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I. D. Novikov
Researcher at Russian Academy of Sciences
Publications - 263
Citations - 83503
I. D. Novikov is an academic researcher from Russian Academy of Sciences. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 119, co-authored 260 publications receiving 78911 citations. Previous affiliations of I. D. Novikov include University of Copenhagen & Niels Bohr Institute.
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Planck early results. XXI. Properties of the interstellar medium in the Galactic plane
Alain Abergel,Peter A. R. Ade,Nabila Aghanim,M. Arnaud,M. Ashdown,J. Aumont,Carlo Baccigalupi,Amedeo Balbi,A. J. Banday,R. B. Barreiro,James G. Bartlett,James G. Bartlett,E. Battaner,Karim Benabed,Alain Benoit,J.-P. Bernard,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,R. Bhatia,J. J. Bock,Anna Bonaldi,J. R. Bond,Julian Borrill,Julian Borrill,F. R. Bouchet,F. Boulanger,M. Bucher,Carlo Burigana,Paolo Cabella,Jean-François Cardoso,Jean-François Cardoso,Jean-François Cardoso,A. Catalano,A. Catalano,L. Cayón,Anthony Challinor,A. Chamballu,Lung-Yih Chiang,C. Chiang,P. R. Christensen,Stéphane Colombi,F. Couchot,A. Coulais,B. P. Crill,F. Cuttaia,Thomas M. Dame,Luigi Danese,R. D. Davies,R. J. Davis,P. de Bernardis,G. de Gasperis,A. de Rosa,G. de Zotti,G. de Zotti,Jacques Delabrouille,J.-M. Delouis,F.-X. Désert,Clive Dickinson,S. Donzelli,S. Donzelli,Olivier Doré,U. Dörl,Marian Douspis,X. Dupac,George Efstathiou,Torsten A. Enßlin,Fabio Finelli,Olivier Forni,Olivier Forni,M. Frailis,E. Franceschi,S. Galeotta,Ken Ganga,Ken Ganga,M. Giard,M. Giard,G. Giardino,Y. Giraud-Héraud,J. González-Nuevo,K. M. Górski,K. M. Górski,Serge Gratton,A. Gregorio,I. A. Grenier,Alessandro Gruppuso,F. K. Hansen,D. L. Harrison,Sophie Henrot-Versille,D. Herranz,S. R. Hildebrandt,S. R. Hildebrandt,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,W. Hovest,Roger J. Hoyland,Kevin M. Huffenberger,T. R. Jaffe,T. R. Jaffe,Andrew H. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,Reijo Keskitalo,Reijo Keskitalo,Theodore Kisner,R. Kneissl,R. Kneissl,Lloyd Knox,Hannu Kurki-Suonio,Hannu Kurki-Suonio,Guilaine Lagache,Anne Lähteenmäki,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,René J. Laureijs,Charles R. Lawrence,S. Leach,Rodrigo Leonardi,Rodrigo Leonardi,C. Leroy,C. Leroy,C. Leroy,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,C. J. MacTavish,Bruno Maffei,Nazzareno Mandolesi,Robert G. Mann,Michele Maris,D. J. Marshall,D. J. Marshall,E. Martínez-González,Silvia Masi,Sabino Matarrese,F. Matthai,Pasquale Mazzotta,P. M. McGehee,Peter Meinhold,Alessandro Melchiorri,L. Mendes,A. Mennella,A. Mennella,Marc-Antoine Miville-Deschênes,Marc-Antoine Miville-Deschênes,A. Moneti,L. Montier,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,Dipak Munshi,A. Murphy,Pavel Naselsky,Paolo Natoli,Paolo Natoli,Paolo Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,S. Osborne,F. Pajot,Roberta Paladini,Fabio Pasian,G. Patanchon,O. Perdereau,L. Perotto,Francesca Perrotta,F. Piacentini,M. Piat,Stéphane Plaszczynski,Etienne Pointecouteau,Etienne Pointecouteau,G. Polenta,G. Polenta,N. Ponthieu,T. Poutanen,T. Poutanen,T. Poutanen,G. Prézeau,Simon Prunet,Jean-Loup Puget,Jörg P. Rachen,William T. Reach,Rafael Rebolo,Rafael Rebolo,W. Reich,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,I. Ristorcelli,Graca Rocha,C. Rosset,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,D. Santos,Giorgio Savini,Douglas Scott,M. D. Seiffert,P. Shellard,George F. Smoot,George F. Smoot,George F. Smoot,Jean-Luc Starck,Jean-Luc Starck,F. Stivoli,V. Stolyarov,Radek Stompor,R. V. Sudiwala,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,M. Tomasi,J. P. Torre,Matthieu Tristram,Jussi Tuovinen,G. Umana,Luca Valenziano,Jussi Varis,P. Vielva,F. Villa,Nicola Vittorio,Lawrence A. Wade,Benjamin D. Wandelt,Benjamin D. Wandelt,Althea Wilkinson,Nathalie Ysard,D. Yvon,Andrea Zacchei,Andrea Zonca +242 more
