activity
20102024
most citedFirst Light LBT AO Images of HR 8799 bcde at 1.65 and 3.3 Microns: New Discrepancies between Young Planets and Old Brown Dwarfs

153 citations · 1.4k across the 58 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.IM2020

EMCCD for Pyramid wavefront sensor: laboratory characterization

Guido Agapito, Tommaso Mazzoni, Fabio Rossi +3

Electro-Multiplying CCDs offer a unique combination of speed, sub-electron noise and quantum efficiency. These features make them extremely attractive for astronomical adaptive opt…

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★ 1 cited

Operational forecast of the PSF figures of merit

A. Turchi, G. Agapito, E. Masciadri +6

The optimization and scheduling of scientific observations done with instrumentation supported by adaptive optics could greatly benefit from the forecast of PSF figures of merit (F…

astro-ph.IM2020★ 1 cited

MICADO PSF-Reconstruction work package description

Matteo Simioni, Carmelo Arcidiacono, Andrea Grazian +25

The point spread function reconstruction (PSF-R) capability is a deliverable of the MICADO@ESO-ELT project. The PSF-R team works on the implementation of the instrument software de…

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.SR2020★ 124 cited

The HOSTS survey for exozodiacal dust: Observational results from the complete survey

Steve Ertel, Denis Defrère, Philip M. Hinz +43

The Large Binocular Telescope Interferometer (LBTI) enables nulling interferometric observations across the N band (8 to 13 um) to suppress a star's bright light and probe for fain…