Planck intermediate results - XIII. Constraints on peculiar velocities

@article{Ade2013PlanckIR,
  title={Planck intermediate results - XIII. Constraints on peculiar velocities},
  author={P. A. R. Ade and Nabila Aghanim and Monique D. Arnaud and Mark Ashdown and J. Aumont and Carlo Baccigalupi and Amedeo Balbi and A. J. Banday and Rita Bel{\'e}n Barreiro and Eduardo Battaner and Karim Benabed and Aur{\'e}lien Benoit-L{\'e}vy and J-Ph. Bernard and M. Bersanelli and Pawel Bielewicz and Ilfan F. Bikmaev and J{\'e}r{\^o}me Bobin and James J. Bock and Anna Bonaldi and J. Richard Bond and Julian Borrill and Francois R. Bouchet and Carlo Burigana and R. C. Butler and Paolo Cabella and J.-F. Cardoso and A. Catalano and A. Chamballu and L. Y. Chiang and Gayoung Chon and Philip R. Christensen and David L. Clements and St{\'e}phane Colombi and Loris P. L. Colombo and Brendan P. Crill and F. Cuttaia and A. da Silva and H{\aa}kon Dahle and Rodney D. Davies and R. J. Davis and Paolo Bernardis and Giancarlo de Gasperis and Gianfranco de Zotti and Jacques Delabrouille and Jessica Democles and Jose M. Diego and Klaus Dolag and Herve A. Dole and Simona Donzelli and Olivier Dor{\'e} and U. Doerl and Marian Douspis and Xavier Dupac and Torsten A. Ensslin and Fabio Finelli and In{\'e}s Flores-Cacho and Olivier Forni and Marco Frailis and Mona Frommert and S. Galeotta and Ken Ganga and Ricardo G{\'e}nova-Santos and Martin Giard and G. Giardino and Joaqu{\'i}n Gonz{\'a}lez-Nuevo and Anna Gregorio and Alessandro Gruppuso and Frode K. Hansen and D. L. Harrison and Carlos Hernandez-Monteagudo and Diego Herranz and Sergi R. Hildebrandt and Eric Hivon and Warren Albert Holmes and W. Hovest and Kevin M. Huffenberger and Guillaume Hurier and Tess R. Jaffe and Andrew H. Jaffe and Jens Jasche and William C Jones and Mika Juvela and Elina Keihanen and Reijo Keskitalo and Irek M. Khamitov and Theodore Kisner and J{\"o}rg Knoche and Martin Kunz and Hannu Kurki-Suonio and Guilaine Lagache and Anne Lahteenmaki and J-M. Lamarre and Anthony N. Lasenby and Charles R. Lawrence and Maude Le Jeune and Rodrigo Leonardi and Per B. Lilje and M. J. D. Linden-V{\o}rnle and Marcos L{\'o}pez-Caniego and J. F. Mac{\'i}as-P{\'e}rez and Davide Maino and Daisy S. Y. Mak and Nazzareno Mandolesi and Michele Maris and Francine Roxanne Marleau and Enrique Mart{\'i}nez-Gonz{\'a}lez and Serena Masi and S. Matarrese and Pasquale Mazzotta and Alessandro Melchiorri and J. B. Melin and Luis Mendes and Aniello Mennella and Marina Migliaccio and Supriyo Mitra and Marc-Antoine Miville-Desch{\^e}nes and Andrea Moneti and Ludovic Montier and G. Morgante and Daniel J. Mortlock and Adam Moss and Dipak Munshi and J. Anthony Murphy and Pavel D. Naselsky and Federico Nati and Paolo Natoli and Calvin Barth Netterfield and Hans Ulrik N{\o}rgaard-Nielsen and Fabio Noviello and Dmitry I. Novikov and I. Novikov and Shannon Osborne and Luca Pagano and Daniela Paoletti and Olivier Perdereau and F. Perrotta and Francesco Piacentini and Michel Piat and Elena Pierpaoli and Davide Pietrobon and St{\'e}phane Plaszczynski and Etienne Pointecouteau and Gianluca Polenta and L. A. Popa and Torsti J. Poutanen and Gabriel W. Pratt and Simon Prunet and J-L. Puget and Salom{\'e} Puisieux and Jorg P. Rachen and Rafael Rebolo and Martin Reinecke and Mathieu Remazeilles and C{\'e}cile Renault and Stefano Ricciardi and M. Roman and Jos{\'e} Alberto Rubi{\~n}o-Mart{\'i}n and Ben Rusholme and M. Sandri and Giorgio Savini and Douglas Scott and Locke D Spencer and Rashid Alievich Sunyaev and David O. Sutton and A.-S. Suur-Uski and J. -F. Sygnet and Jan Tauber and Luca Terenzi and Luigi Toffolatti and Maurizio Tomasi and M. Tristram and Marco Tucci and Luca Valenziano and Jussi Valiviita and Bartjan van Tent and Patricio Vielva and Fabrizio Villa and Nicola Vittorio and Lawrence A. Wade and Niraj Welikala and D. Yvon and Andrea Zacchei and James P. Zibin and Andrea Zonca},
  journal={Astronomy and Astrophysics},
  year={2013},
  volume={561},
  pages={1-21}
}
Using Planck data combined with the Meta Catalogue of X-ray detected Clusters of galaxies (MCXC), we address the study of peculiar motions by searching for evidence of the kinetic Sunyaev-Zeldovich effect (kSZ). By implementing various filters designed to extract the kSZ generated at the positions of the clusters, we obtain consistent constraints on the radial peculiar velocity average, root mean square (rms), and local bulk flow amplitude at different depths. For the whole cluster sample of… 
