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INAF - Osservatorio di
Arcetri
Largo E. Fermi 5 50125 Firenze ITALY |
|
Office +39-055-2752-207
Lab +39-055-2752-201/210 |
Research activitiesSince 2004 I'm involved in the development of high order Adaptive Optics systems for ground based telescopes.I'm specialized in AO system calibration and in pyramid wavefront sensor development and integration. The main projects I'm currently involved are: - SOUL: Single conjugated adaptive Optics Upgrade for the Large Binocular Telescope - SHARK: System for coronagraphy with High order Adaptive optics from R to K band (Large Binocular Telesope) - NGWS: the Natural Guidestar Wavefront Sensor for the Giant Magellan Telecope - The Pyramid Wavefront Sensor for ERIS (collaboration with ESO) - FLAO: First Light Adaptive Optics of the Large Binocular Telescope (press relase) - AO system for the LBTI (collaboration with the Arizona University - USA) - Magellan Adaptive Optics system (collaboration with the Steward Observatory - USA) The main past projects: - High Order Testbench (Opticon - JRA1 collaboration with ESO) - the Active Phasing Experiment (WP4600 ELT Design Study - FP6) |
FLAO system at the Large Binocular
Telescope |
Rodigas et al.; On the Morphology and Chemical Composition of the HR 4796A Debris Disk. ; arXiv , arXiv:1410.7753.(2014) 2014arXiv1410.7753R
Arcidiacono et al.; A high-resolution image of the inner shell of the P Cygni nebula in the infrared [Fe II] line. ; MNRAS , 443, 1142-1150.(2014) 2014MNRAS.443.1142A
Guerra et al.; Usage of Large Binocular Telescope pupils to estimate the local outer scale of turbulence. ; SPIE , 9148, 914869.(2014) 2014SPIE.9148E..69G
Pinna et al.; Design and numerical simulations of the GMT Natural Guide star WFS. ; SPIE , 9148, 91482M.(2014) 2014SPIE.9148E..2MP
Close et al.; Into the blue: AO science with MagAO in the visible. ; SPIE , 9148, 91481M.(2014) 2014SPIE.9148E..1MC
Stangalini et al.; The solar system at 10 parsec: exploiting the ExAO of LBT in the visual wavelengths. ; SPIE , 9147, 91478F.(2014) 2014SPIE.9147E..8FS
Farinato et al.; SHARK (System for coronagraphy with High order Adaptive optics from R to K band): a proposal for the LBT 2nd generation instrumentation. ; SPIE , 9147, 91477J.(2014) 2014SPIE.9147E..7JF
Antichi et al.; Meaningful options for a dichroic unit within the natural & laser guide star AO systems at the Giant Magellan Telescope. ; SPIE , 9148, 91484X.(2014) 2014SPIE.9148E..4XA
Riccardi et al.; The NGS Pyramid wavefront sensor for ERIS. ; SPIE , 9148, 91483D.(2014) 2014SPIE.9148E..3DR
Males et al.; Direct imaging of exoplanets in the habitable zone with adaptive optics. ; SPIE , 9148, 914820.(2014) 2014SPIE.9148E..20M
Bouchez et al.; The Giant Magellan Telescope adaptive optics program. ; SPIE , 9148, 91480W.(2014) 2014SPIE.9148E..0WB
Morzinski et al.; MagAO: Status and on-sky performance of the Magellan adaptive optics system. ; SPIE , 9148, 914804.(2014) 2014SPIE.9148E..04M
Kuntschner et al.; ERIS: preliminary design phase overview. ; SPIE , 9147, 91471U.(2014) 2014SPIE.9147E..1UK
Males et al.; Magellan Adaptive Optics First-light Observations of the Exoplanet β Pic B. I. Direct Imaging in the Far-red Optical with MagAO+VisAO and in the Near-ir with NICI. ; ApJ , 786, 32.(2014) 2014ApJ...786...32M
Farinato et al.; The NIR arm of SHARK (System for coronagraphy with High order Adaptive optics from R to K band). ; ebi..conf , P4P.(2014) 2014ebi..confP4.74F
Morzinski et al.; The atmosphere of Beta Pictoris b via 0.9-5um imaging with Magellan Adaptive Optics. ; ebi..conf , P4P.(2014) 2014ebi..confP4.71M
Morzinski et al.; Direct imaging of Beta Pictoris b with first-light Magellan Adaptive Optics. ; IAUS , 299, 252-256.(2014) 2014IAUS..299..252M
Follette et al.; Visible Light Adaptive Optics Imaging of the Orion 218-354 Silhouette Disk. ; IAUS , 299, 159-160.(2014) 2014IAUS..299..159F
Males et al.; High Contrast Imaging of an Exoplanet with the Magellan VisAO Camera. ; IAUS , 299, 46-47.(2014) 2014IAUS..299...46M
Bailey et al.; The Large Binocular Telescope Interferometer & Adaptive Optics System: On-sky Performance and Results. ; IAUS , 299, 26-27.(2014) 2014IAUS..299...26B