G
G. Polenta
Researcher at Agenzia Spaziale Italiana
Publications - 379
Citations - 104689
G. Polenta is an academic researcher from Agenzia Spaziale Italiana. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 136, co-authored 337 publications receiving 92816 citations. Previous affiliations of G. Polenta include INAF.
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Journal ArticleDOI
Is there a common origin for the WMAP low multipole and for the ellipticity in BOOMERanG CMB maps
Vahe Gurzadyan,P. A. R. Ade,P. de Bernardis,Carlo Luciano Bianco,J. J. Bock,A. Boscaleri,B. P. Crill,G. De Troia,E. Hivon,V. V. Hristov,A. L. Kashin,Andrew E. Lange,Serena Masi,P. D. Mauskopf,T. E. Montroy,P. Natoli,Calvin B. Netterfield,Enzo Pascale,F. Piacentini,G. Polenta,J. E. Ruhl,G. Yegorian +21 more
TL;DR: In this paper, the authors measured the ellipticity of several degree scale anisotropies in the BOOMERanG maps of the Cosmic Microwave Background (CMB) at 150 GHz.
Posted Content
QUBIC II: Spectro-Polarimetry with Bolometric Interferometry
L. Mousset,Gamboa Lerena,Elia S. Battistelli,P. de Bernardis,P. Chanial,Giuseppe D'Alessandro,G. Dashyan,M. De Petris,L. Grandsire,J.-Ch. Hamilton,F. Incardona,S. Landau,S. Marnieros,Silvia Masi,A. Mennella,Créidhe O'Sullivan,M. Piat,G. Ricciardi,C. Scóccola,M. Stolpovskiy,A. Tartari,J.-P. Thermeau,Steve Torchinsky,F. Voisin,Mario Zannoni,P. A. R. Ade,J.G. Alberro,Alejandro Almela,G. Amico,L. H. Arnaldi,D. Auguste,J. Aumont,S. Azzoni,S. Banfi,B. Bélier,A. Baù,D. Bennett,L. Bergé,J.-Ph. Bernard,Marco Bersanelli,M.-A. Bigot-Sazy,J. Bonaparte,J. Bonis,E. Bunn,D. L. Burke,D. Buzi,Francesco Cavaliere,C. Chapron,R. Charlassier,A.C. Cobos Cerutti,F. Columbro,Alessandro Coppolecchia,G. de Gasperis,M. De Leo,S. Dheilly,C. Duca,L. Dumoulin,A. Etchegoyen,A. Fasciszewski,L.P. Ferreyro,D. Fracchia,Cristian Franceschet,K. Ganga,Bruce Rafael Mellado Garcia,M. E. García Redondo,M. Gaspard,D. Gayer,M. Gervasi,M. Giard,V. Gilles,Y. Giraud-Héraud,M. Gómez Berisso,M. González,Marcin Gradziel,Matías Rolf Hampel,D. Harari,Sophie Henrot-Versille,E. Jules,Jean Kaplan,C. Kristukat,Luca Lamagna,S. Loucatos,Thibaut Louis,Bruno Maffei,W. Marty,A. Mattei,Andrew May,Mark McCulloch,L. Mele,D. Melo,L. Montier,L. M. Mundo,J. A. Murphy,J.D. Murphy,Federico Nati,E. Olivieri,C. Oriol,Alessandro Paiella,F. Pajot,A. Passerini,H. Pastoriza,A. Pelosi,C. Perbost,M. Perciballi,Federico Pezzotta,F. Piacentini,Lucio Piccirillo,G. Pisano,M. Platino,G. Polenta,D. Prêle,R. Puddu,Damien Rambaud,E. Rasztocky,P. Ringegni,Gustavo E. Romero,J.M. Salum,A. Schillaci,S. Scully,S. Spinelli,G. Stankowiak,A.D. Supanitsky,Peter T. Timbie,M. Tomasi,G. S. Tucker,C. Tucker,D. Viganò,Nicola Vittorio,F. Wicek,M. Wright,A. Zullo +130 more
TL;DR: In this article, the point spread function as a function of frequency was characterized for point source reconstruction and Galactic dust mapping using the Q \& U Bolometric Interferometer for Cosmology (QUBIC) and the authors concluded that spectro-imaging performance is nearly optimal up to five sub-bands in the case of QUBIC.
