G
G. Roudier
Researcher at California Institute of Technology
Publications - 188
Citations - 77342
G. Roudier is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 104, co-authored 186 publications receiving 72114 citations. Previous affiliations of G. Roudier include Centre national de la recherche scientifique & University of Paris.
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Journal ArticleDOI
Planck intermediate results: XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes at the Canary Islands observatories
Peter A. R. Ade,Nabila Aghanim,Monique Arnaud,M. Ashdown,J. Aumont,Carlo Baccigalupi,A. J. Banday,R. B. Barreiro,R. Barrena,R. Barrena,Nicola Bartolo,Nicola Bartolo,E. Battaner,Karim Benabed,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,P. Bielewicz,P. Bielewicz,I. F. Bikmaev,I. F. Bikmaev,Hans Böhringer,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,Julian Borrill,F. R. Bouchet,R. A. Burenin,R. A. Burenin,Carlo Burigana,Carlo Burigana,Erminia Calabrese,Jean-François Cardoso,A. Catalano,A. Chamballu,R.-R. Chary,H. C. Chiang,H. C. Chiang,G. Chon,P. R. Christensen,David L. Clements,L. P. L. Colombo,L. P. L. Colombo,C. Combet,B. Comis,B. P. Crill,A. Curto,A. Curto,F. Cuttaia,Håkon Dahle,Luigi Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,G. de Zotti,Jacques Delabrouille,Jose M. Diego,H. Dole,S. Donzelli,O. Doré,Marian Douspis,X. Dupac,George Efstathiou,F. Elsner,Torsten A. Enßlin,H. K. Eriksen,A. Ferragamo,A. Ferragamo,Fabio Finelli,Olivier Forni,M. Frailis,Aurelien A. Fraisse,E. Franceschi,S. Fromenteau,S. Galeotta,S. Galli,K. Ganga,Ricardo Genova-Santos,Ricardo Genova-Santos,M. Giard,E. Gjerløw,J. González-Nuevo,J. González-Nuevo,K. M. Górski,K. M. Górski,Alessandro Gruppuso,F. K. Hansen,D. L. Harrison,A. Hempel,A. Hempel,A. Hempel,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,G. Hurier,T. R. Jaffe,E. Keihänen,Reijo Keskitalo,Irek Khamitov,Irek Khamitov,Theodore Kisner,R. Kneissl,R. Kneissl,J. Knoche,M. Kunz,Hannu Kurki-Suonio,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,R. Leonardi,Jonathan León-Tavares,Jonathan León-Tavares,Jonathan León-Tavares,François Levrier,H. Lietzen,H. Lietzen,Michele Liguori,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,Davide Maino,Davide Maino,N. Mandolesi,N. Mandolesi,Michele Maris,Peter G. Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Sabino Matarrese,P. M. McGehee,Alessandro Melchiorri,A. Mennella,A. Mennella,M. Migliaccio,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Pavel Naselsky,Federico Nati,Paolo Natoli,Paolo Natoli,Paolo Natoli,Dmitry Novikov,I. D. Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,Daniela Paoletti,Fabio Pasian,O. Perdereau,Valeria Pettorino,F. Piacentini,M. Piat,Elena Pierpaoli,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,G. Polenta,G. W. Pratt,Simon Prunet,Jean-Loup Puget,Jörg P. Rachen,Jörg P. Rachen,Rafael Rebolo,Rafael Rebolo,Martin Reinecke,Mathieu Remazeilles,C. Renault,A. Renzi,I. Ristorcelli,Graca Rocha,C. Rosset,M. Rossetti,M. Rossetti,G. Roudier,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,D. Santos,M. Savelainen,Giorgio Savini,Douglas Scott,V. Stolyarov,V. Stolyarov,V. Stolyarov,Alina Streblyanska,Alina Streblyanska,R. V. Sudiwala,R. A. Sunyaev,R. A. Sunyaev,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tomasi,D. Tramonte,D. Tramonte,Matthieu Tristram,M. Tucci,Luca Valenziano,Jussi Valiviita,B. Van Tent,P. Vielva,F. Villa,Lawrence A. Wade,Benjamin D. Wandelt,Ingunn Kathrine Wehus,D. Yvon,A. Zacchei,Andrea Zonca +233 more
TL;DR: The results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with telescopes at the Canary Islands observatories as part of the general optical follow-up programme undertaken by the Planck Collaboration are discussed in this article.
