6, UMR 7095, 98bis boulevard Arago, 75014 Paris, France
(90) Université de Toulouse, UPS-OMP, IRAP, 31028 Toulouse, Cedex 4, France
(91) University Observatory, Ludwig Maximilian University of Munich, Scheinerstrasse 1, 81679 Munich, Germany
(92) University of Granada, Departamento de Física Teórica y del Cosmos, Facultad de Ciencias, Granada, Spain
(93) University of Miami, Knight Physics Building, 1320 Campo Sano Dr., Coral Gables, Florida, USA
(94) Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland (literal)
- Titolo
- Planck intermediate results II : comparison of Sunyaev-Zeldovich measurements from Planck and from the Arcminute Microkelvin Imager for 11 galaxy clusters (literal)
- Abstract
- About half of the baryons of the Universe are expected to be in the form of filaments of hot and low density intergalactic medium. Most of these baryons remain undetected even by the most advanced X-ray observatories which are limited in sensitivity to the diffuse low density medium. The Planck satellite has provided hundreds of detections of the hot gas in clusters of galaxies via the thermal Sunyaev-Zel'dovich (tSZ) effect and is an ideal instrument for studying extended low density media through the tSZ effect. In this paper we use the Planck data to search for signatures of a fraction of these missing baryons between pairs of galaxy clusters. Cluster pairs are good candidates for searching for the hotter and denser phase of the intergalactic medium (which is more easily observed through the SZ effect). Using an X-ray catalogue of clusters and the Planck data, we select physical pairs of clusters as candidates. Using the Planck data we construct a local map of the tSZ effect centered on each pair of galaxy clusters. ROSAT data is used to construct X-ray maps of these pairs. After having modelled and subtracted the tSZ effect and X-ray emission for each cluster in the pair we study the residuals on both the SZ and X-ray maps. For the merging cluster pair A399-A401 we observe a significant tSZ effect signal in the intercluster region beyond the virial radii of the clusters. A joint X-ray SZ analysis allows us to constrain the temperature and density of this intercluster medium. We obtain a temperature of kT = 7.1 +- 0.9, keV (consistent with previous estimates) and a baryon density of (3.7 +- 0.2)x10^-4, cm^-3. The Planck satellite mission has provided the first SZ detection of the hot and diffuse intercluster gas. (literal)
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