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.
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Papers
The TVO Archive for Cosmological Simulations: Web Services and Architecture
Alessandro Costa,P. Manzato,Ugo Becciani,M. Comparato,V. Costa,F. Gasparo,Claudio Gheller,Alessandro Grillo,Marco Molinaro,Fabio Pasian,Giuliano Taffoni +10 more
TL;DR: This work describes two Web portals as two ways to access and share complex data coming from numerical astrophysical simulations and presents a set of Web services aimed at offering services such as Simple Numeric Access (ProtocolSNAP) and Randomizers dealing with different data formats.
Euclid space mission: a cosmological challenge for the next 15 years
R. Scaramella,Yannick Mellier,J. Amiaux,Carlo Burigana,C. S. Carvalho,Jean-Charles Cuillandre,A. Da Silva,J. Dinis,A. Derosa,Elisabetta Maiorano,P. Franzetti,B. Garilli,Michele Maris,Massimo Meneghetti,Ismael Tereno,Stefanie Wachter,Luca Amendola,Mark Cropper,V. F. Cardone,Richard Massey,S. Niemi,Henk Hoekstra,T. Kitching,L. Miller,Tim Schrabback,E. Semboloni,Andrew M. Taylor,Marcos Douglas Z. Viola,Thierry Maciaszek,Anne Ealet,Luigi Guzzo,Knud Jahnke,Will J. Percival,Fabio Pasian,Marc Sauvage +34 more
TL;DR: Euclid is the next ESA mission devoted to cosmology as mentioned in this paper, which aims at observing most of the extragalactic sky, studying both gravitational lensing and clustering over $15,000 square degrees.
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.
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.
Planck 2015 results - XXV. Diffuse low-frequency Galactic foregrounds
Peter A. R. Ade,Nabila Aghanim,M. I. R. Alves,M. I. R. Alves,M. I. R. Alves,M. Arnaud,M. Ashdown,J. Aumont,Carlo Baccigalupi,A. J. Banday,A. J. Banday,R. B. Barreiro,James G. Bartlett,James G. Bartlett,N. Bartolo,N. 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,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,A. Catalano,Anthony Challinor,A. Chamballu,A. Chamballu,A. Chamballu,R.-R. Chary,H. C. Chiang,H. C. Chiang,P. R. Christensen,Stéphane Colombi,L. P. L. Colombo,L. P. L. Colombo,C. Combet,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,J.-M. Delouis,F.-X. Désert,Clive Dickinson,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,E. Falgarone,James R. Fergusson,Fabio Finelli,Olivier Forni,Olivier Forni,M. Frailis,A. A. Fraisse,E. Franceschi,A. Frejsel,S. Galeotta,S. Galli,K. Ganga,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,Jon E. Gudmundsson,F. K. Hansen,Duncan Hanson,Duncan Hanson,Duncan Hanson,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,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,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,J. P. Leahy,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,Davide Maino,N. Mandolesi,N. Mandolesi,A. Mangilli,A. Mangilli,Michele Maris,D. J. Marshall,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,Subhasish Mitra,Subhasish 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,Federico Nati,Paolo Natoli,Paolo Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,I. D. Novikov,E. Orlando,Carol Anne Oxborrow,F. Paci,L. Pagano,F. Pajot,Roberta Paladini,Daniela Paoletti,B. Partridge,Fabio Pasian,G. Patanchon,T. J. Pearson,Michael W. Peel,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,G. W. Pratt,G. Prézeau,Simon Prunet,J.-L. Puget,Jörg P. Rachen,William T. Reach,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,Locke D. Spencer,V. Stolyarov,V. Stolyarov,V. Stolyarov,Radek Stompor,Andrew W. Strong,R. V. Sudiwala,R. A. Sunyaev,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,M. Tucci,J. Tuovinen,G. Umana,Luca Valenziano,Jussi-Pekka Väliviita,F. Van Tent,Matias Vidal,P. Vielva,Fabrizio Villa,Lawrence A. Wade,B. D. Wandelt,B. D. Wandelt,Robert A. Watson,Ingunn Kathrine Wehus,Ingunn Kathrine Wehus,Althea Wilkinson,D. Yvon,Andrea Zacchei,Andrea Zonca +306 more
TL;DR: In this article, the authors discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP, and identify a number of new faint features in the polarized sky, including a dearth of polarized synchrotron emission directly correlated with a narrow, roughly 20deg long filament seen in Hα at high latitude.