The NIR arm of SHARK: System for coronagraphy with High-order Adaptive optics from R to K bands

被引:22
|
作者
Farinato, Jacopo [1 ]
Baffa, Carlo [2 ]
Baruffolo, Andrea [1 ]
Bergomi, Maria [1 ]
Carbonaro, Luca [2 ]
Carlotti, Alexis [3 ]
Centrone, Mauro [4 ]
Codona, Johanan [5 ]
Dima, Marco [1 ]
Esposito, Simone [2 ]
Fantinel, Daniela [1 ]
Farisato, Giancarlo [1 ]
Gaessler, Wolfgang [6 ]
Giallongo, Emanuele [4 ]
Greggio, Davide [1 ]
Hinz, Philip [5 ]
Lisi, Franco [2 ]
Magrin, Demetrio [1 ]
Marafatto, Luca [1 ]
Pedichini, Fernando [4 ]
Pinna, Enrico [2 ]
Puglisi, Alfio [2 ]
Ragazzoni, Roberto [1 ]
Salasnich, Bernardo [1 ]
Stangalini, Marco [4 ]
Verinaud, Christophe [3 ]
Viotto, Valentina [1 ]
机构
[1] INAF Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy
[2] INAF Arcetri, I-50125 Florence, Italy
[3] Inst Planetol & Astrophys Grenoble, F-38400 St Martin Dheres, France
[4] INAF Roma, I-00040 Monte Porzio Catone, Italy
[5] Univ Arizona, Steward Observ, Dept Astron, Tucson, AZ USA
[6] Max Planck Inst Astron, D-69117 Heidelberg, Germany
关键词
coronagraphy; extreme adaptive optics; large binocular telescope; planet finding; WAVE-FRONT SENSOR; EXTRASOLAR PLANETS; SUPPRESSION; DISK;
D O I
10.1017/S1473550414000494
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
SHARK is a proposal aimed at investigating the technical feasibility and the scientific capabilities of high-contrast cameras to be implemented at the Large Binocular Telescope (LBT). SHARK foresees two separated channels: near-infrared (NIR) channel and visible, both providing imaging and coronagraphic modes. We describe here the SHARK instrument concept, with particular emphasis on the NIR channel at the level of a conceptual study, performed in the framework of the call for proposals for new LBT instruments. The search for giant extra-Solar planets is the main science case, as we will outline in the paper.
引用
收藏
页码:365 / 373
页数:9
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