Fabio Pasian
INAF
307 Papers
8.7K Citations
Fabio Pasian is an academic researcher from INAF. The author has contributed to research in topics: Planck & Galaxy. The author has an hindex of 99, co-authored 307 publications.
Chat about Author
Papers
Planck Early Results: The Planck View of Nearby Galaxies
P. A. R. Ade,Nabila Aghanim,M. Arnaud,M. Ashdown,Jonathan Aumont,C. Baccigalupi,Amedeo Balbi,A. J. Banday,R. B. Barreiro,J. G. Bartlett,E. Battaner,K. Benabed,Aurélien Benoit,J.-P. Bernard,Marco Bersanelli,R. S. Bhatia,J. J. Bock,Anna Bonaldi,J. R. Bond,J. Borrill,F. R. Bouchet,M. Bucher,Carlo Burigana,P. Cabella,Jean-François Cardoso,A. Catalano,L. Cayón,Anthony Challinor,A. Chamballu,Ranga-Ram Chary,Lung-Yih Chiang,P. R. Christensen,D. L. Clements,Stéphane Colombi,F. Couchot,A. Coulais,B. P. Crill,F. Cuttaia,L. Danese,R. D. Davies,R. J. Davis,P. de Bernardis,G. de Gasperis,A. de Rosa,G. de Zotti,J. Delabrouille,J.-M. Delouis,F.-X. Désert,Clive Dickinson,H. Dole,S. Donzelli,O. Doré,U. Dörl,M. Douspis,X. Dupac,George Efstathiou,Torsten A. Enßlin,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,F. K. Hansen,D. L. Harrison,George Helou,Sophie Henrot-Versille,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,W. Hovest,Roger J. Hoyland,Kevin M. Huffenberger,Andrew H. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,R. Keskitalo,Theodore Kisner,R. Kneissl,Lloyd Knox,Hannu Kurki-Suonio,G. Lagache,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,R. J. Laureijs,Charles R. Lawrence,S. Leach,R. Leonardi,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,C. J. MacTavish,S. C. Madden,Bruno Maffei,Davide Maino,Nazzareno Mandolesi,Robert G. Mann,Michele Maris,E. Martínez-González,Silvia Masi,Sabino Matarrese,F. Matthai,Pasquale Mazzotta,Alessandro Melchiorri,L. Mendes,A. Mennella,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,A. Murphy,Pavel D. Naselsky,P. Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,S. Osborne,F. Pajot,B. Partridge,Fabio Pasian,G. Patanchon,Michael W. Peel,O. Perdereau,L. Perotto,F. Perrotta,F. Piacentini,M. Piat,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,N. Ponthieu,T. Poutanen,G. Prézeau,Simon Prunet,J.-L. Puget,William T. Reach,Rafael Rebolo,Martin Reinecke,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,G. Rocha,C. Rosset,Michael Rowan-Robinson,Jose Alberto Rubino-Martin,B. Rusholme,M. Sandri,Giorgio Savini,Douglas Scott,M. D. Seiffert,P. Shellard,G. F. Smoot,Jean-Luc Starck,F. Stivoli,V. Stolyarov,R. V. Sudiwala,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,J.-P. Torre,M. Tristram,Jussi Tuovinen,M. Turler,G. Umana,Luca Valenziano,Jussi Varis,P. Vielva,F. Villa,Nicola Vittorio,Lawrence A. Wade,B. D. Wandelt,D. Yvon,A. Zacchei,A. Zonca +193 more
TL;DR: In this paper, the spectral energy distributions (SEDs) of distant submm galaxies are measured using parametric dust models to determine the range of dust temperatures and emissivities.
