F. Bernardeau
Institut d'Astrophysique de Paris
2 Papers
3 Citations
F. Bernardeau is an academic researcher from Institut d'Astrophysique de Paris. The author has contributed to research in topics: Payload & Spectral density. The author has an hindex of 1, co-authored 2 publications.
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Papers
Euclid mission status after mission critical design
René J. Laureijs,Giuseppe D. Racca,Yannick Mellier,P. Musi,L. Brouard,T. Boenke,L. Gaspar Venancio,E. Maiorano,A. Short,P. Strada,B. Altieri,G. Buenadicha,X. Dupac,P. Gomez Alvarez,J. Hoar,R. Kohley,R. Vavrek,A. Rudolph,M. Schmidt,J. Amiaux,H. Aussel,M. Berthe,Mark Cropper,J. C. Cuillandre,Christophe Dabin,José Dinis,R. Nakajima,Thierry Maciaszek,Roberto Scaramella,A. Da Silva,Ismael Tereno,O.R. Williams,Andrea Zacchei,Ruyman Azzollini,F. Bernardeau,Jarle Brinchmann,C. Brockley-Blatt,F. J. Castander,A. Cimatti,C. J. Conselice,Anne Ealet,P. Fosalba,W. Gillard,Luigi Guzzo,Henk Hoekstra,P. Hudelot,Knud Jahnke,Thomas D. Kitching,Lance Miller,Joseph J. Mohr,Will J. Percival,Valeria Pettorino,Jason Rhodes,Ariel G. Sánchez,Marc Sauvage,S. Serrano,Romain Teyssier,Jochen Weller,Julien Zoubian +58 more
- 13 Dec 2020
TL;DR: The status of the main elements of the Euclid mission is presented in the light of the demanding high optical performance which is the essential design driver is the to meet the scientific requirements.
•Posted Content
Euclid: Forecasts for $k$-cut $3 \times 2$ Point Statistics
Peter Taylor,T. Kitching,V. F. Cardone,Agnès Ferté,E. M. Huff,F. Bernardeau,Jason Rhodes,A. C. Deshpande,I. Tutusaus,Alkistis Pourtsidou,Stefano Camera,Carmelita Carbone,S. Casas,M. Martinelli,V. Pettorino,Z. Sakr,Domenico Sapone,V. Yankelevich,Natalia Auricchio,A. Balestra,C. Bodendorf,D. Bonino,A. Boucaud,E. Branchini,Massimo Brescia,V. Capobianco,J. Carretero,Marco Castellano,Stefano Cavuoti,A. Cimatti,R. Cledassou,G. Congedo,L. Conversi,Leonardo Corcione,Mark Cropper,E. Franceschi,B. Garilli,B. Gillis,C. Giocoli,Luigi Guzzo,Stein Vidar Hagfors Haugan,W. A. Holmes,Felix Hormuth,Knud Jahnke,S. Kermiche,M. Kilbinger,M. Kunz,Hannu Kurki-Suonio,Sebastiano Ligori,P. B. Lilje,I. Lloro,Ole Marggraf,K. Markovic,Richard Massey,E. Medinaceli,Simona Mei,Massimo Meneghetti,G. Meylan,Michele Moresco,B. Morin,L. Moscardini,S. Niemi,C. Padilla,S. Paltani,Fabio Pasian,K. Pedersen,Will J. Percival,S. Pires,G. Polenta,M. Poncet,L. Popa,F. Raison,Mauro Roncarelli,Emanuel Rossetti,R. P. Saglia,Peter Schneider,A. Secrou,G. Seidel,S. Serrano,Chiara Sirignano,G. Sirri,F. Sureau,P. Tallada Crespí,Daniele Tavagnacco,Andy Taylor,Harry I. Teplitz,Ismael Tereno,Rafael Toledo-Moreo,Edwin A. Valentijn,Luca Valenziano,T. Vassallo,Yu Wang,Jochen Weller,A. Zacchei,Julien Zoubian +94 more
TL;DR: In this paper, the authors extended the Fisher matrix analysis to a point analysis of the wide field survey data, and showed that removing 50% of the observed galaxies in the photometric clustering part of the analysis decreases the dark energy Figure of Merit (FOM).
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