Peer Review
The Future of Gamma-Ray Experiments in the MeV-EeV Range
Kristi Engel,J. A. Goodman,Petra Huentemeyer,Carolyn Kierans,Tiffany R. Lewis,M. Negro,Marcos Santander,David R. Williams,Alice Allen,Tsuguo Aramaki,R. Alves Batista,Mathieu Benoit,Peter F. Bloser,Jen Bohon,Aleksey E. Bolotnikov,Isabella Brewer,Michael S. Briggs,Chad Brisbois,J. Michael Burgess,Eric Burns,Regina Caputo,Gabriella Carini,S. Bradley Cenko,Eric Charles,Stefano Ciprini,Valerio D'Elia,Tansu Daylan,J. Distel,Axel Donath,W. S. Duvall,Henrike Fleischhack,C. Fletcher,Wen Fe Fong,Dario Gasparrini,Marco Giardino,Adam Goldstein,S. Griffin,J. E. Grove,Rachel Hamburg,J. P. Harding,Jeremy Hare,Boyan Hristov,C. M. Hui,T. R. Jaffe,Peter Jenke,Oleg Kargaltsev,C. Karwin,Matthew Kerr,Dongsung Kim,Daniel Kocevski,John Krizmanic,Ranjan Laha,N. Di Lalla,Jason S. Legere,C. Leto,Richard Leys,F. Lucarelli,I. Martinez-Castellanos,A. Maselli,M. N. Mazziotta,Mark L. McConnell,Julie McEnery,Jessica Metcalfe,Manuel Meyer,A. A. Moiseev,Reshmi Mukherjee,Keiichi Ogasawara,Nicola Omodei,Ivan Peric,J. S. Perkins,M. Perri,C. Pittori,G. Polenta,D. Poulson,Robert D. Preece,Giacomo Principe,Judith Racusin,Oliver J. Roberts,Nicholas L. Rodd,P. Shawhan,T. A. Shutt,Clio Sleator,Alan P. Smale,John Smedley,Jacob Smith,Jay D. Tasson,Peter Teuben,John A. Tomsick,Péter Veres,F. Verrecchia,Zorawar Wadiasingh,Colleen A. Wilson-Hodge,Joshua Wood,Richard S. Woolf,Hui Yan,Bing Zhang,Hao Zhang,Andreas Zoglauer +97 more
TL;DR: Gamma-rays, the most energetic photons, carry information from the far reaches of extragalactic space with minimal interaction or loss of information as mentioned in this paper , and they bring messages about particle acceleration in environments so extreme they cannot be reproduced on earth for a closer look.
Journal ArticleDOI
Euclid preparation: XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography
O. Ilbert,S. de la Torre,N. Martinet,A. H. Wright,S. Paltani,C. Laigle,I. Davidzon,Eric Jullo,Hendrik Hildebrandt,D. Masters,A. Amara,C. J. Conselice,Stefano Andreon,Natalia Auricchio,Ruyman Azzollini,C. Baccigalupi,A. Balaguera-Antolínez,Marco Baldi,A. Balestra,S. Bardelli,R. Bender,Andrea Biviano,C. Bodendorf,D. Bonino,Stefano Borgani,A. Boucaud,Enrico Bozzo,E. Branchini,Massimo Brescia,Carlo Burigana,Remi A. Cabanac,Stefano Camera,V. Capobianco,A. Cappi,Carmelita Carbone,J. Carretero,C. S. Carvalho,S. Casas,F. J. Castander,M. Castellano,Gianluca Castignani,Stefano Cavuoti,A. Cimatti,R. Cledassou,C. Colodro-Conde,G. Congedo,L. Conversi,Y. Copin,Leonardo Corcione,Anne Costille,Jean Coupon,Hélène M. Courtois,Mark Cropper,J. G. Cuby,A. Da Silva,H. Degaudenzi,D. Di Ferdinando,F. Dubath,C. A. J. Duncan,X. Dupac,S. Dusini,Anne Ealet,M. H. Fabricius,S. Farrens,Pedro G. Ferreira,Fabio Finelli,P. Fosalba,Sotiria