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
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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…