TL;DR: In this paper, a spectral energy distribution (SED) was created for various Galactocentric radii using velocity information from atomic (neutral hydrogen) and molecular ((12)CO) observations.
Journal ArticleDOI
Planck 2015 results. VII. HFI TOI and beam processing
R. Adam,P. A. R. Ade,Nabila Aghanim,M. Arnaud,M. Ashdown,J. Aumont,Carlo Baccigalupi,A. J. Banday,R. B. Barreiro,Nicola Bartolo,E. Battaner,K. Benabed,Alain Benoit,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,B. Bertincourt,P. Bielewicz,J. J. Bock,Laura Bonavera,J. R. Bond,J. Borrill,François R. Bouchet,F. Boulanger,M. Bucher,Carlo Burigana,E. Calabrese,Jean-François Cardoso,A. Catalano,Anthony Challinor,A. Chamballu,R.-R. Chary,H. C. Chiang,P. R. Christensen,D. L. Clements,Stéphane Colombi,L. P. L. Colombo,C. Combet,F. Couchot,A. Coulais,B. P. Crill,A. Curto,F. Cuttaia,L. Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,J. Delabrouille,J.-M. Delouis,F.-X. Désert,Jose M. Diego,H. Dole,S. Donzelli,O. Doré,M. Douspis,A. Ducout,X. Dupac,George Efstathiou,F. Elsner,Torsten A. Ensslin,H. K. Eriksen,E. Falgarone,James R. Fergusson,Fabio Finelli,Olivier Forni,M. Frailis,Aurelien A. Fraisse,E. Franceschi,A. Frejsel,S. Galeotta,Silvia Galli,K. Ganga,Tuhin Ghosh,M. Giard,Y. Giraud-Héraud,E. Gjerløw,J. González-Nuevo,K. M. Górski,Steven Gratton,Alessandro Gruppuso,Jon E. Gudmundsson,F. K. Hansen,D. Hanson,D. L. Harrison,Sophie Henrot-Versille,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,R. Keskitalo,Theodore Kisner,R. Kneissl,J. Knoche,M. Kunz,Hannu Kurki-Suonio,G. Lagache,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,M. Le Jeune,J. P. Leahy,E. Lellouch,R. Leonardi,Julien Lesgourgues,François Levrier,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Gianmarco Maggio,Davide Maino,Nazzareno Mandolesi,Anna Mangilli,Michele Maris,Pierrick Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Peregrine McGehee,Alessandro Melchiorri,L. Mendes,A. Mennella,M. Migliaccio,S. Mitra,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,R. Moreno,Gianluca Morgante,Daniel J. Mortlock,A. Moss,S. Mottet,Dipak Munshi,J. A. Murphy,Pavel D. Naselsky,Federico Nati,P. Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,Carol Anne Oxborrow,F. Paci,L. Pagano,F. Pajot,D. Paoletti,Fabio Pasian,G. Patanchon,T. J. Pearson,O. Perdereau,L. Perotto,F. Perrotta,V. Pettorino,F. Piacentini,M. Piat,Elena Pierpaoli,D. Pietrobon,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,G. W. Pratt,G. Prézeau,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Martin Reinecke,Mathieu Remazeilles,C. Renault,A. Renzi,I. Ristorcelli,G. Rocha,C. Rosset,M. Rossetti,G. Roudier,Michael Rowan-Robinson,B. Rusholme,M. Sandri,D. Santos,A. Sauvé,M. Savelainen,Giorgio Savini,Douglas Scott,M. D. Seiffert,E. P. S. Shellard,Locke D. Spencer,V. Stolyarov,R. Stompor,R. V. Sudiwala,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,M. Tristram,M. Tucci,Jussi Tuovinen,Luca Valenziano,J. Valiviita,B. Van Tent,L. Vibert,P. Vielva,F. Villa,Lawrence A. Wade,B. D. Wandelt,Robert A. Watson,Ingunn Kathrine Wehus,D. Yvon,A. Zacchei,A. Zonca +226 more
TL;DR: The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polarization as discussed by the authors.
