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
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CHIPP: INAF pilot project for HTC, HPC and HPDA
Giuliano Taffoni,Ugo Becciani,Bianca Garilli,Gianmarco Maggio,Fabio Pasian,Grazia Umana,Riccardo Smareglia,Fabio Vitello +7 more
TL;DR: The CHIPP infrastructures are described and the results of the first two years of activity are described, including HPC, data reduction and analysis, machine learning.
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Euclid: Reconstruction of weak-lensing mass maps for non-Gaussianity studies
Sandrine Pires,V. Vandenbussche,V. Kansal,Ralf Bender,Ralf Bender,Linda Blot,D. Bonino,A. Boucaud,Jarle Brinchmann,V. Capobianco,J. Carretero,Marco Castellano,Stefano Cavuoti,R. Cledassou,G. Congedo,L. Conversi,Leonardo Corcione,F. Dubath,Pablo Fosalba,M. Frailis,E. Franceschi,M. Fumana,Frank Grupp,Felix Hormuth,S. Kermiche,Mischa Knabenhans,R. Kohley,B. Kubik,Martin Kunz,Sebastiano Ligori,P. B. Lilje,Ivan Lloro,Elisabetta Maiorano,Ole Marggraf,Richard Massey,G. Meylan,C. Padilla,S. Paltani,Fabio Pasian,M. Poncet,Doug Potter,F. Raison,Jason Rhodes,Mauro Roncarelli,Mauro Roncarelli,Roberto P. Saglia,Roberto P. Saglia,Peter Schneider,A. Secroun,S. Serrano,Joachim Stadel,P. Tallada Crespí,Ismael Tereno,Rafael Toledo-Moreo,Yu Wang +54 more
TL;DR: In this article, two mass-inversion methods, the Kaiser and Squires method (KS) and the mass-mapping systematic effects (KS+), were proposed to reduce the information loss during the mass inversion.
BaSTI: An updated, advanced and VO-compliant database of stellar evolution predictions
Adriano Pietrinferni,Marco Molinaro,Santi Cassisi,Fabio Pasian,Maurizio Salaris,Danilo Pelusi,P. Manzato,Claudio Vuerli +7 more
TL;DR: The current status of the widely used BaSTI (A Bag of Stellar Tracks and Isochrones) database is described, in particular on the efforts devoted to port BaSTi to a VO-compliant environment, the Ba STI Web portal that enables users to retrieve data tables and run a range of web tools to facilitate the theoretical analysis of observations.
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Euclid: Effect of sample covariance on the number counts of galaxy clusters
A. Fumagalli,A. Saro,Stefano Borgani,Tiago Castro,M. Costanzi,Pierluigi Monaco,E. Munari,Emiliano Sefusatti,A. Amara,Natalia Auricchio,A. Balestra,C. Bodendorf,D. Bonino,E. Branchini,Jarle Brinchmann,V. Capobianco,Carmelita Carbone,M. Castellano,Stefano Cavuoti,A. Cimatti,R. Cledassou,C. J. Conselice,Leonardo Corcione,Anne Costille,Mark Cropper,H. Degaudenzi,M. Douspis,F. Dubath,S. Dusini,Anne Ealet,P. Fosalba,E. Franceschi,P. Franzetti,M. Fumana,B. Garilli,C. Giocoli,Frank Grupp,Luigi Guzzo,Stein Vidar Hagfors Haugan,Henk Hoekstra,W. A. Holmes,Felix Hormuth,Knud Jahnke,Alina Kiessling,M. Kilbinger,Thomas D. Kitching,M. Kümmel,Martin Kunz,Hannu Kurki-Suonio,R. J. Laureijs,P. B. Lilje,I. Lloro,Elisabetta Maiorano,Ole Marggraf,K. Markovic,Richard Massey,Massimo Meneghetti,G. Meylan,L. Moscardini,S. Niemi,C. Padilla,S. Paltani,Fabio Pasian,K. Pedersen,Valeria Pettorino,S. Pires,M. Poncet,L. Popa,Lucia Pozzetti,F. Raison,Jason Rhodes,Mauro Roncarelli,Emanuel Rossetti,Roberto P. Saglia,R. Scaramella,Peter Schneider,A. Secroun,G. Seidel,S. Serrano,Chiara Sirignano,G. Sirri,Andy Taylor,Ismael Tereno,Rafael Toledo-Moreo,Edwin A. Valentijn,Luca Valenziano,Yu Wang,Jochen Weller,G. Zamorani,Julien Zoubian,Massimo Brescia,G. Congedo,L. Conversi,Simona Mei,Michele Moresco,T. Vassallo +95 more
TL;DR: In this paper, the authors investigate the contribution of shot-noise and sample variance to the uncertainty of cosmological parameter constraints inferred from cluster number counts in the context of the Euclid survey.
The double Prime Focus camera for the Large Binocular Telescope
Roberto Ragazzoni,Roberto Ragazzoni,Emanuele Giallongo,Fabio Pasian,Carmelo Arcidiacono,Andrea Baruffolo,Emiliano Diolaiti,Andrea Di Paola,Fabio Faccin,Jacopo Farinato,Adriano Fontana,F. Gasparo,Fernando Pedichini,Riccardo Smareglia,Roberto Speziali,Elise Vernet +15 more
TL;DR: The Prime Focus for the Large Binocular Telescope (PF-LBT) as discussed by the authors is a two-camera system with four 4kx2k CCDs and a six lenses corrector with an aspheric surface.
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