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
Euclid preparation: VI. Verifying the Performance of Cosmic Shear Experiments
P. Paykari,T. Kitching,Henk Hoekstra,Ruyman Azzollini,V. F. Cardone,Mark Cropper,C. A. J. Duncan,Arun Kannawadi,Lance Miller,H. Aussel,Ian Fenech Conti,Natalia Auricchio,Marco Baldi,S. Bardelli,Andrea Biviano,D. Bonino,E. Borsato,Enrico Bozzo,E. Branchini,S. Brau-Nogue,Massimo Brescia,Jarle Brinchmann,Carlo Burigana,Stefano Camera,V. Capobianco,Carmelita Carbone,J. Carretero,F. J. Castander,Marco Castellano,Stefano Cavuoti,Y. Charles,R. Cledassou,C. Colodro-Conde,G. Congedo,C. J. Conselice,L. Conversi,Y. Copin,Jean Coupon,Hélène M. Courtois,A. Da Silva,X. Dupac,Giulio Fabbian,S. Farrens,Pedro G. Ferreira,P. Fosalba,N. Fourmanoit,M. Frailis,M. Fumana,S. Galeotta,B. Garilli,W. Gillard,B. Gillis,C. Giocoli,Javier Graciá-Carpio,Frank Grupp,Felix Hormuth,S. Ilić,H. Israel,Knud Jahnke,E. Keihänen,S. Kermiche,M. Kilbinger,C. C. Kirkpatrick,B. Kubik,M. Kunz,Hannu Kurki-Suonio,F. Lacasa,R. J. Laureijs,D. Le Mignant,Sebastiano Ligori,P. B. Lilje,I. Lloro,Thierry Maciaszek,Elisabetta Maiorano,Ole Marggraf,M. Martinelli,N. Martinet,F. Marulli R. Massey,N. Mauri,E. Medinaceli,Simona Mei,Yannick Mellier,Massimo Meneghetti,R. B. Metcalf,Michele Moresco,Lauro Moscardini,E. Munari,C. Neissner,Robert C. Nichol,S. Niemi,T. Nutma,C. Padilla,S. Paltani,Fabio Pasian,V. Pettorino,S. Pires,G. Polenta,Alkistis Pourtsidou,F. Raison,A. Renzi,Jason Rhodes,E. Romelli,Mauro Roncarelli,Emanuel Rossetti,Roberto P. Saglia,Ariel G. Sánchez,Domenico Sapone,R. Scaramella,Peter Schneider,Tim Schrabback,V. Scottez,A. Secroun,S. Serrano,Chiara Sirignano,G. Sirri,L. Stanco,Jean-Luc Starck,F. Sureau,P. Tallada-Crespí,Angela C. Taylor,M. Tenti,Ismael Tereno,Rafael Toledo-Moreo,F. Torradeflot,Isaac Tutusaus,Luca Valenziano,Martin Vannier,T. Vassallo,Julien Zoubian,E. Zucca +129 more
TL;DR: In this article, an end-to-end approach that introduces sources of bias in a modelled weak lensing survey on a galaxy-by-galaxy level is presented.
Planck intermediate results: VI. The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusters
Peter A. R. Ade,Nabila Aghanim,M. Arnaud,M. Ashdown,F. Atrio-Barandela,J. Aumont,Carlo Baccigalupi,Amedeo Balbi,A. J. Banday,A. J. Banday,R. B. Barreiro,James G. Bartlett,James G. Bartlett,E. Battaner,K. Benabed,K. Benabed,Alain Benoit,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,R. Bhatia,I. F. Bikmaev,Hans Böhringer,Anna Bonaldi,J. R. Bond,Julian Borrill,Julian Borrill,François R. Bouchet,François R. Bouchet,Hervé Bourdin,R. A. Burenin,Carlo Burigana,Carlo Burigana,Paolo Cabella,Jean-François Cardoso,G. Castex,A. Catalano,A. Catalano,L. Cayón,A. Chamballu,Lung-Yih Chiang,G. Chon,P. R. Christensen,David L. Clements,S. Colafrancesco,S. Colombi,S. Colombi,L. P. L. Colombo,L. P. L. Colombo,B. Comis,A. Coulais,B. P. Crill,F. Cuttaia,A. Da Silva,Håkon Dahle,Luigi Danese,R. J. Davis,P. de Bernardis,G. de Gasperis,G. de Zotti,Jacques Delabrouille,J. Démoclès,Jose M. Diego,Klaus Dolag,Herve Dole,Herve Dole,S. Donzelli,O. Doré,U. Dörl,Marian Douspis,X. Dupac,George Efstathiou,Torsten A. Enßlin,H. K. Eriksen,Fabio Finelli,I. Flores-Cacho,I. Flores-Cacho,Olivier Forni,Olivier Forni,M. Frailis,E. Franceschi,M. Frommert,S. Galeotta,K. Ganga,Ricardo Génova-Santos,M. Giard,M. Giard,Marat Gilfanov,Y. Giraud-Héraud,J. González-Nuevo,J. González-Nuevo,K. M. Górski,K. M. Górski,A. Gregorio,Alessandro