Planck intermediate results III : The relation between galaxy cluster mass and Sunyaev-Zeldovich signal (Articolo in rivista)

Type
Label
  • Planck intermediate results III : The relation between galaxy cluster mass and Sunyaev-Zeldovich signal (Articolo in rivista) (literal)
Anno
  • 2013-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.1051/0004-6361/201219398 (literal)
Alternative label
  • Ade P. A. R.; Aghanim N.; Arnaud M.; Ashdown M.; Atrio-Barandela F.; Aumont J.; Baccigalupi C.; Balbi A.; Banday A. J.; Barreiro R. B.; Bartlett J.G.; Battaner E.; Battye R.; Benabed K.; Bernard J.-P.; Bersanelli M.; Bathia R.; Bikmaev I.; Bohringer H.; Bonaldi A.; Bond J.R.; Borgani S.; Borrill J.; Bouchet F. R.; Bourdin H.; Brown M.L.; Bucher M.; Burenin R.; Burigana C.; Butler R. C.; Cabella P.; Cardoso J.F.; Carvalho P.; Chamballu A.; Chiang L.-Y.; Chon G.; Clements D.; Colafrancesco S.; Coulais A.; Cuttaia F.; da Silva P.; Dahel H.; Davis R. J.; de Bernardis P.; de Gasperis G.; Delabrouille J.; Democles J.; Desert F.X.; ; Diego J.M.; Dolag K.; Dole H.; Donzelli S.; Dorè O.; Douspis M.; Dupac X.; Efstathiou G.; Enßlin T. A.; Eriksen H. K.; Finelli F.; Flores-Cacho I.; Forni O.; Frailis M.; Franceschi E.; Frommert M.; Galeotta S.; Ganga K.; Genova-Santos R.T.; Giard M.; Giraud-Heraud Y.; Gonzales-Nuevo J.; Górski K. M.; Gregorio A.; Gruppuso A.; Hansen F. K.; Harrison D.; Hernández-Monteagudo C.; Herranz D.; Hildebrandt S. R.; Hivon E.; Hobson M.; Holmes W.A.; Huffenberger K. M.; Hurier G.; Jagemann T.; Juvela M.; Keihänen E.; Khamitov I.; Kneissl R.; Knoche J.; Kunz M.; Kurki-Suonio H.; Lagache G.; Lamarre J.-M.; Lasenby A.; Lawrence C.R.; Le Jeune M.; Leach S.; Leonardi R.; Liddle A.; Lilje P. B.; Linden-Vornle M.; Lopez-Caniego M.; Luzzi G.; Macias-Perez J. F.; Maino D.; Mandolesi N.; Maris M.; Marleau F.; Marshall D.J.; Martinez-Gonzalez E.; Masi S.; Matarrese S.; Matthai F.; Mazzotta P.; Meinhold P. R.; Melchiorri A.; Mélin J.-B.; Mendes L.; Mitra S.; Miville-Deschenes M.-A.; Montier L.; Morgante G.; Munshi D.; Natoli P.; Nørgaard-Nielsen H. U.; Noviello F.; Osborne S.; Pajot F.; Paoletti D.; Partridge B.; Pearson T.J.; Perdereau O.; Perrotta F.; Piacentini F.; Piat M.; Pierpaoli E.; Piffaretti R.; Platania P.; Pointecouteau E.; Polenta G.; Ponthieu N.; Popa L.; Poutanen T.; Pratt G.W.; Prunet S.; Puget J.-L.; Rachen J. P.; Rebolo R.; Reinecke M.; Remazeilles M.; Renault C.; Ricciardi S.; Ristorcelli I.; Rocha G.; Rosset C.; Rossetti M.; Rubino-Martin J.A.; Rusholme B.; Sandri M.; Savini G.; Scott D.; Starck J.-L.; Stivoli F.; Stolyarov V.; Sudiwala R.; Sunyaev R.; Sutton D.; Suur-Uski A.S.; Sygnet J.-F.; Tauber J. A.; Terenzi L.; Toffolatti L.; Tomasi M.; Tristram M.; Valenziano L.; Van Tent B.; Vielva P.; Villa F.; Vittorio N.; Wandelt B. D.; Weller J.; White S.D.M.; Yvon D.; Zacchei A.; Zonca A. (2013)
    Planck intermediate results III : The relation between galaxy cluster mass and Sunyaev-Zeldovich signal
    in Astronomy & astrophysics (Online); EDP Sciences, Les Ulis Cedex (Francia)
