292 citations · 473 across the 22 of their papers we have counts for
11 papers · 1 filter
SHINS, the SHARK-NIR Instrument Control Software
Davide Ricci, Fulvio Laudisio, Alessandro Lorenzetto +20
SHARK-NIR is a new compact instrument for coronagraphic imaging, direct imaging, and coronagraphic spectroscopy in the near-infrared wavelengths mounted at LBT. Taking advantage of…
New developments on the Ingot WFS laboratory testing
Tânia Gomes Machado, Simone Di Filippo, Kalyan K. R. Santhakumari +16
The Ingot WFS was designed to overcome some of the challenges present in classical wavefront sensors when they deal with sodium LGSs. This innovative sensor works by sensing the fu…
Pupil plane WFSs for LGS systems of giant telescopes: the case of Ingot
Elisa Portaluri, Roberto Ragazzoni, Davide Greggio +9
The Ingot WFS belongs to a class of pupil-plane WFSs designed to address the challenges posed by Sodium Laser Guide Stars, and consists of a combination of refractive and reflectiv…
The PLATO Mission
Heike Rauer, Conny Aerts, Juan Cabrera +842
PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…
An Ingot-like class of WaveFront Sensors for Laser Guide Stars
Roberto Ragazzoni, Elisa Portaluri, Davide Greggio +15
Full sky coverage Adaptive Optics on Extremely Large Telescopes requires the adoption of several Laser Guide Stars as references.With such large apertures, the apparent elongation…
MORFEO enters final design phase
Lorenzo Busoni, Guido Agapito, Alessandro Ballone +81
MORFEO (Multi-conjugate adaptive Optics Relay For ELT Observations, formerly MAORY), the MCAO system for the ELT, will provide diffraction-limited optical quality to the large fiel…
The Ingot WFS ON an ELT-like telescope: the project and simulations
Elisa Portaluri, Simone Di Filippo, Valentina Viotto +12
The Ingot WFS represents an innovative and indispensable class of sensors conceived to overcome some limitations due to the LGSs geometry, which is significantly different from the…
Laboratory testing of the Ingot WFS
Simone Di Filippo, Davide Greggio, Maria Bergomi +9
The ingot WFS is a new kind of wavefront sensor specifically designed to deal with the elongation of LGS reference sources on ELT-class telescopes. Like the pyramid, it belongs to…
The CHEOPS mission
Willy Benz, Christopher Broeg, Andrea Fortier +107
The CHaracterising ExOPlanet Satellite (CHEOPS) was selected in 2012, as the first small mission in the ESA Science Programme and successfully launched in December 2019. CHEOPS is…
Simulations of ELT-GMCAO performance for deep field observations
Elisa Portaluri, Valentina Viotto, Roberto Ragazzoni +6
The Global-Multi Conjugated Adaptive Optics (GMCAO) approach offers an alternative way to correct an adequate scientific Field of View (FoV) using only natural guide stars (NGSs) t…
To PLAnetary Transit Or NOT? An extremely large field of view camera with a CaF2 component tested in thermo-vacuum
M. Bergomi, D. Magrin, J. Farinato +13
Because of its nicely chromatic behavior, Calcium Fluoride (CaF2) is a nice choice for an optical designer as it can easily solve a number of issues, giving the right extra degree…