TY - JOUR
T1 - SPICES
T2 - Spectro-polarimetric imaging and characterization of exoplanetary systems: From planetary disks to nearby Super Earths
AU - Boccaletti, Anthony
AU - Schneider, Jean
AU - Traub, Wes
AU - Lagage, Pierre Olivier
AU - Stam, Daphne
AU - Gratton, Raffaele
AU - Trauger, John
AU - Cahoy, Kerri
AU - Snik, Frans
AU - Baudoz, Pierre
AU - Galicher, Raphael
AU - Reess, Jean Michel
AU - Mawet, Dimitri
AU - Augereau, Jean Charles
AU - Patience, Jenny
AU - Kuchner, Marc
AU - Wyatt, Mark
AU - Pantin, Eric
AU - Maire, Anne Lise
AU - Vérinaud, Christophe
AU - Ronayette, Samuel
AU - Dubreuil, Didier
AU - Min, Michiel
AU - Rodenhuis, Michiel
AU - Mesa, Dino
AU - Belikov, Russ
AU - Guyon, Olivier
AU - Tamura, Motohide
AU - Murakami, Naoshi
AU - Beerer, Ingrid Mary
PY - 2012/10
Y1 - 2012/10
N2 - SPICES (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.
AB - SPICES (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.
KW - Exoplanets
KW - High contrast imaging
UR - https://www.scopus.com/pages/publications/84866927948
UR - https://www.scopus.com/pages/publications/84866927948#tab=citedBy
U2 - 10.1007/s10686-012-9290-5
DO - 10.1007/s10686-012-9290-5
M3 - Article
AN - SCOPUS:84866927948
SN - 0922-6435
VL - 34
SP - 355
EP - 384
JO - Experimental Astronomy
JF - Experimental Astronomy
IS - 2
ER -