Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Isabelle Zenone"'
Autor:
Pierre Tapie, April D. Jewell, D. Christopher Martin, Jean Evrard, Gillian Kyne, Vincent Picouet, Xavier Soors, Frederi Mirc, Jose Zorilla, Mateusz Matuszewski, Keri Hoadley, Nicole Lingner, Philippe Balard, P. Blanchard, Muriel Saccoccio, Nicolas Bray, Marty Crabill, Nicole Melso, Etienne Pirot, Donal O'Sullivan, Julia Blue Bird, Hwei Ru Ong, Shouleh Nikzad, Isabelle Zenone, David Schiminovich, Johan Montel, Robert Grange, Albert Gomes, Bruno Milliard, Michele Limon, Ramona Augustin, D. Vibert, Sandrine Pascal, Erika T. Hamden
The Faint Intergalactic Medium Redshifted Emission Balloon (FIREBall) is a mission designed to observe faint emission from the circumgalactic medium of moderate redshift (z~0.7) galaxies for the first time. FIREBall observes a component of galaxies t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a6ae8975036bb28d896b3a1c7cd934d4
http://arxiv.org/abs/2007.08528
http://arxiv.org/abs/2007.08528
Autor:
Keri Hoadley, Donal O'Sullivan, Shouleh Nikzad, Erika T. Hamden, D. Vibert, B. Smiley, Bruno Milliard, Hwei Ru Ong, Nicole Lingner, April D. Jewell, Michele Limon, Nicole Melso, Vincent Picouet, David Schiminovich, Robert Grange, Frederi Mirc, P. Balard, Johan Montel, D. Christopher Martin, Jose Zorrilla, Jean Evrard, Xavier Soors, Etienne Perot, Mateusz Matuszewski, Isabelle Zenone, Nicolas Bray, Muriel Saccoccio, Pierre Tapie, Albert Gomes, Marty Crabill, Sandrine Pascal, Gillian Kyne, Ramona Augustin, P. Blanchard, Julia Gross
Publikováno v:
Micro- and Nanotechnology Sensors, Systems, and Applications XI.
Here we discuss advances in UV technology over the last decade, with an emphasis on photon counting, low noise, high efficiency detectors in sub-orbital programs. We focus on the use of innovative UV detectors in a NASA astrophysics balloon telescope
Autor:
Pierre Tapie, Bruno Milliard, Nicolas Bray, Jean-Marc Nicot, Pascal Vola, Robert Grange, Johan Montel, Jean Evrard, David Schiminovich, Frederi Mirc, Isabelle Zenone, Etienne Perot, Albert Gomes
Publikováno v:
SPIE Proceedings.
FIREBALL (the Faint Intergalactic Redshifted Emission Balloon, funded by CNES-NASA, PI C.Martin, Caltech) is a balloon-borne 1m telescope coupled to an ultraviolet Multi Object Spectrometer (MOS), designed to study the faint and diffuse emission of t
Autor:
Pierre Lemonde, F. Picard, Ph. Laurent, Isabelle Zenone, Sébastien Bize, André Clairon, N. Ladiette, J.F. Vega, L. Guillet, I. Maksimovic, Muriel Saccoccio, C. H. Jentsch, Giorgio Santarelli, Christophe Salomon, Ch. Sirmain, M. Chaubet, Ch. Delaroche, M. Abgrall, O. Grosjean, D. Blonde
Publikováno v:
Applied Physics B-Laser and Optics
Applied Physics B-Laser and Optics, 2006, 84, pp.683-690. ⟨10.1007/s00340-006-2396-6⟩
Applied Physics B-Laser and Optics, 2006, 84, pp.683-690. ⟨10.1007/s00340-006-2396-6⟩
International audience; In this paper we describe the cold atom clock PHARAO, designed for microgravity operation. All elements of the PHARAO engineering model have been manufactured and delivered to CNES, the French space agency. We present the cloc
Autor:
Philippe Laurent, Michel Abgrall, Emilie Leynia de la Jarrige, Muriel Saccoccio, Igor Moric, M. Chaubet, Bernard Vivian, Benoit Leger, Phillipe Gase, F. Gonzalez, Philippe Chatard, Serge Beraud, Caroline Stepien, Patrizia Torresi, C. Delaroche, David Valat, Francois-Xavier Esnault, Thomas Basquin, C. Sirmain, Claude Escandes, Nadine Ladiette, Sabine Julien, Jean-Francois Vega, O. Grosjean, Didier Massonnet, Thomas Leveque, P. Guillemot, Fabrice Buffe, D. Blonde, Christophe Salomon, Benoit Faure, Lionel Fonta, Andria Ratsimandresy, Jean-Pierre Granier, Sebastien Telllier, Clement Luitot, Daniele Rovera, Isabelle Zenone, Charles-Marie de Graeve, F. Picard, Philippe Lariviere, S. Leon
Publikováno v:
