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dc.contributor.authorBoccaletti, Anthony
dc.contributor.authorSchneider, Jean
dc.contributor.authorTraub, Wes
dc.contributor.authorLagage, Pierre-Olivier
dc.contributor.authorStam, Daphne
dc.contributor.authorGratton, Raffaele
dc.contributor.authorTrauger, John
dc.contributor.authorCahoy, Kerri
dc.contributor.authorSnik, Frans
dc.contributor.authorBaudoz, Pierre
dc.contributor.authorGalicher, Raphael
dc.contributor.authorReess, Jean-Michel
dc.contributor.authorMawet, Dimitri
dc.contributor.authorAugereau, Jean-Charles
dc.contributor.authorPatience, Jenny
dc.contributor.authorKuchner, Marc
dc.contributor.authorWyatt, Mark
dc.contributor.authorPantin, Eric
dc.contributor.authorMaire, Anne-Lise
dc.contributor.authorVérinaud, Christophe
dc.date.accessioned2017-07-20T21:05:48Z
dc.date.available2017-07-20T21:05:48Z
dc.date.issued2012-10
dc.identifier.issn0922-6435
dc.identifier.urihttp://hdl.handle.net/1721.1/110795
dc.description.abstractSPICES (Spectro-Polarimetric Imaging and Characterization of Exoplanetary Systems) is a five-year M-class mission proposed to ESA Cosmic Vision. Its purpose is to image and characterize long-period extrasolar planets and circumstellar disks in the visible (450-900 nm) at a spectral resolution of about 40 using both spectroscopy and polarimetry. By 2020/2022, present and near-term instruments will have found several tens of planets that SPICES will be able to observe and study in detail. Equipped with a 1.5 m telescope, SPICES can preferentially access exoplanets located at several AUs (0.5-10 AU) from nearby stars (<25 pc) with masses ranging from a few Jupiter masses to Super Earths (∼2 Earth radii, ∼10 M) as well as circumstellar disks as faint as a few times the zodiacal light in the Solar System.en_US
dc.language.isoen_USen_US
dc.publisherExperimental Astronomyen_US
dc.subjectAstrophysical spectropolarimetryen_US
dc.subjectImaging systemsen_US
dc.subjectPlanetary systemsen_US
dc.subjectTelescopesen_US
dc.subjectNearby starsen_US
dc.subjectAstrophysicsen_US
dc.subjectExoplanetsen_US
dc.subjectHigh contrast imagingen_US
dc.titleSPICES: spectro-polarimetric imaging and characterization of exoplanetary systems.en_US
dc.typeArticleen_US
dc.identifier.citationBoccaletti, A., J. Schneider, W. Traub, P.-O. Lagage, D. Stam, R. Gratton, J. Trauger, K. Cahoy, F. Snik, R. Galicher, J.- M. Reess, D. Mawet, J.-C. Augereau, J. Patience, M. Kuchner, M. Wyatt, E. Pantin, A.-L. Maire, P. Baudoz, C. Verinaud, S. Ronayette, D. Dubreuil, M. Min, M. Rodenbuis, D. Mesa, R. Belikov, O. Guyon, and M. Tamura,“SPICES: Spectro- Polarimetric Imaging and Characterization of Exoplanetary Systems: From planetary disks to nearby Super Earths,” Experimental Astronomy, 34, 2, pp.355-384, doi: 10.1007/s10686-012-9290-5, 2012.en_US
dc.contributor.departmentSpace Telecommunications Astronomy and Radiation (STAR) Lab
dc.contributor.departmentMassachusetts Institute of Technology. Department of Aeronautics and Astronautics


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