Journal ArticleDOI
Planck 2013 results. XVIII. Gravitational lensing-infrared background correlation
P. A. R. Ade,Nabila Aghanim,C. Armitage-Caplan,M. Arnaud,M. Ashdown,Fernando Atrio-Barandela,Jonathan Aumont,C. Baccigalupi,A. J. Banday,R. B. Barreiro,J. G. Bartlett,Soumen Basak,E. Battaner,K. Benabed,Aurélien Benoit,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,Matthieu Béthermin,P. Bielewicz,Jérôme Bobin,J. J. Bock,Anna Bonaldi,J. R. Bond,J. Borrill,F. R. Bouchet,F. Boulanger,M. Bridges,M. Bucher,Carlo Burigana,R. C. Butler,Jean-François Cardoso,A. Catalano,Anthony Challinor,A. Chamballu,Lung-Yih Chiang,H. C. Chiang,P. R. Christensen,Sarah E. Church,D. L. Clements,Stéphane Colombi,L. P. L. Colombo,F. Couchot,A. Coulais,B. P. Crill,A. Curto,F. Cuttaia,L. Danese,R. D. Davies,P. de Bernardis,A. de Rosa,G. de Zotti,J. Delabrouille,J.-M. Delouis,F.-X. Désert,Jose M. Diego,H. Dole,S. Donzelli,O. Doré,M. Douspis,X. Dupac,George Efstathiou,Torsten A. Enßlin,H. K. Eriksen,Fabio Finelli,Olivier Forni,M. Frailis,E. Franceschi,S. Galeotta,K. Ganga,M. Giard,Giovanna Giardino,Y. Giraud-Héraud,J. González-Nuevo,K. M. Górski,Steven Gratton,A. Gregorio,A. Gruppuso,Jon E. Gudmundsson,F. K. Hansen,D. Hanson,D. L. Harrison,Sophie Henrot-Versille,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,T. R. Jaffe,Andrew H. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,R. Keskitalo,Theodore Kisner,R. Kneissl,J. Knoche,Lloyd Knox,M. Kunz,Hannu Kurki-Suonio,F. Lacasa,G. Lagache,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,R. J. Laureijs,Charles R. Lawrence,R. Leonardi,J. Leon-Tavares,Julien Lesgourgues,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,Davide Maino,Nazzareno Mandolesi,Michele Maris,D. J. Marshall,Pierrick Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,F. Matthai,Pasquale Mazzotta,Alessandro Melchiorri,L. Mendes,A. Mennella,M. Migliaccio,S. Mitra,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,Pavel D. Naselsky,Federico Nati,P. Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,S. Osborne,Carol Anne Oxborrow,F. Paci,L. Pagano,F. Pajot,D. Paoletti,Fabio Pasian,G. Patanchon,O. Perdereau,L. Perotto,F. Perrotta,F. Piacentini,M. Piat,Elena Pierpaoli,D. Pietrobon,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,N. Ponthieu,L. Popa,T. Poutanen,G. W. Pratt,G. Prézeau,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Rafael Rebolo,Martin Reinecke,Mathieu Remazeilles,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,G. Rocha,C. Rosset,G. Roudier,Michael Rowan-Robinson,B. Rusholme,M. Sandri,D. Santos,Giorgio Savini,Douglas Scott,M. D. Seiffert,Paolo Serra,E. P. S. Shellard,Locke D. Spencer,Jean-Luc Starck,V. Stolyarov,R. Stompor,R. V. Sudiwala,R. A. Sunyaev,F. Sureau,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Daniele Tavagnacco,Luca Terenzi,L. Toffolatti,M. Tomasi,M. Tristram,M. Tucci,Jussi Tuovinen,Luca Valenziano,J. Valiviita,B. Van Tent,P. Vielva,F. Villa,Nicola Vittorio,Lawrence A. Wade,B. D. Wandelt,S. D. M. White,D. Yvon,A. Zacchei,A. Zonca +224 more
TL;DR: In this paper, the authors measured the SFR density with around 2 sigma significance for three redshift bins between z=1 and 7, thus opening a new window into the study of the formation of stars at early times.
