4 results on '"Rolando Dünner"'
Search Results
2. Evidence for Dark Energy from the Cosmic Microwave Background Alone Using the Atacama Cosmology Telescope Lensing Measurements
- Author
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Blake D. Sherwin, Joanna Dunkley, Sudeep Das, John W. Appel, J. Richard Bond, C. Sofia Carvalho, Mark J. Devlin, Rolando Dünner, Thomas Essinger-Hileman, Joseph W. Fowler, Amir Hajian, Mark Halpern, Matthew Hasselfield, Adam D. Hincks, Renée Hlozek, John P. Hughes, Kent D. Irwin, Jeff Klein, Arthur Kosowsky, Tobias A. Marriage, Danica Marsden, Kavilan Moodley, Felipe Menanteau, Michael D. Niemack, Michael R. Nolta, Lyman A. Page, Lucas Parker, Erik D. Reese, Benjamin L. Schmitt, Neelima Sehgal, Jon Sievers, David N. Spergel, Suzanne T. Staggs, Daniel S. Swetz, Eric R. Switzer, Robert Thornton, Katerina Visnjic, and Ed Wollack
- Published
- 2011
- Full Text
- View/download PDF
3. Detection of the Power Spectrum of Cosmic Microwave Background Lensing by the Atacama Cosmology Telescope
- Author
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Sudeep Das, Blake D. Sherwin, Paula Aguirre, John W. Appel, J. Richard Bond, C. Sofia Carvalho, Mark J. Devlin, Joanna Dunkley, Rolando Dünner, Thomas Essinger-Hileman, Joseph W. Fowler, Amir Hajian, Mark Halpern, Matthew Hasselfield, Adam D. Hincks, Renée Hlozek, Kevin M. Huffenberger, John P. Hughes, Kent D. Irwin, Jeff Klein, Arthur Kosowsky, Robert H. Lupton, Tobias A. Marriage, Danica Marsden, Felipe Menanteau, Kavilan Moodley, Michael D. Niemack, Michael R. Nolta, Lyman A. Page, Lucas Parker, Erik D. Reese, Benjamin L. Schmitt, Neelima Sehgal, Jon Sievers, David N. Spergel, Suzanne T. Staggs, Daniel S. Swetz, Eric R. Switzer, Robert Thornton, Katerina Visnjic, and Ed Wollack
- Published
- 2011
- Full Text
- View/download PDF
4. Evidence of Galaxy Cluster Motions with the Kinematic Sunyaev-Zel’dovich Effect
- Author
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Rolando Dünner, Michael D. Niemack, Stephanie A. Snedden, Suzanne T. Staggs, Kyle S. Dawson, Michael R. Nolta, J. Richard Bond, Nick Battaglia, Benjamin A. Weaver, Kavilan Moodley, Yen-Ting Lin, David N. Spergel, Jon Brinkmann, Megan Gralla, Sudeep Das, Howard Brewington, Kent D. Irwin, Edward J. Wollack, Erik D. Reese, Elia S. Battistelli, Tobias A. Marriage, Jon Sievers, Joseph W. Fowler, Graeme E. Addison, Kaike Pan, Éric Aubourg, Neelima Sehgal, Dmitry Bizyaev, Amir Hajian, Caroline Zunckel, Lyman A. Page, Arthur Kosowsky, Elena Malanushenko, Christophe Yèche, Daniel Oravetz, Audrey Simmons, Renée Hlozek, Danica Marsden, Mark Halpern, Hy Trac, Mark J. Devlin, Cristóbal Sifón, Felipe Menanteau, Nathalie Palanque-Delabrouille, Nick Hand, Leopoldo Infante, Adam D. Hincks, Viktor Malanushenko, John P. Hughes, David J. Schlegel, Joanna Dunkley, Eric R. Switzer, Alaina Shelden, Daniel J. Eisenstein, Benjamin R. Brown, Donald P. Schneider, Matt Hilton, Daniel S. Swetz, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), APC - Cosmologie, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Observational cosmology ,Background radiations ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Structure formation ,redshifts ,[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Cosmic microwave background ,FOS: Physical sciences ,General Physics and Astronomy ,Galaxy clusters ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Sunyaev–Zel'dovich effect ,01 natural sciences ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Physics and Astronomy (all) ,Galaxy groups and clusters ,0103 physical sciences ,spatial distribution of galaxies ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Galaxy cluster ,Physics ,010308 nuclear & particles physics ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,Galaxy ,Distances ,Atacama Cosmology Telescope ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,radial velocities ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Using 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., Comment: 6 pages, 1 figure. Updated version matches published paper. Updated analysis, with slightly different figure than the first version
- Published
- 2012
- Full Text
- View/download PDF
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