activity
20162026
most citedIngot Laser Guide Stars Wavefront Sensing

10 citations · 25 across the 18 of their papers we have counts for

collaborators

19 papers

astro-ph.IM2026

Toward the Italian Astronomical Community's Contribution to HWO: Science, Technology, and Instrument Concepts

A. Fontana, F. Annibali, N. Antonietti +101

This paper summarizes the interest of the Italian astronomical community in the possible participation in the development of the Habitable Worlds Observatory (HWO). It is largely b…

astro-ph.IM2025

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…

astro-ph.EP2024

Deep imaging of three accelerating stars using SHARK-NIR and LMIRCam at LBT

D. Mesa, R. Gratton, V. D'Orazi +29

The combination of detection techniques enhances our ability to identify companions orbiting nearby stars. We employed high-contrast imaging to constrain mass and separation of pos…

astro-ph.IM2024★ 1 cited

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…

astro-ph.IM2023★ 2 cited

TIPTOP: cone effect for single laser adaptive optics systems

Guido Agapito, Cédric Plantet, Fabio Rossi +6

TIPTOP is a python library that is able to quickly compute Point Spread Functions (PSF) of any kind of Adaptive Optics systems. This library has multiple objectives: support the ex…

astro-ph.IM2022★ 2 cited

MAVIS: performance estimation of the adaptive optics module

Guido Agapito, Daniele Vassallo, Cédric Plantet +5

The MCAO Assisted Visible Imager and Spectrograph (MAVIS) is a new visible instrument for ESO Very Large Telescope (VLT). Its Adaptive Optics Module (AOM) must provide extreme adap…

astro-ph.IM2021★ 1 cited

Optical design trade-off study for the AO module of MAVIS

Davide Greggio, Simone Di Filippo, Demetrio Magrin +18

MAVIS (MCAO-Assisted Visible Imager and Spectrograph) is an instrument proposed for the VLT Adaptive Optics Facility (AOF), which is currently in the phase-A conceptual design stud…

astro-ph.IM2020★ 2 cited

MAVIS: system modelling and performance prediction

Guido Agapito, Daniele Vassallo, Cedric Plantet +5

The MCAO Assisted Visible Imager and Spectrograph (MAVIS) Adaptive Optics Module has very demanding goals to support science in the optical: providing 15% SR in V band on a large F…

astro-ph.IM2020

XAO-assisted coronagraphy with SHARK NIR: from simulations to laboratory tests

Gabriele Umbriaco, Elena Carolo, Daniele Vassallo +22

Several Extreme Adaptive Optics (XAO) systems dedicated to the detection and characterisation of the exoplanets are currently in operation for 8-10 meter class telescopes. Coronagr…

astro-ph.IM2018★ 1 cited

Prospects of Deep Field Surveys with Global-MCAO on an ELT

Elisa Portaluri, Valentina Viotto, Roberto Ragazzoni +12

Several astronomical surveys aimed at the investigation of the extragalactic components were carried out in order to map systematically the universe and its constituents. An excell…

astro-ph.EP2018

Data processing on simulated data for SHARK-NIR

E. Carolo, D. Vassallo, J. Farinato +22

A robust post processing technique is mandatory to analyse the coronagraphic high contrast imaging data. Angular Differential Imaging (ADI) and Principal Component Analysis (PCA) a…

astro-ph.IM2018★ 1 cited

A Holographic Diffuser Generalised Optical Differentiation Wavefront Sensor

Luca Marafatto, Roberto Ragazzoni, Daniele Vassallo +12

The wavefront sensors used today at the biggest World's telescopes have either a high dynamic range or a high sensitivity, and they are subject to a linear trade off between these…

astro-ph.IM2018★ 1 cited

A testing facility for AO on-sky demonstrations at the Copernico's Telescope within the ADONI framework

S. Chinellato, R. Ragazzoni, J. Farinato +21

In the context of ADONI - the ADaptive Optics National laboratory of INAF - we are arranging for a facility, accessible to the AO community, in which visiting multi-purpose instrum…

astro-ph.IM2018

A virtual coronagraphic test bench for SHARK-NIR, the second-generation high contrast imager for the Large Binocular Telescope

D. Vassallo, E. Carolo, J. Farinato +21

In this article, we present a simulator conceived for the conceptual study of an AO-fed high-contrast coronagraphic imager. The simulator implements physical optics: a complex dist…

astro-ph.IM2018★ 10 cited

Ingot Laser Guide Stars Wavefront Sensing

Roberto Ragazzoni, Elisa Portaluri, Valentina Viotto +11

We revisit one class of z-invariant WaveFront sensor where the LGS is fired aside of the telescope aperture. In this way there is a spatial dependence on the focal plane with respe…

astro-ph.IM2018

Hierarchichal-segmented AO in order to attain wide field compensation in the visible on an 8m class telescope

Roberto Ragazzoni, Demetrio Magrin, Jacopo Farinato +10

We describe the preliminary optimized layout for a partially optimized concept of an optical-8m class VLT-like 2x2 segmented camera where each channel is assisted by an equivalent…

astro-ph.IM2018★ 3 cited

Multiple spatial frequencies wavefront sensing

Roberto Ragazzoni, Daniele Vassallo, Marco Dima +10

We describe the concept of splitting spatial frequency perturbations into some kind of pupil planes wavefront sensors. Further to the existing approach of dropping higher spatial f…

astro-ph.IM2018

SHARK-NIR, the coronagraphic camera for LBT, moving toward construction

Jacopo Farinato, Francesca Bacciotti, Carlo Baffa +37

SHARK-NIR is one of the two coronagraphic instruments proposed for the Large Binocular Telescope. Together with SHARK-VIS (performing coronagraphic imaging in the visible domain),…

astro-ph.IM2016★ 1 cited

High order dark wavefront sensing simulations

Roberto Ragazzoni, Carmelo Arcidiacono, Jacopo Farinato +8

Dark wavefront sensing takes shape following quantum mechanics concepts in which one is able to "see" an object in one path of a two-arm interferometer using an as low as desired a…