Journal ArticleDOI
Planck intermediate results. XXIII. Galactic plane emission components derived from Planck with ancillary data
Peter A. R. Ade,Nabila Aghanim,M. I. R. Alves,M. Arnaud,M. Ashdown,Fernando Atrio-Barandela,Jonathan Aumont,C. Baccigalupi,A. J. Banday,R. B. Barreiro,E. Battaner,K. Benabed,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,P. Bielewicz,Jérôme Bobin,Anna Bonaldi,J. R. Bond,F. R. Bouchet,F. Boulanger,Carlo Burigana,Jean-François Cardoso,A. Catalano,A. Chamballu,H. C. Chiang,P. R. Christensen,D. L. Clements,Stéphane Colombi,L. P. L. Colombo,C. Combet,F. Couchot,B. P. Crill,F. Cuttaia,L. Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,J. Delabrouille,Clive Dickinson,Jose M. Diego,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,Ricardo Génova-Santos,Tuhin Ghosh,M. Giard,Giovanna Giardino,Y. Giraud-Héraud,J. González-Nuevo,K. M. Górski,A. Gregorio,Alessandro Gruppuso,F. K. Hansen,D. L. Harrison,Sophie Henrot-Versille,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,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,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,Charles R. Lawrence,R. Leonardi,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Davide Maino,Nazzareno Mandolesi,Pierrick Martin,E. Martínez-González,Silvia Masi,Marcella Massardi,Sabino Matarrese,Pasquale Mazzotta,Peter Meinhold,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,J. A. Murphy,Pavel Naselsky,Federico Nati,P. Natoli,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,R. Paladini,D. Paoletti,Fabio Pasian,T. J. Pearson,Michael W. Peel,O. Perdereau,F. Perrotta,F. Piacentini,M. Piat,Elena Pierpaoli,D. Pietrobon,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,N. Ponthieu,L. Popa,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,William T. Reach,Rafael Rebolo,W. Reich,Martin Reinecke,Mathieu Remazeilles,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,G. Rocha,C. Rosset,G. Roudier,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,Giorgio Savini,Douglas Scott,Locke D. Spencer,V. Stolyarov,Andrew W. Strong,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Daniele Tavagnacco,Luca Terenzi,Christopher Tibbs,L. Toffolatti,M. Tomasi,M. Tristram,M. Tucci,Luca Valenziano,J. Valiviita,B. Van Tent,Jussi Varis,P. Vielva,F. Villa,Lawrence A. Wade,B. D. Wandelt,Robert A. Watson,D. Yvon,A. Zacchei,A. Zonca +190 more
TL;DR: In this article, the spectral energy distributions (SEDs) at positions along the Galactic plane using the wide frequency coverage of Planck (28.4-857GHz) in combination with low-frequency radio data at 0.408-2.3GHz plus WMAP data at 23-94GHz, along with far-infrared (FIR) data from DIRBE and IRAS.
Journal ArticleDOI
Planck intermediate results: XLIII. Spectral energy distribution of dust in clusters of galaxies
R. Adam,Peter A. R. Ade,Nabila Aghanim,M. Ashdown,J. Aumont,Carlo Baccigalupi,A. J. Banday,A. J. Banday,R. B. Barreiro,Nicola Bartolo,Nicola Bartolo,E. Battaner,K. Benabed,A. Benoit-Lévy,A. Benoit-Lévy,Marco Bersanelli,Marco Bersanelli,P. Bielewicz,P. Bielewicz,I. F. Bikmaev,I. F. Bikmaev,Anna Bonaldi,J. R. Bond,Julian Borrill,Julian Borrill,François R. Bouchet,R. A. Burenin,R. A. Burenin,Carlo Burigana,Carlo Burigana,Erminia Calabrese,Jean-François Cardoso,Jean-François Cardoso,Jean-François Cardoso,A. Catalano,A. Catalano,H. C. Chiang,H. C. Chiang,P. R. Christensen,E. Churazov,E. Churazov,L. P. L. Colombo,L. P. L. Colombo,C. Combet,B. Comis,F. Couchot,B. P. Crill,A. Curto,A. Curto,F. Cuttaia,Luigi Danese,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,G. de Zotti,Jacques Delabrouille,F.