Gruppuso,F. K. Hansen,D. L. Harrison,Pekka Heinämäki,A. Hempel,Sophie Henrot-Versille,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,G. Hurier,T. R. Jaffe,T. R. Jaffe,Andrew H. Jaffe,T. Jagemann,W. C. Jones,Mika Juvela,E. Keihänen,I. M. Khamitov,Theodore Kisner,R. Kneissl,R. Kneissl,J. Knoche,Lloyd Knox,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,Guilaine Lagache,Anne Lähteenmäki,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,Charles R. Lawrence,M. Le Jeune,R. Leonardi,P. B. Lilje,M. López-Caniego,G. Luzzi,J. F. Macías-Pérez,Davide Maino,N. Mandolesi,Michele Maris,Francine R. Marleau,D. J. Marshall,E. Martínez-González,Silvia Masi,Marcella Massardi,Sabino Matarrese,Pasquale Mazzotta,Simona Mei,Simona Mei,Simona Mei,Alessandro Melchiorri,Jean-Baptiste Melin,L. Mendes,A. Mennella,Subhasish Mitra,Subhasish Mitra,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,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,S. Osborne,F. Pajot,D. Paoletti,Fabio Pasian,G. Patanchon,O. Perdereau,L. Perotto,Francesca Perrotta,F. Piacentini,M. Piat,Elena Pierpaoli,R. Piffaretti,R. Piffaretti,Stéphane Plaszczynski,Etienne Pointecouteau,Etienne Pointecouteau,G. Polenta,Nicolas Ponthieu,Nicolas Ponthieu,L. Popa,T. Poutanen,T. Poutanen,G. W. Pratt,Simon Prunet,Jean-Loup Puget,Jörg P. Rachen,Rafael Rebolo,Rafael Rebolo,Martin Reinecke,Mathieu Remazeilles,Mathieu Remazeilles,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,I. Ristorcelli,Graca Rocha,Matthieu Roman,C. Rosset,M. Rossetti,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,Giorgio Savini,Douglas Scott,George F. Smoot,George F. Smoot,George F. Smoot,Jean-Luc Starck,R. V. Sudiwala,R. A. Sunyaev,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,L. Toffolatti,M. Tomasi,Matthieu Tristram,Jussi Tuovinen,Luca Valenziano,B. Van Tent,P. Vielva,F. Villa,Nicola Vittorio,Lawrence A. Wade,Benjamin D. Wandelt,Benjamin D. Wandelt,Niraj Welikala,D. Yvon,A. Zacchei,Saleem Zaroubi,Andrea Zonca +244 more
TL;DR: In this paper, the results from a deep XMM-Newton re-observation were used to build a template model to extract the total SZ signal of the PLCKG214.6+37.0 galaxy cluster.
Double prime focus camera for the F/1.14 Large Binocular Telescope
Roberto Ragazzoni,Emanuele Giallongo,Fabio Pasian,Fernando Pedichini,Adriano Fontana,Gianni Marconi,Roberto Speziali,Massimo Turatto,J. Danziger,Gabriele Cremonese,Riccardo Smareglia,Daniele Gallieni,Enzo Anaclerio,Paolo Lazzarini +13 more
TL;DR: In this article, the authors presented the most relevant features of the instrument, the optical design as well as the structural and mechanical layout of the LBT, and a brief overview of the informative facilities to be provided with the instrument and of a few science case studies that can be attacked by this instrument are also given.
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LBC: the prime focus optical imagers at the LBT telescope
Fernando Pedichini,Emanuele Giallongo,Roberto Ragazzoni,Andrea Di Paola,Adriano Fontana,Roberto Speziali,Jacopo Farinato,Andrea Baruffolo,Carlo E. Magagna,Emiliano Diolaiti,Fabio Pasian,Riccardo Smareglia,Enzo Anaclerio,Daniele Gallieni,Paolo Lazzarini +14 more
TL;DR: The Large Binocular Camera (LBC) as mentioned in this paper is the double optical imager that will be installed at the prime foci of the LBT, which is composed of two separated large field (27 arcmin FOV) cameras, one optimized for the UBV bands and the second for the VRIZ bands.
