Zobrazeno 1 - 10
of 32
pro vyhledávání: '"Muriel, Saccoccio"'
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:
G. Foënard, A. Lacourt, L. Rodriguez, I. Ristorcelli, L. Montier, Christopher Tibbs, René J. Laureijs, Peter Charles Hargrave, D. Alina, J. A. Tauber, G. de Gasperis, C. Engel, J.-Ph. Bernard, Bruno Maffei, K. Ferrière, F. Pajot, Silvia Masi, Muriel Saccoccio, Annie Hughes, P. de Bernardis, Giorgio Savini, A. M. Magalhes, E. M. de Gouveia Dal Pino, B. Mot, Etienne Perot, P. A. R. Ade, H. Roussel, Vincent Guillet, Johan Montel, Alessandro Buzzelli, Jean-Pierre Dubois, J. B. Durrive, Y. Longval, C. Marty, S. Stever, Maria Salatino, R. Misawa, Anna Mangilli, Jonathan Aumont, Carole Tucker
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 630, pp.A74. ⟨10.1051/0004-6361/201935072⟩
Astronomy and Astrophysics-A&A, 2019, 630, pp.A74. ⟨10.1051/0004-6361/201935072⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 630, pp.A74. ⟨10.1051/0004-6361/201935072⟩
Astronomy and Astrophysics-A&A, 2019, 630, pp.A74. ⟨10.1051/0004-6361/201935072⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
We present the first far infrared (FIR) dust emission polarization map covering the full extent Milky Way's Central molecular zone (CMZ). The data, obtained with the PILOT balloon-borne experiment, covers the Galactic Center region $-2\,^\circ
C
C
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c88712a3a8467b52212995f1b769a9c0
http://arxiv.org/abs/1901.06196
http://arxiv.org/abs/1901.06196
Autor:
C. Engel, F. Pajot, J. Martignac, F. Bousqet, Y. Lepennec, S. Maestre, Nicolas Bray, Matthew Joseph Griffin, Peter A. R. Ade, A. Hughes, Silvia Masi, J. Narbonne, G. Foënard, René J. Laureijs, Frederi Mirc, Christopher Tibbs, J. M. Nicot, P. deBernardis, Y. André, G. Roudil, L. Rodriguez, Pierre Tapie, L. Bautista, B. Maffei, P. Etcheto, Etienne Perot, Peter Charles Hargrave, J. A. Tauber, J. P. Dubois, S. Grabarnik, B. Mot, M. Bouzit, L. Montier, O. Boulade, C. Marty, E. Doumayrou, Giampaolo Pisano, Isabelle Ristorcelli, H. Roussel, Nicolas Ponthieu, B. Leriche, A. Mangilli, X. Dupac, C. Tucker, Ph. Gelot, Y. Longval, Giorgio Savini, A. Lacourt, J. Aumont, V. Buttice, R. Misawa, M. Charra, Johan Montel, J. Pimentao, Muriel Saccoccio, W. Marty, B. Crane, M. Chaigneau, J.-P. Bernard, G. Parot, S. Stever, Maria Salatino, O. Simonella
Publikováno v:
Experimental Astronomy
Experimental Astronomy, 2019, 48, pp.265-295. ⟨10.1007/s10686-019-09648-6⟩
Experimental Astronomy, 2019, 48, pp.265-295. ⟨10.1007/s10686-019-09648-6⟩
International audience; The Polarized Instrument for Long-wavelength Observation of the Tenuous interstellar medium (PILOT) is a balloon-borne experiment that aims to measure the polarized emission of thermal dust at a wavelength of 240 µm (1.2 THz)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0bf9e552686c12be37cd6a310ff3b79f
http://hdl.handle.net/11573/1417357
http://hdl.handle.net/11573/1417357
Publikováno v:
International Conference on Space Optics — ICSO 2000.
The new generation of atomic clocks, using cold atoms, require laser beams with high spectral quality and very fine frequency control.
Autor:
André Clairon, Jacques Loesel, Muriel Saccoccio, Yvan Aubry, Jacques Berthon, Pierre Lemonde, Nathalie Raimbault, Philippe Laurent
Publikováno v:
International Conference on Space Optics — ICSO 2000.