Journal ArticleDOI
Planck intermediate results. XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust
R. Adam,Peter A. R. Ade,Nabila Aghanim,M. I. R. Alves,M. Arnaud,Doris Arzoumanian,M. Ashdown,J. Aumont,Carlo Baccigalupi,A. J. Banday,R. B. Barreiro,Nicola Bartolo,E. Battaner,K. Benabed,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,P. Bielewicz,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,François R. Bouchet,F. Boulanger,Andrea Bracco,Carlo Burigana,R. C. Butler,Erminia Calabrese,Jean-François Cardoso,A. Catalano,A. Chamballu,H. C. Chiang,P. R. Christensen,Stéphane Colombi,L. P. L. Colombo,C. Combet,F. Couchot,B. P. Crill,A. Curto,F. Cuttaia,Luigi Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,Jacques Delabrouille,Clive Dickinson,Jose M. Diego,H. Dole,S. Donzelli,Olivier Doré,M. Douspis,A. Ducout,X. Dupac,George Efstathiou,F. Elsner,Torsten A. Enßlin,H. K. Eriksen,E. Falgarone,K. Ferrière,Fabio Finelli,Olivier Forni,M. Frailis,A. A. Fraisse,E. Franceschi,A. Frejsel,S. Galeotta,Silvia Galli,K. Ganga,Tuhin Ghosh,M. Giard,E. Gjerløw,J. González-Nuevo,Krzysztof M. Gorski,A. Gregorio,Alessandro Gruppuso,Vincent Guillet,F. K. Hansen,D. Hanson,D. L. Harrison,Sophie Henrot-Versille,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,W. A. Holmes,W. Hovest,Kevin M. Huffenberger,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,W. C. Jones,E. Keihänen,R. Keskitalo,Theodore Kisner,R. Kneissl,J. Knoche,M. Kunz,Hannu Kurki-Suonio,G. Lagache,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,R. Leonardi,François Levrier,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,Davide Maino,Nazzareno Mandolesi,Michele Maris,D. J. Marshall,Pierrick Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Pasquale Mazzotta,Alessandro Melchiorri,L. Mendes,A. Mennella,M. Migliaccio,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Pavel Naselsky,P. Natoli,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,Niels Oppermann,Carol Anne Oxborrow,L. Pagano,F. Pajot,D. Paoletti,Fabio Pasian,O. Perdereau,L. Perotto,F. Perrotta,V. Pettorino,F. Piacentini,M. Piat,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,N. Ponthieu,L. Popa,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,William T. Reach,Martin Reinecke,Mathieu Remazeilles,C. Renault,I. Ristorcelli,G. Rocha,G. Roudier,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,D. Santos,Giorgio Savini,Douglas Scott,Juan D. Soler,Locke D. Spencer,V. Stolyarov,R. V. Sudiwala,R. A. Sunyaev,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,M. Tristram,M. Tucci,G. Umana,Luca Valenziano,J. Valiviita,B. Van Tent,P. Vielva,F. Villa,Lawrence A. Wade,B. D. Wandelt,Ingunn Kathrine Wehus,Helmut Wiesemeyer,D. Yvon,A. Zacchei,A. Zonca +200 more