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Ade P. A. R.; Aghanim N.; Arnaud M.; Ashdown M.; Atrio-Barandela F.; Aumont J.; Baccigalupi C.; Balbi A.; Banday A. J.; Barreiro R. B.; Bartlett J.G.; Battaner E.; Battye R.; Benabed K.; Bernard J.-P.; Bersanelli M.; Bathia R.; Bikmaev I.; Bohringer H.; Bonaldi A.; Bond J.R.; Borgani S.; Borrill J.; Bouchet F. R.; Bourdin H.; Brown M.L.; Bucher M.; Burenin R.; Burigana C.; Butler R. C.; Cabella P.; Cardoso J.F.; Carvalho P.; Chamballu A.; Chiang L.-Y.; Chon G.; Clements D.; Colafrancesco S.; Coulais A.; Cuttaia F.; da Silva P.; Dahel H.; Davis R. J.; de Bernardis P.; de Gasperis G.; Delabrouille J.; Democles J.; Desert F.X.; ; Diego J.M.; Dolag K.; Dole H.; Donzelli S.; Dorè O.; Douspis M.; Dupac X.; Efstathiou G.; Enßlin T. A.; Eriksen H. K.; Finelli F.; Flores-Cacho I.; Forni O.; Frailis M.; Franceschi E.; Frommert M.; Galeotta S.; Ganga K.; Genova-Santos R.T.; Giard M.; Giraud-Heraud Y.; Gonzales-Nuevo J.; Górski K. M.; Gregorio A.; Gruppuso A.; Hansen F. K.; Harrison D.; Hernández-Monteagudo C.; Herranz D.; Hildebrandt S. R.; Hivon E.; Hobson M.; Holmes W.A.; Huffenberger K. M.; Hurier G.; Jagemann T.; Juvela M.; Keihänen E.; Khamitov I.; Kneissl R.; Knoche J.; Kunz M.; Kurki-Suonio H.; Lagache G.; Lamarre J.-M.; Lasenby A.; Lawrence C.R.; Le Jeune M.; Leach S.; Leonardi R.; Liddle A.; Lilje P. B.; Linden-Vornle M.; Lopez-Caniego M.; Luzzi G.; Macias-Perez J. F.; Maino D.; Mandolesi N.; Maris M.; Marleau F.; Marshall D.J.; Martinez-Gonzalez E.; Masi S.; Matarrese S.; Matthai F.; Mazzotta P.; Meinhold P. R.; Melchiorri A.; Mélin J.-B.; Mendes L.; Mitra S.; Miville-Deschenes M.-A.; Montier L.; Morgante G.; Munshi D.; Natoli P.; Nørgaard-Nielsen H. U.; Noviello F.; Osborne S.; Pajot F.; Paoletti D.; Partridge B.; Pearson T.J.; Perdereau O.; Perrotta F.; Piacentini F.; Piat M.; Pierpaoli E.; Piffaretti R.; Platania P.; Pointecouteau E.; Polenta G.; Ponthieu N.; Popa L.; Poutanen T.; Pratt G.W.; Prunet S.; Puget J.-L.; Rachen J. P.; Rebolo R.; Reinecke M.; Remazeilles M.; Renault C.; Ricciardi S.; Ristorcelli I.; Rocha G.; Rosset C.; Rossetti M.; Rubino-Martin J.A.; Rusholme B.; Sandri M.; Savini G.; Scott D.; Starck J.-L.; Stivoli F.; Stolyarov V.; Sudiwala R.; Sunyaev R.; Sutton D.; Suur-Uski A.S.; Sygnet J.-F.; Tauber J. A.; Terenzi L.; Toffolatti L.; Tomasi M.; Tristram M.; Valenziano L.; Van Tent B.; Vielva P.; Villa F.; Vittorio N.; Wandelt B. D.; Weller J.; White S.D.M.; Yvon D.; Zacchei A.; Zonca A. (literal)
Pagina inizio
  • A129 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
  • http://www.aanda.org/articles/aa/abs/2013/02/aa19398-12/aa19398-12.html (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 550 (literal)
Rivista
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • [ 1 ] Univ Paris Diderot, APC, CNRS, CEA,Irfu,Observ Paris,IN2P3, F-75205 Paris 13, France [ 2 ] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland [ 3 ] Acad Sci Tatarstan, Kazan 420111, Republic Of Tat, Russia [ 4 ] ESRIN, Agenzia Spaziale Italiana Sci Data Ctr, Frascati, Italy [ 5 ] Agenzia Spaziale Italiana, Rome, Italy [ 6 ] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England [ 7 ] ALMA Santiago Cent Off, Atacama Large Millimeter Submillimeter Array, Santiago, Chile [ 8 ] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada [ 9 ] CNRS, IRAP, F-31028 Toulouse 4, France [ 10 ] CALTECH, Pasadena, CA 91125 USA [ 11 ] Univ Oslo, Ctr Math Applicat, Oslo, Norway [ 12 ] Univ Porto, Ctr Astrofis, P-4150762 Oporto, Portugal [ 13 ] CEFCA, Teruel 