N. Mandolesi
University of Ferrara
123 Papers
1K Citations
N. Mandolesi is an academic researcher from University of Ferrara. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 37, co-authored 123 publications. Previous affiliations of N. Mandolesi include INAF & Agenzia Spaziale Italiana.
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Papers
Planck 2018 results - VI. Cosmological parameters (Corrigendum)
Nabila Aghanim,Yashar Akrami,Yashar Akrami,Yashar Akrami,M. Ashdown,Jonathan Aumont,Carlo Baccigalupi,Mario Ballardini,Mario Ballardini,A. J. Banday,A. J. Banday,R. B. Barreiro,Nicola Bartolo,Nicola Bartolo,Soumen Basak,Richard A. Battye,Karim Benabed,J.-P. Bernard,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,P. Bielewicz,J. J. Bock,J. R. Bond,Julian Borrill,Julian Borrill,F. R. Bouchet,F. Boulanger,F. Boulanger,F. Boulanger,M. Bucher,M. Bucher,Carlo Burigana,Carlo Burigana,R. C. Butler,Erminia Calabrese,Jean-François Cardoso,Julien Carron,Anthony Challinor,H. C. Chiang,H. C. Chiang,Jens Chluba,L. P. L. Colombo,C. Combet,D. Contreras,B. P. Crill,F. Cuttaia,P. de Bernardis,G. de Zotti,Jacques Delabrouille,J.-M. Delouis,E. Di Valentino,Jose M. Diego,O. Doré,Marian Douspis,A. Ducout,X. Dupac,S. Dusini,George Efstathiou,Franz Elsner,Torsten A. Enßlin,H. K. Eriksen,Yabebal Fantaye,Yabebal Fantaye,Marzieh Farhang,James R. Fergusson,R. Fernandez-Cobos,Fabio Finelli,Francesco Forastieri,M. Frailis,Aurelien A. Fraisse,E. Franceschi,Andrei V. Frolov,S. Galeotta,S. Galli,Ken Ganga,Ricardo Genova-Santos,Ricardo Genova-Santos,Martina Gerbino,Tuhin Ghosh,Tuhin Ghosh,J. González-Nuevo,K. M. Górski,K. M. Górski,Steven Gratton,Alessandro Gruppuso,Jon E. Gudmundsson,Jon E. Gudmundsson,Jan Hamann,Will Handley,F. K. Hansen,D. Herranz,S. R. Hildebrandt,E. Hivon,Zhiqi Huang,Andrew H. Jaffe,W. C. Jones,A. Karakci,E. Keihänen,Reijo Keskitalo,K. Kiiveri,K. Kiiveri,J. B. Kim,Theodore Kisner,Lloyd Knox,Nicoletta Krachmalnicoff,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,Hannu Kurki-Suonio,Guilaine Lagache,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,M. Le Jeune,P. Lemos,Julien Lesgourgues,François Levrier,Antony Lewis,Michele Liguori,Michele Liguori,P. B. Lilje,M. Lilley,V. Lindholm,V. Lindholm,M. López-Caniego,Philip Lubin,Yin-Zhe Ma,Yin-Zhe Ma,J. F. Macías-Pérez,Gianmarco Maggio,Davide Maino,Davide Maino,N. Mandolesi,N. Mandolesi,A. Mangilli,A. Marcos-Caballero,Michele Maris,Peter G. Martin,M. Martinelli,E. Martínez-González,Sabino Matarrese,Sabino Matarrese,N. Mauri,Jason D. McEwen,Peter Meinhold,Alessandro Melchiorri,A. Mennella,A. Mennella,M. Migliaccio,Marius Millea,Marius Millea,Marius Millea,Subhasish Mitra,Subhasish Mitra,Marc-Antoine Miville-Deschênes,Marc-Antoine Miville-Deschênes,Diego Molinari,Diego Molinari,L. Montier,L. Montier,Gianluca Morgante,Adam Moss,Paolo Natoli,Paolo Natoli,Hans Ulrik Nørgaard-Nielsen,L. Pagano,L. Pagano,Daniela Paoletti,B. Partridge,G. Patanchon,Hiranya V. Peiris,Francesca Perrotta,Valeria Pettorino,F. Piacentini,L. Polastri,G. Polenta,J.-L. Puget,J.