Abstract: The role of the magnetic field in the formation of the filamentary structures observed in the interstellar medium (ISM) is a debated topic. The Planck all-sky maps of linearly polarized emission from dust at 353GHz provide the required combination of imaging and statistics to study the correlation between the structures of the Galactic magnetic field and of interstellar matter, both in the diffuse ISM and in molecular clouds. The data reveal structures, or ridges, in the intensity map with counterparts in the Stokes Q and/or U maps. We focus on structures at intermediate and high Galactic latitudes with column density from $10^{20}$ to $10^{22}$ cm$^{-2}$. We measure the magnetic field orientation on the plane of the sky from the polarization data, and present an algorithm to estimate the orientation of the ridges from the dust intensity map. We use analytical models to account for projection effects. Comparing polarization angles on and off the structures, we estimate the mean ratio between the strengths of the turbulent and mean components of the magnetic field to be between 0.6 and 1.0, with a preferred value of 0.8. We find that the ridges are preferentially aligned with the magnetic field measured on the structures. This trend becomes more striking for increasing polarization fraction and decreasing column density. We interpret the increase of alignment with polarization fraction as a consequence of projections effects. The decrease of alignment for high column density is not due to a loss of correlation between the structures and the geometry of the magnetic field. In molecular complexes, we observe structures perpendicular to the magnetic field, which cannot be accounted for by projection effects. We discuss our results in the context of models and MHD simulations, which describe the formation of structures in the magnetized ISM.
Journal ArticleDOI
Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
Peter A. R. Ade,Nabila Aghanim,C. Armitage-Caplan,Monique Arnaud,M. Ashdown,Fernando Atrio-Barandela,J. Aumont,Carlo Baccigalupi,A. J. Banday,A. J. Banday,R. B. Barreiro,James G. Bartlett,James G. Bartlett,Nicola Bartolo,E. Battaner,K. Benabed,Alain Benoit,A. Benoit-Lévy,A. Benoit-Lévy,J.-P. Bernard,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,P. Bielewicz,P. Bielewicz,P. Bielewicz,Jérôme Bobin,J. J. Bock,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,Julian Borrill,François R. Bouchet,M. Bridges,M. Bucher,Carlo Burigana,Carlo Burigana,R. C. Butler,Jean-François Cardoso,Jean-François Cardoso,Jean-François Cardoso,A. Catalano,A. Catalano,Anthony Challinor,A. Chamballu,A. Chamballu,A. Chamballu,H. C. Chiang,H. C. Chiang,Lung-Yih Chiang,P. R. Christensen,Sarah E. Church,David L. Clements,S. Colombi,L. P. L. Colombo,L. P. L. Colombo,F. Couchot,A. Coulais,B. P. Crill,A. Curto,A. Curto,F. Cuttaia,Luigi Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,G. de Zotti,Jacques Delabrouille,J.-M. Delouis,F.