44001, Spain [ 14 ] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA [ 15 ] CSIC, Madrid, Spain [ 16 ] CEA Saclay, SPP, Irfu, DSM, F-91191 Gif Sur Yvette, France [ 17 ] Natl Space Inst, DTU Space, Copenhagen, Denmark [ 18 ] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland [ 19 ] Univ Salamanca, Fac Ciencias, Dept Fis Fundamental, E-37008 Salamanca, Spain [ 20 ] Univ Oviedo, Dept Fis, E-33007 Oviedo, Spain [ 21 ] Kazan Fed Univ, Dept Astron & Geodesy, Kazan 420008, Russia [ 22 ] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, NL-6500 GL Nijmegen, Netherlands [ 23 ] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada [ 24 ] Univ So Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA [ 25 ] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England [ 26 ] Univ Helsinki, Dept Phys, Helsinki, Finland [ 27 ] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA [ 28 ] Univ Illinois, Dept Phys, Urbana, IL USA [ 29 ] Univ Padua, Dipartimento Fis & Astron G Galilei, I-35131 Padua, Italy [ 30 ] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy [ 31 ] Univ Milan, Dipartimento Fis, Milan, Italy [ 32 ] Univ Trieste, Dipartmento Fis, I-34127 Trieste, Italy [ 33 ] Univ Ferrara, Dipartimento Fis, I-44122 Ferrara, Italy [ 34 ] Univ Roma Tor Vergata, Dipartimento Fis, I-00173 Rome, Italy [ 35 ] Univ Roma Tor Vergata, Dipartimento Matemat, I-00133 Rome, Italy [ 36 ] ULL, Dpto Astrofis, Tenerife 38206, Spain [ 37 ] ESO Vitacura, European So Observ, Santiago 19001, Chile [ 38 ] European Space Agcy, ESAC, Planck Sci Off, Madrid, Spain [ 39 ] European Space Agcy, Estec, NL-2201 AZ Noordwijk, Netherlands [ 40 ] Haverford Coll, Dept Astron, Haverford, PA 19041 USA [ 41 ] Univ Helsinki, Helsinki Inst Phys, Helsinki, Finland [ 42 ] INAF Osservatorio Astron Roma, Monte Porzio Catone, Italy [ 43 ] INAF Osservatorio Astron Trieste, Trieste, Italy [ 44 ] INAF IASF Bologna, Bologna, Italy [ 45 ] INAF IASF Milano, Milan, Italy [ 46 ] Univ Roma La Sapienza, Ist Nazl Fis Nucl, Sez Roma 1, I-00185 Rome, Italy [ 47 ] Univ Paris 11, INRIA, Rech Informat Lab, F-91405 Orsay, France [ 48 ] Univ Grenoble 1, CNRS, INSU, IPAG,UMR 5274, F-38041 Grenoble, France [ 49 ] IUCAA, Pune 411007, Maharashtra, India [ 50 ] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England [ 51 ] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA [ 52 ] Inst Univ France, F-75005 Paris, France [ 53 ] Univ Paris 11, CNRS, Inst Astrophys Spatiale, UMR 8617, F-91405 Orsay, France [ 54 ] Inst Astrophys, CNRS, UMR 7095, F-75014 Paris, France [ 55 ] Inst Space Sci, Bucharest, Romania [ 56 ] Univ Innsbruck, Inst Astro & Particle Phys, A-6020 Innsbruck, Austria [ 57 ] Acad Sinica, Inst Astron & Astrophys, Taipei 115, Taiwan [ 58 ] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England [ 59 ] Univ Oslo, Inst Theoret Astrophys, Oslo, Norway [ 60 ] Inst Astrofis Canarias, Tenerife, Spain [ 61 ] Univ Cantabria, CSIC, Inst Fis Cantabria, E-39005 Santander, Spain [ 62 ] CNR ENEA EURATOM Assoc, Ist Fis Plasma, Milan, Italy [ 63 ] CALTECH, Jet Prop Lab, Pasadena, CA USA [ 64 ] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England [ 65 ] Kavli Inst Cosmol Cambridge, Cambridge CB3 0HA, England [ 66 ] Univ Paris 11, CNRS, IN2P3, LAL, F-91405 Orsay, France [ 67 ] Observ Paris, CNRS, LERMA, F-75014 Paris, France [ 68 ] Univ Paris Diderot, Lab AIM, IRFU Serv Astrophys, CEA DSM,CNRS,CEA Saclay, F-91191 Gif Sur Yvette, France [ 69 ] CNRS, Lab Traitement & Commun Informat, UMR 5141, F-75634 Paris 13, France [ 70 ] Telecom ParisTech, F-75634 Paris 13, France [ 71 ] Univ Grenoble 1, Inst Natl Polytech Grenoble, Lab Phys Subat & Cosmol, CNRS,IN2P3, F-38026 St Martin Dheres, France [ 72 ] Univ Paris 11, Phys Theor Lab, F-91405 Orsay, France [ 73 ] CNRS, F-91405 Orsay, France [ 74 ] Max Planck Inst Astrophys, D-85741 Garching, Germany [ 75 ] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany [ 76 ] UCL, Opt Sci Lab, London, England [ 77 ] SISSA, Astrophys Sect, I-34136 Trieste, Italy [ 78 ] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales [ 79 ] Space Res Inst IKI, Moscow, Russia [ 80 ] Russian Acad Sci, Space Res Inst IKI, Moscow 117997, Russia [ 81 ] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA [ 82 ] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Zelenchukskiy R, Russia [ 83 ] Stanford Univ, Dept Phys, Stanford, CA 94305 USA [ 84 ] TUBITAK Natl Observ, TR-0708 Antalya, Turkey [ 85 ] UPMC Univ Paris 06, UMR 7095, F-75014 Paris, France [ 86 ] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France [ 87 ] Univ Munich, Univ Observ, D-81679 Munich, Germany [ 88 ] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, Granada, Spain [ 89 ] Univ Miami, Coral Gables, FL 33124 USA [ 90 ] Univ Warsaw Observ, Warsaw, Poland (literal)
Titolo
  • Planck intermediate results III : The relation between galaxy cluster mass and Sunyaev-Zeldovich signal (literal)
Abstract
  • We examine the relation between the galaxy cluster mass M and Sunyaev-Zeldovich (SZ) effect signal D-A(2) Y-500 for a sample of 19 objects for which weak lensing (WL) mass measurements obtained from Subaru Telescope data are available in the literature. Hydrostatic X-ray masses are derived from XMM-Newton archive data, and the SZ effect signal is measured from Planck all-sky survey data. We find an M-WL-D-A(2) Y-500 relation that is consistent in slope and normalisation with previous determinations using weak lensing masses; however, there is a normalisation offset with respect to previous measures based on hydrostatic X-ray mass-proxy relations. We verify that our SZ effect measurements are in excellent agreement with previous determinations from Planck data. For the present sample, the hydrostatic X-ray masses at R-500 are on average similar to 20 percent larger than the corresponding weak lensing masses, which is contrary to expectations. We show that the mass discrepancy is driven by a difference in mass concentration as measured by the two methods and, for the present sample, that the mass discrepancy and difference in mass concentration are especially large for disturbed systems. The mass discrepancy is also linked to the offset in centres used by the X-ray and weak lensing analyses, which again is most important in disturbed systems. We outline several approaches that are needed to help achieve convergence in cluster mass measurement with X-ray and weak lensing observations. (literal)
Editore
Prodotto di
Autore CNR

Incoming links:


Prodotto
Autore CNR di
Editore di
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#rivistaDi
data.CNR.it