Planck intermediate results - XXVIII. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck
Peter A. R. Ade,Nabila Aghanim,G. Aniano,Monique Arnaud,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,Marco Bersanelli,P. Bielewicz,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,Julian Borrill,François R. Bouchet,F. Boulanger,Carlo Burigana,Carlo Burigana,R. C. Butler,Erminia Calabrese,Jean-François Cardoso,J. M. Casandjian,A. Catalano,A. Chamballu,H. C. Chiang,H. C. Chiang,P. R. Christensen,L. P. L. Colombo,L. P. L. Colombo,C. Combet,F. Couchot,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,J. Delabrouille,F.-X. Désert,Clive Dickinson,Jose M. Diego,Seth Digel,H. Dole,S. Donzelli,Olivier Doré,Marian Douspis,A. Ducout,X. Dupac,George Efstathiou,F. Elsner,Torsten A. Enßlin,H. K. Eriksen,E. Falgarone,Fabio Finelli,Olivier Forni,M. Frailis,Aurelien A. Fraisse,E. Franceschi,A. Frejsel,Yasuo Fukui,S. Galeotta,S. Galli,K. Ganga,Tuhin Ghosh,M. Giard,E. Gjerløw,J. González-Nuevo,J. González-Nuevo,K. M. Górski,K. M. Górski,A. Gregorio,A. Gregorio,I. A. Grenier,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,Michael P. Hobson,W. A. Holmes,W. Hovest,Kevin M. Huffenberger,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,Reijo Keskitalo,Theodore Kisner,R. Kneissl,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,Davide Maino,N. Mandolesi,N. Mandolesi,N. Mandolesi,Michele Maris,D. J. Marshall,Peter G. Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Pasquale Mazzotta,Alessandro Melchiorri,L. Mendes,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,Paolo Natoli,Paolo Natoli,Paolo Natoli,Hans Ulrik Nørgaard-Nielsen,Dmitry Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,Roberta Paladini,Daniela Paoletti,Fabio Pasian,O. Perdereau,L. Perotto,Francesca Perrotta,Valeria Pettorino,F. Piacentini,M. Piat,Stéphane Plaszczynski,E. Pointecouteau,G. Polenta,G. Polenta,L. Popa,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Jörg P. Rachen,William T. Reach,Rafael Rebolo,Rafael Rebolo,Martin Reinecke,Mathieu Remazeilles,C. Renault,I. Ristorcelli,Graca Rocha,G. Roudier,Ben Rusholme,M. Sandri,D. Santos,Douglas Scott,Locke D. Spencer,V. Stolyarov,V. Stolyarov,Andrew W. Strong,Rashmikant V. Sudiwala,R. A. Sunyaev,R. A. Sunyaev,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Tibaldo,L. Toffolatti,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tomasi,M. Tristram,M. Tucci,G. Umana,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 +225 more
TL;DR: In this paper, the authors compare the dust and cosmic rays in the Chamaeleon clouds with the results obtained from the Fermi Large Area Telescope (LAT) and IRAS, and provide average values for the dust properties per gas nucleon in different phases.
Euclid preparation: X. The Euclid photometric-redshift challenge