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The interaction of the cosmic microwave background (CMB) with the hot gas in clusters of galaxies, the so-called Sunyaev--Zel'dovich (SZ) effect, is a very useful tool that allows us to determine the
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Context. Our Local Group of galaxies appears to be moving relative to the cosmic microwave background with the source of the peculiar motion still uncertain. While in the past this has been studied
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Our velocity relative to the rest frame of the cosmic microwave background (CMB) generates a dipole temperature anisotropy on the sky which has been well measured for more than 30 years, and has an
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We re-analyze the detectability of large scale dark flow (or local bulk flow) with respect to the CMB background based upon the redshift-distance relation for Type Ia supernovae (SN Ia). We made two
Quasar host environments: The view from Planck
We measure the far-infrared emission of the general quasar (QSO) population using Planck observations of the Baryon Oscillation Spectroscopic Survey QSO sample. By applying multi-component matched
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References

SHOWING 1-10 OF 126 REFERENCES
Planck intermediate results: V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect
Taking advantage of the all-sky coverage and broad frequency range of the Planck satellite, we study the Sunyaev-Zeldovich (SZ) and pressure profiles of 62 nearby massive clusters detected at high
Using the kinematic Sunyaev-Zeldovich effect to determine the peculiar velocities of clusters of galaxies
We have investigated the possibility of inferring peculiar velocities for clusters of galaxies from the Doppler shift of scattered cosmic microwave background (CMB) photons. We find that if the core
A measurement of large-scale peculiar velocities of clusters of galaxies: technical details
This paper presents detailed analysis of large-scale peculiar motions derived from a sample of ~700 X-ray clusters and cosmic microwave background (CMB) data obtained with WMAP. We use the kinematic
A Measurement of Large-Scale Peculiar Velocities of Clusters of Galaxies: Results and Cosmological Implications
Peculiar velocities of clusters of galaxies can be measured by studying the fluctuations in the cosmic microwave background (CMB) generated by the scattering of the microwave photons by the hot
Limits on the Peculiar Velocities of Two Distant Clusters Using the Kinematic Sunyaev-Zeldovich Effect
We report millimeter-wavelength observations of the Sunyaev-Zeldovich (S-Z) effect in two distant galaxy clusters. A relativistically correct analysis of the S-Z data is combined with the results of
Peculiar velocity limits from measurements of the spectrum of the Sunyaev-Zeldovich effect in six clusters of galaxies
We have made measurements of the Sunyaev-Zeldovich (SZ) effect in six galaxy clusters at z > 0.2 using the Sunyaev-Zeldovich Infrared Experiment (SuZIE II) in three frequency bands between 150 and
Measuring Bulk Flow of Galaxy Clusters Using Kinematic Sunyaev-Zeldovich Effect: Prediction for Planck
We predict the performance of the Planck satellite in determining the bulk flow through kinetic Sunyaev-Zeldovich (kSZ) measurements. As velocity tracers, we use ROSAT All-Sky Survey (RASS) clusters
A Large-scale Bulk Flow of Galaxy Clusters
We report first results from the Streaming Motions of Abell Clusters (SMAC) project, an all-sky Fundamental Plane survey of 699 early-type galaxies in 56 clusters between ~3000 and ~14,000 km s-1.
Planckearly results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations
We present precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z < 0.5) detected at high signal-tonoise in the first Planck all-sky data set. The sample
Shellflow. I. The Convergence of the Velocity Field at 6000 Kilometers Per Second
We present the first results from the Shellflow program, an all-sky Tully-Fisher (TF) peculiar-velocity survey of 276 Sb-Sc galaxies with redshifts between 4500 and 7000 km s-1. Shellflow was
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