The purpose of the PHARAO project is to develop a new atomic clock generation in space. This clock takes advantage of the very low atomic velocities obtained by laser cooling techniques and the microgravity environment. Designing the PHARAO optical b
Autor:
N. Dimarcq, F. Rigaud, J. Valentin, F.-J.. Vermersch, M. Krakowski, J. Berton, Francoise Lozes, Muriel Saccoccio, C. Chappaz, M. de Labachelerie, S. Bonnefont, Philippe Arguel, J. Loesel, D. Holleville
Publikováno v:
Scopus-Elsevier
In this proceeding we present a set of studies which are in progress in different labs and industrials. The aim of this project is to study the possibilities to design a very compact and reliable laser cooling bench for space and inboard applications
Autor:
Michel Abgrall, Claude Coatantiec, Muriel Saccoccio, I. Maksimovic, Jacques Loesel, Pierre Lemonde, Eric Simon, Philippe Laurent
Publikováno v:
Scopus-Elsevier
The PHARAO project purpose is to open the way for a new atomic clock generation in space, where laser cooling techniques and microgravity allow high frequency stability and accuracy. The French space agency, CNES is funding and managing the clock con
Autor:
Nicolas Ponthieu, F. Pajot, J. M. Nicot, M. Chaigneau, G. Parot, Giorgio Savini, Y. André, M. Bouzit, Nicolas Bray, Johan Montel, C. Tucker, J.-P. Dubois, J. Martignac, J. Aumont, Maria Salatino, O. Simonella, V. Buttice, Bruno Maffei, R. J. Laureijs, R. Misawa, J.-Ph. Bernard, Frederi Mirc, B. Mot, J. Narbonne, Silvia Masi, O. Boulade, C. Engel, Etienne Perot, E. Doumayrou, A. Caillat, J. A. Tauber, C. Coudournac, A. Hughes, I. Ristorcelli, Y. Lepennec, S. Maestre, Pierre Tapie, Y. Longval, P. de Bernardis, F. Bousquet, G. Foenard, S. Grabarnik, Giampaolo Pisano, G. Roudil, P. Etcheto, P. Gélot, B. Leriche, Muriel Saccoccio, J. P. Crussaire, J. Pimentao, C. Marty, Matthew Joseph Griffin, Peter A. R. Ade, L. Baustista, M. Charra, F. Douchin, J.-P. Torre, L. Rodriguez, L. Montier, Peter Charles Hargrave, B. Crane, W. Marty, G. Versepuech
Publikováno v:
International Conference on Space Optics — ICSO 2016.
PILOT (Polarized Instrument for Long wavelength Observations of the Tenuous interstellar medium) is a balloonborne astronomy experiment designed to study the polarization of dust emission in the diffuse interstellar medium in our Galaxy. The PILOT in
Autor:
G. Roudil, B. Mot, Y. Longval, W. Marty, J. Aumont, R. Misawa, A. Caillat, Y. Lepennec, E. Doumayrou, G. Foënard, J. A. Tauber, A. Hughes, G. Parot, L. Montier, J. Pimentao, M. Chaigneau, F. Pajot, J.-Ph. Bernard, B. Crane, Johan Montel, B. Leriche, M. Bouzit, Nicolas Bray, V. Buttice, Nicolas Ponthieu, Pierre Tapie, Isabelle Ristorcelli, J. M. Nicot, Muriel Saccoccio, Giorgio Savini, F. Douchin, P. deBernardis, C. Coudournac, Frederi Mirc, J. Martignac, Etienne Perot, Bruno Maffei, J.-P. Torre, C. Engel, A. Mangilli, L. Rodriguez, Peter Charles Hargrave, S. Maestre, Y. André, Silvia Masi, L. Bautista, P. Etcheto, C. Marty, S. Stever, S. Grabarnik, Maria Salatino, O. Simonella, Giampaolo Pisano, J.-P. Dubois, Carole Tucker, P. Gélot, René J. Laureijs, F. Bousquet, Matthew Joseph Griffin, Peter A. R. Ade, J. Narbonne, Christopher Tibbs, O. Boulade
PILOT is a balloon-borne astronomy experiment designed to study the polarization of dust emission in the diffuse interstellar medium in our Galaxy at wavelengths 240 and 550 µm with an angular resolution of about two arc-min. PILOT optics is compose
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b2ea70679b35a30e5c7752086aee7dc
http://hdl.handle.net/11573/1557103
http://hdl.handle.net/11573/1557103