activity
20122026
most citedA prototype of a large tunable Fabry-Perot interferometer for solar spectroscopy

5 citations · 6 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.IM2026

R&D activity in INAF on light instrumentation for continuous optical turbulence monitoring

Camilo Weinberger, Elena Masciadri, Luca Carbonaro +5

Measurements of optical turbulence are essential in both ground-based astronomy and free-space optical communication systems contexts for multiple reasons including supporting and…

astro-ph.IM2026

Progress of the design of the 12-m optical, Wide-field Spectroscopic Telescope (WST)

P. Dierickx, G. Gausachs, C. Cudennec +16

The Wide-Field Spectroscopic Telescope (WST) is a 12-m class, Alt-Az optical telescope providing two simultaneous foci, 2 degrees and 3 by 3 arc minutes respectively, for Multi-Obj…

astro-ph.IM2026

Current status of the High-Resolution Multi-Object Spectrograph (MOS-HR) for the Wide-field Spectroscopic Telescope

Andrea Tozzi, Anna Brucalassi, Matteo Munari +10

The Wide-field Spectroscopic Telescope (WST) is a planned 12-meter class dedicated spectroscopic facility for massive spectroscopic surveys. This paper presents the current status…

astro-ph.IM2026

WST, the Wide-field Spectroscopic Telescope: Telescope structure FE analyses

Simone D'Auria, Vincenzo Cianniello, Ciro Del Vecchio +6

The Altitude Structure of the Wide-field Spectroscopic Telescope (WST) is designed to support and position both primary and secondary mirrors, made of structural steel. Due to its…

astro-ph.IM2026

WST, the Wide-field Spectroscopic Telescope: Mechanical Design and FE Analyses for the High Resolution Spectrograph

Simone D'Auria, Andrea Tozzi, Anna Brucalassi +5

The Wide-field Spectroscopic Telescope (WST) is a planned 12-meter-class dedicated spectroscopic facility designed to address key scientific challenges through large spectroscopic…

astro-ph.IM2023

Lateral constraint for thin glass shell: analysis of the requirements and conceptual design for a segmented active mirror

Marcello Agostino Scalera, Runa Briguglio, Ciro Del Vecchio +2

The latest high-performance telescopes for deep space observation employ very large primary mirrors that are made of smaller segments, like the JWST which employs monolithic beryll…

astro-ph.IM2023★ 1 cited

Contactless actuators and pyramid wavefront sensor, the SPLATT concept for space active optics: an overview of the project and the last laboratory results

Runa Briguglio, Marco Xompero, Marcello Scalera +13

In the last few years the concept of an active space telescope has been greatly developed, to meet demanding requirements with a substantial reduction of tolerances, risks and cost…

astro-ph.IM2021★ 5 cited

A prototype of a large tunable Fabry-Perot interferometer for solar spectroscopy

V. Greco, A. Sordini, G. Cauzzi +7

Large Fabry-Perot Interferometers are used in a variety of astronomical instrumentation, including spectro-polarimeters for 4-meter class solar telescopes. In this work we comprehe…

astro-ph.IM2012

The Actuator Design and the Experimental Tests of a New Technology Large Deformable Mirror for Visible Wavelengths Adaptive Optics

Ciro Del Vecchio, Guido Agapito, Carmelo Arcidiacono +5

Recently, Adaptive Secondary Mirrors showed excellent on-sky results in the Near Infrared wavelengths. They currently provide 30mm inter-actuator spacing and about 1 kHz bandwidth.…