Fotopoulou,E. Franceschi,P. Franzetti,S. Galeotta,B. Garilli,W. Gillard,B. Gillis,C. Giocoli,Ghassem Gozaliasl,Javier Graciá-Carpio,Frank Grupp,Luigi Guzzo,Stein Vidar Hagfors Haugan,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,Elisabetta Maiorano,Ole Marggraf,K. Markovic,Federico Marulli,Richard Massey,Matteo Maturi,N. Mauri,S. Maurogordato,H. J. McCracken,E. Medinaceli,Simona Mei,R. Benton Metcalf,Michele Moresco,B. Morin,L. Moscardini,E. Munari,R. Nakajima,C. Neissner,S. Niemi,J. Nightingale,C. Padilla,Fabio Pasian,L. Patrizii,K. Pedersen,R. Pello,V. 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,Emanuel Rossetti,R. P. Saglia,Ariel G. Sánchez,Domenico Sapone,Peter Schneider,Tim Schrabback,V. Scottez,A. Secroun,G. Seidel,S. Serrano,Chiara Sirignano,G. Sirri,L. Stanco,F. Sureau,P. Tallada Crespí,M. Tenti,Harry Teplitz,Ismael Tereno,Rafael Toledo-Moreo,F. Torradeflot,Andrea Tramacere,Edwin A. Valentijn,Luca Valenziano,J. Valiviita,T. Vassallo,Yu Wang,Niraj Welikala,Jochen Weller,L. Whittaker,A. Zacchei,G. Zamorani,Julien Zoubian,E. Zucca +163 more
TL;DR: In this paper, the authors investigated the possibility of measuring the galaxy mean redshift with an accuracy better than 0.2 99.8% in ten tomographic bins spanning the redshift interval.
Journal ArticleDOI
Polarization angle requirements for CMB B-mode experiments. Application to the LiteBIRD satellite
P. Vielva,E. Mart'inez-Gonz'alez,F. J. Casas,Tomotake Matsumura,Sophie Henrot-Versille,Eiichiro Komatsu,J. Aumont,R. Aurlien,Carlo Baccigalupi,A. J. Banday,R. B. Barreiro,N. Bartolo,Erminia Calabrese,K. Cheung,F. Columbro,Alessandro Coppolecchia,P. de Bernardis,T. de Haan,Enrique De La Hoz,Marco De Petris,S. Della Torre,P. Diego-Palazuelos,H. K. Eriksen,Josquin Errard,Fabio Finelli,Cristian Franceschet,Unni Irene Fuskeland,Matt Galloway,K. Ganga,Massimo Gervasi,Ricardo Genova-Santos,T. Ghigna,E. Gjerløw,Alessandro Gruppuso,Masashi Hazumi,D. Herranz,E. Hivon,Kumiko Kohri,Luca Lamagna,Christophe Leloup,J. F. Macías-Pérez,Silvia Masi,Frederick Matsuda,Gianluca Morgante,Ryo Nakano,Federico Nati,Paolo Natoli,S. Nerval,Kiyoyuki Odagiri,Shugo Oguri,L. Pagano,Alessandro Paiella,Daniela Paoletti,F. Piacentini,G. Polenta,Giuseppina Emma Puglisi,Mathieu Remazeilles,A. Ritacco,Jose Alberto Rubino-Martin,Douglas Scott,Yusuke Sekimoto,Mitsuaki Shiraishi,Giovanni Signorelli,S. Takakura,Andrea Tartari,K. L. Thompson,M. Tristram,Luc Vacher,Nicola Vittorio,Ingunn Kathrine Wehus,Mario Zannoni +70 more
TL;DR: In this article , the uncertainties in the polarization angle of each detector set are related to a given bias on the tensor-to-scalar ratio r parameter, and a methodology to provide the requirements for different sets of detectors, at a given frequency of a CMB polarization experiment is presented.