| 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 |
| Rok vydání: |
2017 |
| Předmět: |
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| Zdroj: |
International Conference on Space Optics — ICSO 2016. |
| Popis: |
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 instrument allows observations at wavelengths 240 μm (1.2THz) with an angular resolution about two arc-minutes. The observations performed during the first flight in September 2015 at Timmins, Ontario Canada, have demonstrated the optical performances of the instrument. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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