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Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses
A. Pocino,I. Tutusaus,F. J. Castander,Pablo Fosalba,Martin Crocce,Martin Crocce,A. Porredon,Stefano Camera,Stefano Camera,V. F. Cardone,S. Casas,Thomas D. Kitching,F. Lacasa,M. Martinelli,Alkistis Pourtsidou,Z. Sakr,Stefano Andreon,Natalia Auricchio,C. Baccigalupi,A. Balaguera-Antolínez,A. Balaguera-Antolínez,Marco Baldi,Marco Baldi,A. Balestra,S. Bardelli,Ralf Bender,Ralf Bender,Andrea Biviano,C. Bodendorf,D. Bonino,A. Boucaud,Enrico Bozzo,Enzo Branchini,Enzo Branchini,Massimo Brescia,Jarle Brinchmann,Carlo Burigana,Carlo Burigana,Remi A. Cabanac,V. Capobianco,A. Cappi,A. Cappi,C. S. Carvalho,Marco Castellano,Gianluca Castignani,Stefano Cavuoti,Andrea Cimatti,Andrea Cimatti,R. Cledassou,C. Colodro-Conde,G. Congedo,Christopher J. Conselice,L. Conversi,Y. Copin,Leonardo Corcione,Anne Costille,Jean Coupon,Hélène M. Courtois,Mark Cropper,Jean-Gabriel Cuby,A. Da Silva,S. de la Torre,D. Di Ferdinando,F. Dubath,C. A. J. Duncan,X. Dupac,S. Dusini,S. Farrens,Pedro G. Ferreira,I. Ferrero,Fabio Finelli,Sotiria Fotopoulou,M. Frailis,E. Franceschi,S. Galeotta,B. Garilli,W. Gillard,B. Gillis,Carlo Giocoli,Ghassem Gozaliasl,Javier Graciá-Carpio,F. Grupp,F. Grupp,Luigi Guzzo,W. A. Holmes,Felix Hormuth,Knud Jahnke,E. Keihänen,S. Kermiche,Alina Kiessling,C. C. Kirkpatrick,Martin Kunz,Hannu Kurki-Suonio,Sebastiano Ligori,P. B. Lilje,I. Lloro,Davide Maino,Davide Maino,Elisabetta Maiorano,O. Mansutti,Ole Marggraf,N. Martinet,Federico Marulli,Federico Marulli,Richard Massey,S. Maurogordato,E. Medinaceli,Simona Mei,Simona Mei,Massimo Meneghetti,Massimo Meneghetti,R. Benton Metcalf,R. Benton Metcalf,G. Meylan,Michele Moresco,Michele Moresco,B. Morin,Lauro Moscardini,Lauro Moscardini,E. Munari,R. Nakajima,C. Neissner,Robert C. Nichol,S. M. Niemi,J. Nightingale,C. Padilla,S. Paltani,Fabio Pasian,L. Patrizii,K. Pedersen,Will J. Percival,Will J. Percival,Valeria Pettorino,S. Pires,G. Polenta,M. Poncet,L. Popa,Doug Potter,Lucia Pozzetti,F. Raison,A. Renzi,Jason Rhodes,Giuseppe Riccio,E. Romelli,Mauro Roncarelli,Mauro Roncarelli,Emanuel Rossetti,Roberto P. Saglia,Roberto P. Saglia,Ariel G. Sánchez,Domenico Sapone,Roberto Scaramella,Peter Schneider,V. Scottez,A. Secroun,G. Seidel,S. Serrano,Chiara Sirignano,G. Sirri,L. Stanco,F. Sureau,Andy Taylor,M. Tenti,Ismael Tereno,Romain Teyssier,Rafael Toledo-Moreo,Andrea Tramacere,Edwin A. Valentijn,Luca Valenziano,Jussi Valiviita,Jussi Valiviita,T. Vassallo,M. Viel,Yu Wang,N. Welikala,L. Whittaker,L. Whittaker,Andrea Zacchei,G. Zamorani,Julien Zoubian,E. Zucca +180 more
TL;DR: In this paper, the authors explore how the tomographic redshift binning and depth of ground-based observations will affect the cosmological constraints expected from Euclid, and they find that bins with equal width in redshift provide a higher Figure of Merit (FoM) than equipopulated bins and that increasing the number of redshift bins from 10 to 13 improves the FoM by 35% and 15% for GCph and its combination with GGL, respectively.