6 August 2014 SHARK (System for coronagraphy with High order Adaptive optics from R to K band): a proposal for the LBT 2nd generation instrumentation
Author Affiliations +
Abstract
This article presents a proposal aimed at investigating the technical feasibility and the scientific capabilities of high contrast cameras to be implemented at LBT. Such an instrument will fully exploit the unique LBT capabilities in Adaptive Optics (AO) as demonstrated by the First Light Adaptive Optics (FLAO) system, which is obtaining excellent results in terms of performance and reliability. The aim of this proposal is to show the scientific interest of such a project, together with a conceptual opto-mechanical study which shows its technical feasibility, taking advantage of the already existing AO systems, which are delivering the highest Strehl experienced in nowadays existing telescopes. Two channels are foreseen for SHARK, a near infrared channel (2.5-0.9 um) and a visible one (0.9 – 0.6 um), both providing imaging and coronagraphic modes. The visible channel is equipped with a very fast and low noise detector running at 1.0 kfps and an IFU spectroscopic port to provide low and medium resolution spectra of 1.5 x 1.5 arcsec fields. The search of extra solar giant planets is the main science case and the driver for the technical choices of SHARK, but leaving room for several other interesting scientific topics, which will be briefly depicted here.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jacopo Farinato, Jacopo Farinato, Fernando Pedichini, Fernando Pedichini, Enrico Pinna, Enrico Pinna, Francesca Baciotti, Francesca Baciotti, Carlo Baffa, Carlo Baffa, Andrea Baruffolo, Andrea Baruffolo, Maria Bergomi, Maria Bergomi, Pietro Bruno, Pietro Bruno, Enrico Cappellaro, Enrico Cappellaro, Luca Carbonaro, Luca Carbonaro, Alexis Carlotti, Alexis Carlotti, Mauro Centrone, Mauro Centrone, Laird Close, Laird Close, Johanan Codona, Johanan Codona, Silvano Desidera, Silvano Desidera, Marco Dima, Marco Dima, Simone Esposito, Simone Esposito, Daniela Fantinel, Daniela Fantinel, Giancarlo Farisato, Giancarlo Farisato, Adriano Fontana, Adriano Fontana, Wolfgang Gaessler, Wolfgang Gaessler, Emanuele Giallongo, Emanuele Giallongo, Raffaele Gratton, Raffaele Gratton, Davide Greggio, Davide Greggio, Juan Carlos Guerra, Juan Carlos Guerra, Olivier Guyon, Olivier Guyon, Philip Hinz, Philip Hinz, Francesco Leone, Francesco Leone, Franco Lisi, Franco Lisi, Demetrio Magrin, Demetrio Magrin, Luca Marafatto, Luca Marafatto, Matteo Munari, Matteo Munari, Isabella Pagano, Isabella Pagano, Alfio Puglisi, Alfio Puglisi, Roberto Ragazzoni, Roberto Ragazzoni, Bernardo Salasnich, Bernardo Salasnich, Eleonora Sani, Eleonora Sani, Salvo Scuderi, Salvo Scuderi, Marco Stangalini, Marco Stangalini, Vincenzo Testa, Vincenzo Testa, Christophe Verinaud, Christophe Verinaud, Valentina Viotto, Valentina Viotto, } "SHARK (System for coronagraphy with High order Adaptive optics from R to K band): a proposal for the LBT 2nd generation instrumentation", Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 91477J (6 August 2014); doi: 10.1117/12.2056598; https://doi.org/10.1117/12.2056598
PROCEEDINGS
10 PAGES


SHARE
RELATED CONTENT


Back to Top