2014 IEEE International Frequency Control Symposium (FCS).
PHARAO (Projet d'Horloge Atomique par Refroidissement d'Atomes en Orbite), which is being developed by the French space agency CNES, is the first primary frequency standard specially designed for operation in space. PHARAO is the main instrument of t
Autor:
Isabelle Zenone, S. Leon, T. Potier, Christophe Salomon, J.F. Vega, Ch. Macé, S. Julien, A. Ratsimandresy, Ch.M. de Graeve, Michel Abgrall, Ch. Delaroche, Pierre Lemonde, F. Gonzalez, Didier Massonnet, M. Chaubet, C. Luitot, Ph. Guillemot, O. Grosjean, D. Blonde, J. Guéna, Y. Cossart, F. Picard, B. Vivian, M. Aubourg, Ph. Larivière, J.-P. Granier, André Clairon, A. Granget, J. P. Lelay, Stéphane Thomin, Ph. Chatard, Giorgio Santarelli, Th. Nauleau, Muriel Saccoccio, Benoit Faure, S. Bize, Ph. Laurent, D. Rovera, Fabrice Buffe, N. Ladiette, B. Leger, I. Moric, Ch. Sirmain, S. Béraud, C. Escandes
Publikováno v:
Revue française de métrologie
Revue française de métrologie, 2014, 34, pp.3-21. ⟨10.1051/rfm/2014005⟩
Revue française de métrologie, Laboratoire national de métrologie et d'essais (LNE), 2014, pp.3-21. ⟨10.1051/rfm/2014005⟩
Revue française de métrologie, 2014, 34, pp.3-21. ⟨10.1051/rfm/2014005⟩
Revue française de métrologie, Laboratoire national de métrologie et d'essais (LNE), 2014, pp.3-21. ⟨10.1051/rfm/2014005⟩
CNES, LKB and SYRTE are developing a primary frequency standard, called PHARAO, which is specially designed for space applications. The clock signal is referenced on the frequency measurement of the hyperfine transition performed on a cloud of cold c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af644189e23cf74fccfd8e0b862840dc
https://hal.science/hal-02556589
https://hal.science/hal-02556589
Autor:
M. Abgrall, C. H. Jentsch, F. Picard, Isabelle Zenone, André Clairon, O. Grosjean, Christophe Salomon, M. Chaubet, D. Blonde, N. Ladiette, C. Sirmain, P. Guillemot, Giorgio Santarelli, Pierre Lemonde, J.F. Vega, C. Delaroche, P. Laurent
Publikováno v:
2007 IEEE International Frequency Control Symposium Joint with the 21st European Frequency and Time Forum.
We present the first results of the engineering model of the cold atom space clock PHARA.O. A relative frequency stability of 4.2 times 10-13t-1/2 with a quartz oscillator and of 2.5 times 10-13t-1/2 with a cryogenic oscillator have been obtained on