G. Desprez,S. Paltani,Jean Coupon,Ibrahim Almosallam,A. Alvarez-Ayllon,V. Amaro,Massimo Brescia,Mark Brodwin,Stefano Cavuoti,J. De Vicente-Albendea,Sotiria Fotopoulou,P. W. Hatfield,W. G. Hartley,O. Ilbert,Matt J. Jarvis,Giuseppe Longo,R. Saha,Joshua S. Speagle,Andrea Tramacere,Marco Castellano,F. Dubath,Audrey Galametz,M. Kuemmel,Clotilde Laigle,Emiliano Merlin,Joseph J. Mohr,S. Pilo,Mara Salvato,M. M. Rau,Stefano Andreon,Natalia Auricchio,C. Baccigalupi,A. Balaguera-Antolínez,Marco Baldi,S. Bardelli,R. Bender,Andrea Biviano,C. Bodendorf,D. Bonino,Enrico Bozzo,E. Branchini,Jarle Brinchmann,Carlo Burigana,Remi A. Cabanac,Stefano Camera,V. Capobianco,A. Cappi,Carmelita Carbone,J. Carretero,C. S. Carvalho,Ricard Casas,S. Casas,F. J. Castander,Gianluca Castignani,A. Cimatti,R. Cledassou,C. Colodro-Conde,G. Congedo,C. J. Conselice,L. Conversi,Y. Copin,Leonardo Corcione,Hélène M. Courtois,J. G. Cuby,A. Da Silva,S. de la Torre,H. Degaudenzi,D. Di Ferdinando,M. Douspis,C. A. J. Duncan,X. Dupac,Anne Ealet,Giulio Fabbian,M. H. Fabricius,S. Farrens,Pedro G. Ferreira,Fabio Finelli,P. Fosalba,N. Fourmanoit,M. Frailis,E. Franceschi,M. Fumana,S. Galeotta,B. Garilli,W. Gillard,B. Gillis,C. Giocoli,Ghassem Gozaliasl,Javier Graciá-Carpio,Frank Grupp,Luigi Guzzo,M. Hailey,Stein Vidar Hagfors Haugan,W. A. Holmes,Felix Hormuth,Andrew Humphrey,Knud Jahnke,E. Keihänen,S. Kermiche,M. Kilbinger,C. C. Kirkpatrick,Thomas D. Kitching,R. Kohley,B. Kubik,M. Kunz,Hannu Kurki-Suonio,Sebastiano Ligori,P. B. Lilje,I. Lloro,Davide Maino,Elisabetta Maiorano,Ole Marggraf,K. Markovic,N. Martinet,Federico Marulli,Richard Massey,Matteo Maturi,N. Mauri,S. Maurogordato,E. Medinaceli,Simona Mei,Massimo Meneghetti,R. Benton Metcalf,G. Meylan,Michele Moresco,L. Moscardini,E. Munari,S. Niemi,C. Padilla,Fabio Pasian,L. Patrizii,V. Pettorino,S. Pires,G. Polenta,M. Poncet,L. Popa,Doug Potter,Lucia Pozzetti,F. Raison,A. Renzi,Jason Rhodes,Giuseppe Riccio,Emanuel Rossetti,Roberto P. Saglia,Domenico Sapone,Peter Schneider,V. Scottez,A. Secroun,S. Serrano,Chiara Sirignano,G. Sirri,L. Stanco,D. Stern,F. Sureau,P. Tallada Crespí,Daniele Tavagnacco,Andy Taylor,M. Tenti,Ismael Tereno,Rafael Toledo-Moreo,F. Torradeflot,Luca Valenziano,J. Valiviita,T. Vassallo,Matteo Viel,Yu Wang,Niraj Welikala,L. Whittaker,A. Zacchei,G. Zamorani,Julien Zoubian,E. Zucca +171 more
TL;DR: In this article, the authors report on the performance of 13 photometric redshift code single value redshift estimates and redshift probability distributions on a common set of data, focusing particularly on the 0.2-2.6 redshift range that the Euclid mission will probe.
The Euclid mission design
Giuseppe D. Racca,René J. Laureijs,Luca Stagnaro,Jean-Christophe Salvignol,Jose Lorenzo Alvarez,Gonzalo Saavedra Criado,Luis Gaspar Venancio,Alex Short,Paolo Strada,Tobias Bönke,Cyril Colombo,Adriano Calvi,Elena Maiorano,Osvaldo Piersanti,Sylvain Prezelus,Pierluigi Rosato,Jacques Pinel,H. Rozemeijer,Valentina Lesna,Paolo Musi,Marco Sias,Alberto Anselmi,Vincent Cazaubiel,Ludovic Vaillon,Yannick Mellier,Jérôme Amiaux,Michel Berthé,Marc Sauvage,Ruyman Azzollini,Mark Cropper,S. Pottinger,Knud Jahnke,Anne Ealet,Thierry Maciaszek,Fabio Pasian,Andrea Zacchei,Roberto Scaramella,J. Hoar,R. Kohley,R. Vavrek,Andreas Rudolph,Micha Schmidt +41 more
TL;DR: Euclid as mentioned in this paper is a space-based optical/near-infrared survey mission of the European Space Agency (ESA) to investigate the nature of dark energy, dark matter and gravity by observing the geometry of the Universe and on the formation of structures over cosmological timescales.
