activity
20122026
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 · 745 across the 74 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.IM2021★ 4 cited

Advances in control of a Pyramid Single Conjugate Adaptive Optics system

Guido Agapito, Fabio Rossi, Cedric Plantet +2

Adaptive optics systems are an essential technology for the modern astronomy for ground based telescopes. One of the most recent revolution in the field is the introduction of the…

astro-ph.GA2021★ 9 cited

Towards Realistic Modeling of the Astrometric Capabilities of MCAO Systems: Detecting an Intermediate Mass Black Hole with MAVIS

Stephanie Monty, Francois Rigaut, Richard McDermid +9

Accurate astrometry is a key deliverable for the next generation of multi-conjugate adaptive optics (MCAO) systems. The MCAO Visible Imager and Spectrograph (MAVIS) is being design…

astro-ph.HE2021★ 102 cited

The peculiar short-duration GRB 200826A and its supernova

A. Rossi, B. Rothberg, E. Palazzi +31

Gamma-ray bursts (GRBs) are classified as long and short events. Long GRBs (LGRBs) are associated with the end states of very massive stars, while short GRBs (SGRBs) are linked to…

astro-ph.IM2021★ 7 cited

MAORY: A Multi-conjugate Adaptive Optics RelaY for ELT

Paolo Ciliegi, Guido Agapito, Matteo Aliverti +73

MAORY is the adaptive optics module for ELT providing two gravity invariant ports with the same optical quality for two different client instruments. It enable high angular resolut…

astro-ph.IM2021

Bringing SOUL on sky

Enrico Pinna, Fabio Rossi, Alfio Puglisi +20

The SOUL project is upgrading the 4 SCAO systems of LBT, pushing the current guide star limits of about 2 magnitudes fainter thanks to Electron Multiplied CCD detector. This improv…

astro-ph.IM2021

TIPTOP: a new tool to efficiently predict your favorite AO PSF

Benoit Neichel, Olivier Beltramo-Martin, Cedric Plantet +7

The Adaptive Optics (AO) performance significantly depends on the available Natural Guide Stars (NGSs) and a wide range of atmospheric conditions (seeing, Cn2, windspeed,...). In o…