-L. Puget,Jörg P. Rachen,Martin Reinecke,Mathieu Remazeilles,A. Renzi,Graca Rocha,C. Rosset,G. Roudier,G. Roudier,G. Roudier,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,B. Ruiz-Granados,B. Ruiz-Granados,L. Salvati,M. Sandri,M. Savelainen,M. Savelainen,M. Savelainen,Douglas Scott,E. P. S. Shellard,Chiara Sirignano,Chiara Sirignano,G. Sirri,Locke D. Spencer,R. A. Sunyaev,R. A. Sunyaev,A.-S. Suur-Uski,A.-S. Suur-Uski,Jan Tauber,D. Tavagnacco,D. Tavagnacco,M. Tenti,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tomasi,Tiziana Trombetti,Luca Valenziano,Jussi Valiviita,Jussi Valiviita,B. Van Tent,L. Vibert,L. Vibert,P. Vielva,F. Villa,Nicola Vittorio,Benjamin D. Wandelt,Ingunn Kathrine Wehus,Martin White,Simon D. M. White,Andrea Zacchei,Andrea Zonca +232 more
TL;DR: Aghanim et al. as mentioned in this paper used the same data set to derive a 95% upper bound of 0.020 using the principal component analysis (PCA) model and uniform priors on the PCA mode amplitudes.
Planck 2015 results - XVII. Constraints on primordial non-Gaussianity
Peter A. R. Ade,Nabila Aghanim,Monique Arnaud,Frederico Arroja,Frederico Arroja,M. Ashdown,J. Aumont,Carlo Baccigalupi,Mario Ballardini,A. J. Banday,A. J. Banday,R. B. Barreiro,N. Bartolo,N. Bartolo,S. Basak,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,J. J. Bock,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,Julian Borrill,François R. Bouchet,Francois Boulanger,M. Bucher,Carlo Burigana,Carlo Burigana,R. C. Butler,Erminia Calabrese,Jean-François Cardoso,Jean-François Cardoso,Jean-François Cardoso,A. Catalano,Anthony Challinor,A. Chamballu,A. Chamballu,A. Chamballu,H. C. Chiang,H. C. Chiang,P. R. Christensen,Sarah E. Church,David L. Clements,S. Colombi,L. P. L. Colombo,L. P. L. Colombo,C. Combet,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,F.-X. Désert,Jose M. Diego,H. Dole,H. Dole,S. Donzelli,Olivier Doré,Marian Douspis,A. Ducout,A. Ducout,X. Dupac,George Efstathiou,F. Elsner,F. Elsner,Torsten A. Enßlin,H. K. Eriksen,James R. Fergusson,Fabio Finelli,Olivier Forni,Olivier Forni,M. Frailis,A. A. Fraisse,E. Franceschi,A. Frejsel,S. Galeotta,S. Galli,K. Ganga,C. Gauthier,C. Gauthier,Tuhin Ghosh,M. Giard,M. Giard,Y. Giraud-Héraud,E. Gjerløw,J. González-Nuevo,J. González-Nuevo,Krzysztof M. Gorski,Krzysztof M. Gorski,Serge Gratton,A. Gregorio,A. Gregorio,Alessandro Gruppuso,Jon E. Gudmundsson,Jon E. Gudmundsson,Jan Hamann,Jan Hamann,F. K. Hansen,Duncan Hanson,Duncan Hanson,Duncan Hanson,D. L. Harrison,Alan Heavens,George Helou,Sophie Henrot-Versille,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Zhiqi Huang,Kevin M. Huffenberger,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,T. R. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,Reijo Keskitalo,J. B. Kim,Theodore Kisner,J. Knoche,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,F. Lacasa,F. Lacasa,Guilaine Lagache,Guilaine Lagache,Anne Lähteenmäki,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,R. Leonardi,Julien Lesgourgues,Julien Lesgourgues,François Levrier,Antony Lewis,Michele Liguori,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,G. Maggio,Davide Maino,Davide Maino,N. Mandolesi,N. Mandolesi,A. Mangilli,A. Mangilli,Domenico Marinucci,Michele Maris,Peter G. Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Sabino Matarrese,P. M. McGehee,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,Moritz Münchmeyer,Dipak Munshi,J. A. Murphy,Pavel Naselsky,Federico Nati,Paolo Natoli,Paolo Natoli,Paolo Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,I. D. Novikov,Carol Anne Oxborrow,F. Paci,L. Pagano,F. Pajot,Daniela Paoletti,Fabio Pasian,G. Patanchon,Hiranya V. Peiris,O. Perdereau,L. Perotto,Francesca Perrotta,Valeria Pettorino,F. Piacentini,M. Piat,Elena Pierpaoli,Davide Pietrobon,Stéphane Plaszczynski,Etienne Pointecouteau,Etienne Pointecouteau,G. Polenta,L. Popa,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,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,M. Sandri,D. Santos,M. Savelainen,Giorgio Savini,Douglas Scott,M. D. Seiffert,E. P. S. Shellard,Maresuke Shiraishi,Maresuke Shiraishi,Kendrick M. Smith,Locke D. Spencer,V. Stolyarov,V. Stolyarov,V. Stolyarov,Radek Stompor,R. V. Sudiwala,R. A. Sunyaev,R. A. Sunyaev,Paul M. Sutter,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,Luca Terenzi,L. Toffolatti,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tomasi,M. Tristram,A. Troja,M. Tucci,J. Tuovinen,Luca Valenziano,Jussi-Pekka Väliviita,B. Van Tent,P. Vielva,F. Villa,L. A. Wade,Benjamin D. Wandelt,Benjamin D. Wandelt,Ingunn Kathrine Wehus,Ingunn Kathrine Wehus,D. Yvon,Andrea Zacchei,Andrea Zonca +309 more
TL;DR: In this article, the Planck full mission cosmic microwave background (CMB) temperature and E-mode polarization maps are analysed to obtain constraints on primordial non-Gaussianity (NG).
Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts
Peter A. R. Ade,Nabila Aghanim,Monique Arnaud,M. Ashdown,J. Aumont,Carlo Baccigalupi,A. J. Banday,A. J. Banday,R. B. Barreiro,James G. Bartlett,Nicola Bartolo,Nicola Bartolo,E. Battaner,Richard A. Battye,K. Benabed,Alain Benoit,A. Benoit-Lévy,A. Benoit-Lévy,J.-P. Bernard,J.-P. Bernard,Marco Bersanelli,P. Bielewicz,P. Bielewicz,J. J. Bock,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,Julian Borrill,François R. Bouchet,M. Bucher,Carlo Burigana,Carlo Burigana,R. C. Butler,Erminia Calabrese,Jean-François Cardoso,Jean-François Cardoso,Jean-François Cardoso,A. Catalano,A. Catalano,Anthony Challinor,A. Chamballu,A. Chamballu,A. Chamballu,Ranga-Ram Chary,H. C. Chiang,P. R. Christensen,Sarah E. Church,David L. Clements,Stéphane Colombi,L. P. L. Colombo,C. Combet,B. Comis,F. Couchot,A. Coulais,B. P. Crill,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,F.-X. Désert,Jose M. Diego,Klaus Dolag,H. Dole,H. Dole,S. Donzelli,Olivier Doré,Marian Douspis,A. Ducout,A. Ducout,X. Dupac,George Efstathiou,F. Elsner,F. Elsner,Torsten A. Enßlin,H. K. Eriksen,E. Falgarone,James R. Fergusson,Fabio Finelli,Olivier Forni,Olivier Forni,M. Frailis,Aurelien A. Fraisse,E. Franceschi,A. Frejsel,S. Galeotta,S. Galli,K. Ganga,M. Giard,M. Giard,Y. Giraud-Héraud,E. Gjerløw,J. González-Nuevo,J. González-Nuevo,Krzysztof M. Gorski,Steven Gratton,A. Gregorio,A. Gregorio,Alessandro Gruppuso,Jon E. Gudmundsson,Jon E. Gudmundsson,Jon E. Gudmundsson,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,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,T. R. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,Reijo Keskitalo,Theodore Kisner,R. Kneissl,J. Knoche,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,Guilaine Lagache,Guilaine Lagache,Anne Lähteenmäki,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,R. Leonardi,J. Lesgourgues,J. Lesgourgues,François Levrier,Michele Liguori,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Gianmarco Maggio,Davide Maino,N. Mandolesi,N. Mandolesi,A. Mangilli,Michele Maris,Peter G. Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Sabino Matarrese,P. M. McGehee,Peter Meinhold,Alessandro Melchiorri,Jean-Baptiste Melin,L. Mendes,A. Mennella,M. Migliaccio,Subhabrata Mitra,Subhabrata Mitra,Marc-Antoine Miville-Deschênes,Marc-Antoine Miville-Deschênes,A. Moneti,L. Montier,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Adam Moss,Dipak Munshi,J. A. Murphy,Pavel Naselsky,Federico Nati,Paolo Natoli,Paolo Natoli,Paolo Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,Carol Anne Oxborrow,F. Paci,L. Pagano,F. Pajot,Daniela Paoletti,B. Partridge,Fabio Pasian,G. Patanchon,T. J. Pearson,O. Perdereau,L. Perotto,Francesca Perrotta,Valeria Pettorino,F. Piacentini,M. Piat,Elena Pierpaoli,Davide Pietrobon,Stéphane Plaszczynski,Etienne Pointecouteau,Etienne Pointecouteau,G. Polenta,G. Polenta,L. Popa,G. W. Pratt,G. Prézeau,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,Matthieu Roman,C. Rosset,M. Rossetti,G. Roudier,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,D. Santos,M. Savelainen,Giorgio Savini,Douglas Scott,Michael Seiffert,E. P. S. Shellard,Locke D. Spencer,V. Stolyarov,Radek Stompor,R. V. Sudiwala,R. A. Sunyaev,R. A. Sunyaev,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,L. Toffolatti,L. Toffolatti,M. Tomasi,Matthieu Tristram,M. Tucci,J. Tuovinen,Marc Türler,G. Umana,Luca Valenziano,Jussi Valiviita,B. Van Tent,P. Vielva,F. Villa,L. A. Wade,Benjamin D. Wandelt,Benjamin D. Wandelt,Ingunn Kathrine Wehus,Jochen Weller,Simon D. M. White,D. Yvon,A. Zacchei,Andrea Zonca +285 more
TL;DR: In this article, the authors presented cluster counts and corresponding cosmological constraints from the Planck full mission data set and extended their analysis to the two-dimensional distribution in redshift and signal-to-noise.
Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies
Nabila Aghanim,M. Ashdown,J. Aumont,Carlo Baccigalupi,Mario Ballardini,A. J. Banday,A. J. Banday,R. B. Barreiro,N. Bartolo,N. Bartolo,S. Basak,K. Benabed,J.-P. Bernard,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,P. Bielewicz,P. Bielewicz,Laura Bonavera,J. R. Bond,Julian Borrill,Julian Borrill,François R. Bouchet,Francois Boulanger,Carlo Burigana,Carlo Burigana,Erminia Calabrese,Jean-François Cardoso,Jean-François Cardoso,Jean-François Cardoso,Julien Carron,H. C. Chiang,H. C. Chiang,L. P. L. Colombo,L. P. L. Colombo,Barbara Comis,F. Couchot,A. Coulais,B. P. Crill,A. Curto,A. Curto,F. Cuttaia,P. de Bernardis,G. de Zotti,G. de Zotti,Jacques Delabrouille,E. Di Valentino,Clive Dickinson,Jose M. Diego,Olivier Doré,Marian Douspis,A. Ducout,A. Ducout,X. Dupac,S. Dusini,F. Elsner,F. Elsner,Torsten A. Enßlin,H. K. Eriksen,Edith Falgarone,Yabebal Fantaye,Fabio