92
Planck Early Results. II. The thermal performance of Planck
Peter A. R. Ade,Nabila Aghanim,M. Arnaud,M. Ashdown,Jonathan Aumont,C. Baccigalupi,M. D. Baker,Amedeo Balbi,A. J. Banday,R. B. Barreiro,E. Battaner,K. Benabed,Alain Benoit,J.-P. Bernard,Marco Bersanelli,Pradeep Bhandari,R. S. Bhatia,J. J. Bock,Anna Bonaldi,J. R. Bond,J. Borders,J. Borrill,François R. Bouchet,B. Bowman,Tom Bradshaw,E. Bréelle,M. Bucher,Carlo Burigana,R. C. Butler,P. Cabella,Ph. Camus,Christopher Cantalupo,B. Cappellini,Jean-François Cardoso,A. Catalano,L. Cayón,Anthony Challinor,A. Chamballu,J. P. Chambelland,J. Charra,M. Charra,Lung-Yih Chiang,C. Chiang,P. R. Christensen,D. L. Clements,B. Collaudin,Stéphane Colombi,F. Couchot,A. Coulais,B. P. Crill,Martin Crook,F. Cuttaia,C. Damasio,L. Danese,R. D. Davies,R. J. Davis,P. de Bernardis,G. de Gasperis,A. de Rosa,Jacques Delabrouille,J.-M. Delouis,F.-X. Désert,U. Doerl,Klaus Dolag,S. Donzelli,O. Doré,M. Douspis,X. Dupac,George Efstathiou,Torsten A. Enßlin,H. K. Eriksen,Fabio Finelli,Suzanne Foley,Olivier Forni,P. Fosalba,J. J. Fourmond,M. Frailis,E. Franceschi,S. Galeotta,K. Ganga,E. Gavila,M. Giard,Giovanna Giardino,Y. Giraud-Héraud,J. González-Nuevo,K. M. Górski,Steven Gratton,A. Gregorio,A. Gruppuso,G. Guyot,D. L. Harrison,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,Roger J. Hoyland,Kevin M. Huffenberger,Ulf E. Israelsson,Andrew H. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,R. Keskitalo,Theodore Kisner,R. Kneissl,Lloyd Knox,Hannu Kurki-Suonio,G. Lagache,J.-M. Lamarre,P. Lami,Anthony Lasenby,R. J. Laureijs,Charles R. Lawrence,S. Leach,R. Leonardi,Claude Leroy,P. B. Lilje,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Thierry Maciaszek,C. J. MacTavish,Bruno Maffei,Davide Maino,Nazzareno Mandolesi,Robert G. Mann,Michele Maris,E. Martínez-González,Silvia Masi,Sabino Matarrese,F. Matthai,Pasquale Mazzotta,Peregrine McGehee,Peter Meinhold,Alessandro Melchiorri,F. Melot,L. Mendes,A. Mennella,Marc-Antoine Miville-Deschenes,A. Moneti,L. Montier,J. Mora,Gianluca Morgante,N. Morisset,Daniel J. Mortlock,Dipak Munshi,Anna Murphy,Pavel D. Naselsky,A. Nash,P. Natoli,Calvin B. Netterfield,Dmitry Novikov,I. D. Novikov,I. J. O'Dwyer,S. Osborne,F. Pajot,Fabio Pasian,G. Patanchon,David Pearson,O. Perdereau,L. Perotto,F. Perrotta,F. Piacentini,M. Piat,Stéphane Plaszczynski,Paola Platania,E. Pointecouteau,G. Polenta,N. Ponthieu,T. Poutanen,G. Prézeau,M. Prina,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Rafael Rebolo,Martin Reinecke,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,G. Rocha,C. Rosset,J. A. Rubiino-Martin,Ben Rusholme,M. Sandri,D. Santos,Bjoern Malte Schaefer,Douglas Scott,M. D. Seiffert,P. Shellard,G. F. Smoot,Jean-Luc Starck,P. Stassi,F. Stivoli,V. Stolyarov,R. Stompor,R. V. Sudiwala,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,J.-P. Torre,M. Tristram,Jussi Tuovinen,Luca Valenziano,L. Vibert,P. Vielva,F. Villa,Nicola Vittorio,Lawrence A. Wade,Benjamin D. Wandelt,Christer Watson,S. D. M. White,Althea Wilkinson,P. R. Wilson,D. Yvon,A. Zacchei,B. Zhang,A. Zonca +226 more
TL;DR: In this paper, the performance of the Planck instruments in space is enabled by their low operating temperatures, 20K for LFI and 0.1K for HFI, achieved through a combination of passive radiative cooling and three active mechanical coolers.