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Evidence of Galaxy Cluster Motions with the Kinematic Sunyaev-Zel’dovich Effect

Author(s): Hand, Nick; Addison, Graeme E.; Aubourg, Eric; Battaglia, Nick; Battistelli, Elia S; et al

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dc.contributor.authorHand, Nick-
dc.contributor.authorAddison, Graeme E.-
dc.contributor.authorAubourg, Eric-
dc.contributor.authorBattaglia, Nick-
dc.contributor.authorBattistelli, Elia S-
dc.contributor.authorBizyaev, Dmitry-
dc.contributor.authorBond, J Richard-
dc.contributor.authorBrewington, Howard-
dc.contributor.authorBrinkmann, Jon-
dc.contributor.authorBrown, Benjamin R-
dc.contributor.authorDas, Sudeep-
dc.contributor.authorDawson, Kyle S-
dc.contributor.authorDevlin, Mark J-
dc.contributor.authorDunkley, Joanna-
dc.contributor.authorDünner Planella, Rolando-
dc.contributor.authorEisenstein, Daniel J.-
dc.contributor.authorFowler, Joseph W-
dc.contributor.authorGralla, Megan B-
dc.contributor.authorHajian, Amir-
dc.contributor.authorHalpern, Mark-
dc.contributor.authorHilton, Matt-
dc.contributor.authorHincks, Adam D-
dc.contributor.authorHlozek, Renee-
dc.contributor.authorHughes, John P-
dc.contributor.authorInfante, Leopoldo-
dc.contributor.authorIrwin, Kent D-
dc.contributor.authorKosowsky, Arthur-
dc.contributor.authorLin, Yen-Ting-
dc.contributor.authorMalanushenko, Elena-
dc.contributor.authorMalanushenko, Viktor-
dc.contributor.authorMarriage, Tobias A-
dc.contributor.authorMarsden, Danica-
dc.contributor.authorMenanteau, Felipe-
dc.contributor.authorMoodley, Kavilan-
dc.contributor.authorNiemack, Michael D-
dc.contributor.authorNolta, Michael R-
dc.contributor.authorOravetz, Daniel-
dc.contributor.authorPage Jr, Lyman A.-
dc.contributor.authorPalanque-Delabrouille, Nathalie-
dc.contributor.authorPan, Kaike-
dc.contributor.authorReese, Erik D-
dc.contributor.authorSchlegel, David J-
dc.contributor.authorSchneider, Donald P-
dc.contributor.authorSehgal, Neelima-
dc.contributor.authorShelden, Alaina-
dc.contributor.authorSievers, Jon-
dc.contributor.authorSifon, Cristobal-
dc.contributor.authorSimmons, Audrey-
dc.contributor.authorSnedden, Stephanie-
dc.contributor.authorSpergel, David N.-
dc.contributor.authorStaggs, Suzanne T.-
dc.contributor.authorSwetz, Daniel S-
dc.contributor.authorSwitzer, Eric R.-
dc.contributor.authorTrac, Hy-
dc.contributor.authorWeaver, Benjamin A.-
dc.contributor.authorWollack, Edward J.-
dc.contributor.authorYèche, Christophe-
dc.contributor.authorZunckel, Caroline-
dc.date.accessioned2018-07-20T15:09:23Z-
dc.date.available2018-07-20T15:09:23Z-
dc.date.issued2012-07-27en_US
dc.identifier.citationHand, Nick, Addison, Graeme E, Aubourg, Eric, Battaglia, Nick, Battistelli, Elia S, Bizyaev, Dmitry, Bond, J Richard, Brewington, Howard, Brinkmann, Jon, Brown, Benjamin R, Das, Sudeep, Dawson, Kyle S, Devlin, Mark J, Dunkley, Joanna, Dunner, Rolando, Eisenstein, Daniel J, Fowler, Joseph W, Gralla, Megan B, Hajian, Amir, Halpern, Mark, Hilton, Matt, Hincks, Adam D, Hlozek, Renee, Hughes, John P, Infante, Leopoldo, Irwin, Kent D, Kosowsky, Arthur, Lin, Yen-Ting, Malanushenko, Elena, Malanushenko, Viktor, Marriage, Tobias A, Marsden, Danica, Menanteau, Felipe, Moodley, Kavilan, Niemack, Michael D, Nolta, Michael R, Oravetz, Daniel, Page, Lyman A, Palanque-Delabrouille, Nathalie, Pan, Kaike, Reese, Erik D, Schlegel, David J, Schneider, Donald P, Sehgal, Neelima, Shelden, Alaina, Sievers, Jon, Sifon, Cristobal, Simmons, Audrey, Snedden, Stephanie, Spergel, David N, Staggs, Suzanne T, Swetz, Daniel S, Switzer, Eric R, Trac, Hy, Weaver, Benjamin A, Wollack, Edward J, Yeche, Christophe, Zunckel, Caroline. (2012). Evidence of Galaxy Cluster Motions with the Kinematic Sunyaev-Zel’dovich Effect. PHYSICAL REVIEW LETTERS, 109 (10.1103/PhysRevLett.109.041101en_US
dc.identifier.issn0031-9007-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1md5j-
dc.description.abstractUsing high-resolution microwave sky maps made by the Atacama Cosmology Telescope, we for the first time present strong evidence for motions of galaxy clusters and groups via microwave background temperature distortions due to the kinematic Sunyaev-Zel’dovich effect. Galaxy clusters are identified by their constituent luminous galaxies observed by the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. We measure the mean pairwise momentum of clusters, with a probability of the signal being due to random errors of 0.002, and the signal is consistent with the growth of cosmic structure in the standard model of cosmology.en_US
dc.language.isoenen_US
dc.relation.ispartofPHYSICAL REVIEW LETTERSen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titleEvidence of Galaxy Cluster Motions with the Kinematic Sunyaev-Zel’dovich Effecten_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1103/PhysRevLett.109.041101-
dc.date.eissued2012-07-23en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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