-X. Désert,Clive Dickinson,Jose M. Diego,Klaus Dolag,Klaus Dolag,H. Dole,H. Dole,S. Donzelli,Olivier Doré,Marian Douspis,X. Dupac,George Efstathiou,Torsten A. Enßlin,H. K. Eriksen,James R. Fergusson,Fabio Finelli,Olivier Forni,Olivier Forni,Pablo Fosalba,M. Frailis,E. Franceschi,M. Frommert,S. Galeotta,K. Ganga,Ricardo Génova-Santos,M. Giard,M. Giard,G. Giardino,Y. Giraud-Héraud,J. González-Nuevo,J. González-Nuevo,Krzysztof M. Gorski,Krzysztof M. Gorski,Serge Gratton,A. Gregorio,A. Gregorio,Alessandro Gruppuso,F. K. Hansen,Duncan Hanson,Duncan Hanson,Duncan Hanson,D. L. Harrison,Sophie Henrot-Versille,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Shirley Ho,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,S. Ilić,Andrew H. Jaffe,T. R. Jaffe,T. R. Jaffe,Jens Jasche,W. C. Jones,Mika Juvela,E. Keihänen,Reijo Keskitalo,Reijo Keskitalo,Theodore Kisner,J. Knoche,Lloyd Knox,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,Hannu Kurki-Suonio,Guilaine Lagache,Anne Lähteenmäki,Anne Lähteenmäki,J.-M. Lamarre,Mathieu Langer,Anthony Lasenby,René J. Laureijs,Charles R. Lawrence,J. P. Leahy,R. Leonardi,Julien Lesgourgues,Julien Lesgourgues,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,Davide Maino,Davide Maino,N. Mandolesi,N. Mandolesi,N. Mandolesi,Anna Mangilli,A. Marcos-Caballero,M. Maris,D. J. Marshall,Peter G. Martin,E. Martínez-González,Silvia Masi,Marcella Massardi,Sabino Matarrese,F. Matthai,Pasquale Mazzotta,Peter Meinhold,Alessandro Melchiorri,L. Mendes,A. Mennella,A. Mennella,M. Migliaccio,Subhabrata Mitra,Subhabrata Mitra,M.-A. Miville-Deschênes,M.-A. Miville-Deschênes,A. Moneti,L. Montier,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Adam Moss,Dipak Munshi,Pavel Naselsky,Federico Nati,Paolo Natoli,Paolo Natoli,Paolo Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,S. Osborne,C. A. Oxborrow,F. Paci,L. Pagano,F. Pajot,Daniela Paoletti,Bruce Partridge,F. Pasian,G. Patanchon,O. Perdereau,L. Perotto,Francesca Perrotta,F. Piacentini,M. Piat,E. Pierpaoli,Davide Pietrobon,Stéphane Plaszczynski,Etienne Pointecouteau,Etienne Pointecouteau,G. Polenta,G. Polenta,N. Ponthieu,N. Ponthieu,L. Popa,T. Poutanen,T. Poutanen,T. Poutanen,G. W. Pratt,G. Prézeau,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Jörg P. Rachen,B. Racine,Rafael Rebolo,Rafael Rebolo,M. Reinecke,Mathieu Remazeilles,Mathieu Remazeilles,Mathieu Remazeilles,C. Renault,A. Renzi,S. Ricciardi,T. Riller,I. Ristorcelli,I. Ristorcelli,Graca Rocha,C. Rosset,G. Roudier,G. Roudier,G. Roudier,Michael Rowan-Robinson,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,D. Santos,Giorgio Savini,B. M. Schaefer,F. Schiavon,Douglas Scott,Michael Seiffert,E. P. S. Shellard,Locke D. Spencer,Jean-Luc Starck,V. Stolyarov,V. Stolyarov,Radek Stompor,R. V. Sudiwala,R. A. Sunyaev,R. A. Sunyaev,F. Sureau,Paul M. Sutter,D. Sutton,A.-S. Suur-Uski,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,D. Tavagnacco,D. Tavagnacco,Luca Terenzi,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tristram,M. Tucci,M. Tucci,Jussi Tuovinen,G. Umana,Luca Valenziano,Jussi-Pekka Väliviita,Jussi-Pekka Väliviita,Jussi-Pekka Väliviita,B. Van Tent,Jussi Varis,Matteo Viel,P. Vielva,Fabrizio Villa,Nicola Vittorio,L. A. Wade,Benjamin D. Wandelt,Benjamin D. Wandelt,Martin White,Jun-Qing Xia,D. Yvon,Andrea Zacchei,Andrea Zonca +311 more
TL;DR: In this paper, the authors presented the detection of the integrated Sachs-Wolfe (ISW) effect, that is, the correlation between the CMB and large-scale evolving gravitational potentials.