Finelli,Francesco Forastieri,M. Frailis,A. A. Fraisse,E. Franceschi,Andrei V. Frolov,S. Galeotta,S. Galli,K. Ganga,Ricardo Genova-Santos,Ricardo Genova-Santos,M. Gerbino,M. Gerbino,Tuhin Ghosh,Y. Giraud-Héraud,J. González-Nuevo,J. González-Nuevo,Krzysztof M. Gorski,Krzysztof M. Gorski,Alessandro Gruppuso,Jon E. Gudmundsson,Jon E. Gudmundsson,F. K. Hansen,George Helou,Sophie Henrot-Versille,D. Herranz,E. Hivon,Zhiqi Huang,Andrew H. Jaffe,W. C. Jones,E. Keihänen,Reijo Keskitalo,K. Kiiveri,Theodore Kisner,Nicoletta Krachmalnicoff,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,J.-M. Lamarre,Mathieu Langer,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,M. Le Jeune,François Levrier,P. B. Lilje,M. Lilley,V. Lindholm,M. López-Caniego,Yin-Zhe Ma,J. F. Macías-Pérez,G. Maggio,Davide Maino,Davide Maino,N. Mandolesi,N. Mandolesi,A. Mangilli,A. Mangilli,M. Maris,Peter G. Martin,E. Martínez-González,Sabino Matarrese,Sabino Matarrese,N. Mauri,Jason D. McEwen,Alessandro Melchiorri,A. Mennella,A. Mennella,M. Migliaccio,M.-A. Miville-Deschênes,M.-A. Miville-Deschênes,D. Molinari,D. Molinari,A. Moneti,L. Montier,L. Montier,Gianluca Morgante,Adam Moss,Paolo Natoli,C. A. Oxborrow,L. Pagano,Daniela Paoletti,Guillaume Patanchon,O. Perdereau,L. Perotto,Valeria Pettorino,F. Piacentini,Stéphane Plaszczynski,L. Polastri,G. Polenta,J.-L. Puget,Jörg P. Rachen,B. Racine,M. Reinecke,Mathieu Remazeilles,A. Renzi,Graca Rocha,C. Rosset,M. Rossetti,M. Rossetti,G. Roudier,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,B. Ruiz-Granados,Laura Salvati,M. Sandri,M. Savelainen,Douglas Scott,C. Sirignano,C. Sirignano,G. Sirri,Juan D. Soler,Locke D. Spencer,A.-S. Suur-Uski,J. A. Tauber,D. Tavagnacco,M. Tenti,L. Toffolatti,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tomasi,M. Tristram,Tiziana Trombetti,Tiziana Trombetti,Jussi-Pekka Väliviita,F. Van Tent,P. Vielva,Fabrizio Villa,Nicola Vittorio,Benjamin D. Wandelt,Benjamin D. Wandelt,Ingunn Kathrine Wehus,Ingunn Kathrine Wehus,Andrea Zacchei,Andrea Zonca +197 more
TL;DR: In this article, the authors used the generalized needlet internal linear combination (GNILC) method, which uses spatial information (the angular power spectra) to disentangle the Galactic thermal dust emission from cosmic infrared background (CIB) anisotropies.
Exploring cosmic origins with CORE: Survey requirements and mission design
Jacques Delabrouille,P. de Bernardis,François R. Bouchet,Ana Achúcarro,Ana Achúcarro,Peter A. R. Ade,R. Allison,Frederico Arroja,Eduardo Artal,M. Ashdown,Carlo Baccigalupi,Mario Ballardini,Mario Ballardini,A. J. Banday,R. Banerji,Domingos Barbosa,James G. Bartlett,Nicola Bartolo,Nicola Bartolo,S. Basak,S. Basak,Jochem J. A. Baselmans,Kaustuv Basu,Elia S. Battistelli,Richard A. Battye,Daniel Baumann,Alain Benoit,Marco Bersanelli,Marco Bersanelli,Aurelien Bideaud,Marek Biesiada,Maciej Bilicki,Maciej Bilicki,A. Bonaldi,Matteo Bonato,Julian Borrill,Julian Borrill,Francois Boulanger,Thejs Brinckmann,Michael L. Brown,Martin Bucher,Carlo Burigana,Carlo Burigana,Alessandro Buzzelli,Alessandro Buzzelli,Giovanni Cabass,Zhen-Yi Cai,Martino Calvo,Andrea Caputo,C. S. Carvalho,F. J. Casas,G. Castellano,A. Catalano,Anthony Challinor,I. Charles,Jens Chluba,David L. Clements,Sebastien Clesse,Sergio Colafrancesco,I. Colantoni,D. Contreras,Alessandro Coppolecchia,Martin Crook,Giuseppe D'Alessandro,Guido D'Amico,A. Da Silva,M. A. de Avillez,M. A. de Avillez,G. de Gasperis,M. De Petris,G. de Zotti,Luigi Danese,F.