-X. Désert,Jose M. Diego,H. Dole,H. Dole,Olivier Doré,Marian Douspis,A. Ducout,A. Ducout,X. Dupac,F. Elsner,F. Elsner,Torsten A. Enßlin,Fabio Finelli,Olivier Forni,Olivier Forni,M. Frailis,A. A. Fraisse,E. Franceschi,S. Galeotta,K. Ganga,Ricardo Genova-Santos,Ricardo Genova-Santos,M. Giard,M. Giard,Y. Giraud-Héraud,E. Gjerløw,J. González-Nuevo,J. González-Nuevo,Krzysztof M. Gorski,Krzysztof M. Gorski,A. Gregorio,A. Gregorio,Alessandro Gruppuso,Jon E. Gudmundsson,Jon E. Gudmundsson,Jon E. Gudmundsson,F. K. Hansen,D. L. Harrison,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,Allan Hornstrup,W. Hovest,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,T. R. Jaffe,W. C. Jones,E. Keihänen,Reijo Keskitalo,Irek Khamitov,Irek Khamitov,Theodore Kisner,R. Kneissl,R. Kneissl,J. Knoche,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,Hannu Kurki-Suonio,Guilaine Lagache,Guilaine Lagache,Anne Lähteenmäki,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,R. Leonardi,François Levrier,Michele Liguori,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,M. López-Caniego,J. F. Macías-Pérez,Bruno Maffei,Gianmarco Maggio,N. Mandolesi,N. Mandolesi,A. Mangilli,A. Mangilli,Michele Maris,Peter G. Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Sabino Matarrese,Alessandro Melchiorri,A. Mennella,A. Mennella,M. Migliaccio,Marc-Antoine Miville-Deschênes,Marc-Antoine Miville-Deschênes,A. Moneti,L. Montier,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Pavel Naselsky,Federico Nati,Paolo Natoli,Paolo Natoli,Hans Ulrik Nørgaard-Nielsen,Dmitry Novikov,I. D. Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,Daniela Paoletti,Fabio Pasian,O. Perdereau,L. Perotto,Valeria Pettorino,F. Piacentini,M. Piat,Stéphane Plaszczynski,Etienne Pointecouteau,Etienne Pointecouteau,G. Polenta,G. Polenta,Nicolas Ponthieu,Nicolas Ponthieu,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Jörg P. Rachen,Rafael Rebolo,Rafael Rebolo,Martin Reinecke,Mathieu Remazeilles,Mathieu Remazeilles,Mathieu Remazeilles,C. Renault,A. Renzi,I. Ristorcelli,I. Ristorcelli,Graca Rocha,C. Rosset,M. Rossetti,M. Rossetti,G. Roudier,G. Roudier,G. Roudier,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,Ben Rusholme,D. Santos,M. Savelainen,M. Savelainen,Giorgio Savini,Douglas Scott,V. Stolyarov,V. Stolyarov,V. Stolyarov,Radek Stompor,R. V. Sudiwala,R. A. Sunyaev,R. A. Sunyaev,D. Sutton,A.-S. Suur-Uski,A.-S. Suur-Uski,J.-F. Sygnet,Jan Tauber,Luca Terenzi,Luca Terenzi,L. Toffolatti,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tomasi,Matthieu Tristram,M. Tucci,Luca Valenziano,Jussi Valiviita,Jussi Valiviita,F. Van Tent,P. Vielva,F. Villa,Lawrence A. Wade,Ingunn Kathrine Wehus,Ingunn Kathrine Wehus,D. Yvon,Andrea Zacchei,Andrea Zonca +249 more
TL;DR: In this article, the spectral energy distribution (SED) of the infrared spectrum of thermal dust emission in clusters of galaxies was obtained by using a stacking approach for a sample of several hundred objects from the Planck cluster sample; this procedure averaged out fluctuations from the IR sky, allowing to reach a significant detection of the faint cluster contribution.
Journal ArticleDOI
Planck intermediate results. XXXIX. The Planck list of high-redshift source candidates
Peter A. R. Ade,Nabila Aghanim,M. Arnaud,J. Aumont,Carlo Baccigalupi,A. J. Banday,R. B. Barreiro,N. Bartolo,E. Battaner,K. Benabed,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,P. Bielewicz,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,F. R. Bouchet,F. Boulanger,Carlo Burigana,R. C. Butler,Erminia Calabrese,A. Catalano,H. C. Chiang,P. R. Christensen,D. L. Clements,L. P. L. Colombo,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,Jacques Delabrouille,Clive Dickinson,Jose M. Diego,H. Dole,Olivier Doré,M. Douspis,A. Ducout,X. Dupac,F. Elsner,Torsten A. Enßlin,H. K. Eriksen,E. Falgarone,Fabio Finelli,I. Flores-Cacho,M. Frailis,Aurelien A. Fraisse,E. Franceschi,S. Galeotta,Silvia Galli,K. Ganga,M. Giard,Y. Giraud-Héraud,E. Gjerløw,J. González-Nuevo,Krzysztof M. Gorski,A. Gregorio,Alessandro Gruppuso,Jon E. Gudmundsson,F. K. Hansen,D. L. Harrison,George Helou,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,E. Keihänen,Reijo Keskitalo,Theodore Kisner,J. Knoche,Martin Kunz,Hannu Kurki-Suonio,G. Lagache,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,R. Leonardi,François Levrier,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,Gianmarco Maggio,Davide Maino,Nazzareno Mandolesi,Anna Mangilli,Michele Maris,Peter G. Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Alessandro Melchiorri,A. Mennella,M. Migliaccio,S. Mitra,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Federico Nati,Paolo Natoli,Nicole P. H. Nesvadba,F. Noviello,Dmitry Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,Daniela Paoletti,B. Partridge,Fabio Pasian,T. J. Pearson,O. Perdereau,L. Perotto,Valeria Pettorino,F. Piacentini,M. Piat,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,M. Reinecke,Mathieu Remazeilles,C. Renault,A. Renzi,I. Ristorcelli,Graca Rocha,C. Rosset,M. Rossetti,G. Roudier,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,D. Santos,M. Savelainen,Giorgio Savini,Douglas Scott,Locke D. Spencer,V. Stolyarov,R. Stompor,R. V. Sudiwala,R. A. Sunyaev,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,M. Tristram,M. Tucci,M. Turler,G. Umana,Luca Valenziano,Jussi-Pekka Väliviita,B. Van Tent,P. Vielva,Fabrizio Villa,Lawrence A. Wade,B. D. Wandelt,Ingunn Kathrine Wehus,Niraj Welikala,D. Yvon,Andrea Zacchei,Andrea Zonca +187 more
TL;DR: In this article, a combination of Planck and IRAS data was used to select the most luminous cold submm sources with spectral energy distributions peaking between 353 and 857GHz at 5' resolution.
Journal ArticleDOI
Planck intermediate results. XLIII. The spectral energy distribution of dust in clusters of galaxies
R. Adam,P. A. R. Ade,Nabila Aghanim,M. Ashdown,Jonathan Aumont,C. Baccigalupi,R. B. Barreiro,Nicola Bartolo,E. Battaner,K. Benabed,A. Benoit-Lévy,M. Bersanelli,P. Bielewicz,I. F. Bikmaev,Anna Bonaldi,J. R. Bond,J. Borrill,F. R. Bouchet,R. A. Burenin,Carlo Burigana,E. Calabrese,J.-F. Cardoso,A. Catalano,H. C. Chiang,P. R. Christensen,E. M. Churazov,L. P. L. Colombo,C. Combet,B. Comis,F. Couchot,B. P. Crill,A. Curto,F. Cuttaia,L. Danese,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,J. Delabrouille,F.-X. Désert,Jose M. Diego,H. Dole,O. Doré,M. Douspis,A. Ducout,X. Dupac,F. Elsner,Torsten A. Enßlin,Fabio Finelli,Olivier Forni,M. Frailis,Aurelien A. Fraisse,E. Franceschi,S. Galeotta,K. Ganga,Ricardo Génova-Santos,M. Giard,Y. Giraud-Héraud,E. Gjerløw,J. González-Nuevo,A. Gregorio,Alessandro Gruppuso,Jon E. Gudmundsson,F. K. Hansen,D. L. Harrison,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,Allan Hornstrup,W. Hovest,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,W. C. Jones,E. Keihänen,R. Keskitalo,I. M. Khamitov,Theodore Kisner,R. Kneissl,J. Knoche,M. Kunz,Hannu Kurki-Suonio,G. Lagache,Anne Lähteenmäki,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,J. F. Macías-Pérez,Bruno Maffei,Gianmarco Maggio,Nazzareno Mandolesi,Anna Mangilli,Michele Maris,Pierrick Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Alessandro Melchiorri,A. Mennella,M. Migliaccio,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Pavel D. Naselsky,Federico Nati,P. Natoli,Hans Ulrik Nørgaard-Nielsen,Dmitry Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,D. Paoletti,Fabio Pasian,O. Perdereau,L. Perotto,V. Pettorino,F. Piacentini,M. Piat,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,N. Ponthieu,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Rafael Rebolo,Martin Reinecke,Mathieu Remazeilles,C. Renault,A. Renzi,I. Ristorcelli,G. Rocha,C. Rosset,M. Rossetti,G. Roudier,Jose Alberto Rubino-Martin,B. Rusholme,D. Santos,M. Savelainen,Giorgio Savini,Douglas Scott,V. Stolyarov,R. Stompor,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,Luca Valenziano,J. Valiviita,F. Van Tent,P. Vielva,F. Villa,Lawrence A. Wade,I. K. Wehus,D. Yvon,A. Zacchei,A. Zonca +178 more
TL;DR: In this paper, the spectral energy distribution (SED) of the infrared spectrum of thermal dust emission in clusters of galaxies was obtained by using a stacking approach for a sample of several hundred objects from the Planck cluster sample; this procedure averaged out fluctuations from the IR sky, allowing to reach a significant detection of the faint cluster contribution.