-X. Désert,Vincent Desjacques,Vincent Desjacques,E. Di Valentino,E. Di Valentino,Clive Dickinson,Jose M. Diego,Simon Doyle,Ruth Durrer,Cora Dvorkin,H. K. Eriksen,Josquin Errard,Stephen M. Feeney,Stephen M. Feeney,R. Fernandez-Cobos,Fabio Finelli,Francesco Forastieri,Cristian Franceschet,U. Fuskeland,Silvia Galli,Ricardo Genova-Santos,Ricardo Genova-Santos,Martina Gerbino,Elena Giusarma,Alicia Gomez,J. González-Nuevo,Sebastian Grandis,J. Greenslade,Johannes Goupy,S. Hagstotz,Shaul Hanany,Will Handley,Sophie Henrot-Versille,Carlos Hernández-Monteagudo,C. Hervias-Caimapo,Matthew Hills,Mark Hindmarsh,Mark Hindmarsh,Mark Hindmarsh,Eric Hivon,D. T. Hoang,D. T. Hoang,Deanna C. Hooper,Bin Hu,Bin Hu,E. Keihänen,E. Keihänen,Reijo Keskitalo,Reijo Keskitalo,K. Kiiveri,K. Kiiveri,Ted Kisner,Ted Kisner,Thomas Kitching,M. Kunz,Hannu Kurki-Suonio,Hannu Kurki-Suonio,Guilaine Lagache,Luca Lamagna,Andrea Lapi,Anthony Lasenby,Massimiliano Lattanzi,A. M. C. Le Brun,Julien Lesgourgues,Michele Liguori,Michele Liguori,V. Lindholm,V. Lindholm,Joanes Lizarraga,Gemma Luzzi,J. F. Macías-Pérez,Bruno Maffei,N. Mandolesi,N. Mandolesi,S. Martin,Enrique Martinez-Gonzalez,C. J. A. P. Martins,Silvia Masi,Marcella Massardi,Sabino Matarrese,Pasquale Mazzotta,D. McCarthy,Alessandro Melchiorri,Jean-Baptiste Melin,A. Mennella,Joseph J. Mohr,Diego Molinari,Diego Molinari,Alessandro Monfardini,L. A. Montier,Paolo Natoli,Mattia Negrello,Alessio Notari,F. Noviello,F. Oppizzi,Créidhe O'Sullivan,L. Pagano,Alessandro Paiella,Enrico Pajer,Daniela Paoletti,S. Paradiso,R. B. Partridge,Guillaume Patanchon,Subodh P. Patil,O. Perdereau,F. Piacentini,M. Piat,Giampaolo Pisano,L. Polastri,Gianluca Polenta,Gianluca Polenta,Agnieszka Pollo,Nicolas Ponthieu,Vivian Poulin,Vivian Poulin,D. Prêle,Miguel Quartin,Andrea Ravenni,Mathieu Remazeilles,A. Renzi,Christophe Ringeval,Diederik Roest,Matthieu Roman,Boudewijn F. Roukema,Boudewijn F. Roukema,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,L. Salvati,Douglas Scott,Stephen Serjeant,G. Signorelli,Alexei A. Starobinsky,Alexei A. Starobinsky,Rashid Sunyaev,C. Y. Tan,A. Tartari,Gianmassimo Tasinato,Luisa Toffolatti,Luisa Toffolatti,M. Tomasi,M. Tomasi,Jesús Torrado,D. Tramonte,Neil Trappe,Sébastien Triqueneaux,Matthieu Tristram,Tiziana Trombetti,Tiziana Trombetti,M. Tucci,Carole Tucker,Jon Urrestilla,Jussi Valiviita,Jussi Valiviita,R. van de Weygaert,B. Van Tent,Vincent Vennin,Licia Verde,G. Vermeulen,P. Vielva,Nicola Vittorio,F. Voisin,Christopher G. R. Wallis,Christopher G. R. Wallis,Benjamin D. Wandelt,Ingunn Kathrine Wehus,Jochen Weller,Karl Young,Mario Zannoni,Mario Zannoni +240 more
TL;DR: The requirements for a future CMB polarisation survey addressing these scientific objectives are listed, and the design drivers of the COREmfive space mission proposed to ESA in answer to the "M5" call for a medium-sized mission are discussed.