activity
20122020
most citedA convergent blind deconvolution method for post-adaptive-optics astronomical imaging

43 citations · 110 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM2020★ 2 cited

Technical and software upgrades completed and planned at OARPAF

D. Ricci, L. Cabona, A. La Camera +3

We present technical, instrumental, and software upgrades completed and planned at astronomical observatory called "Osservatorio Astronomico Regionale Parco Antola, Fascia" (OARPAF…

astro-ph.EP2017★ 10 cited

Multi-filter transit observations of HAT-P-3b and TrES-3b with multiple Northern Hemisphere telescopes

Davide Ricci, Pedro Valdés Sada, Samuel Navarro-Meza +17

We present a photometric follow-up of transiting exoplanets HAT-P-3b and TrES-3b, observed by using several optical and near-infrared filters, with four small-class telescopes (D =…

astro-ph.SR2016★ 24 cited

Sub-0.1" optical imaging of the Z CMa jets with SPHERE/ZIMPOL

S. Antoniucci, L. Podio, B. Nisini +15

Crucial information on the mass accretion-ejection in young stars can be obtained from high spatial resolution images of jets in sources with recurrent accretion outbursts. Using t…

math.NA2015★ 13 cited

A blind deconvolution method for ground based telescopes and Fizeau interferometers

M. Prato, A. La Camera, S. Bonettini +3

In the case of ground-based telescopes equipped with adaptive optics systems, the point spread function (PSF) is only poorly known or completely unknown. Moreover, an accurate mode…

astro-ph.SR2014★ 11 cited

The HH34 outflow as seen in [FeII]1.64um by LBT-LUCI

S. Antoniucci, A. La Camera, B. Nisini +4

Dense atomic jets from young stars copiously emit in [FeII] IR lines, which can, therefore, be used to trace the immediate environments of embedded protostars. We want to investiga…

astro-ph.IM2013★ 43 cited

A convergent blind deconvolution method for post-adaptive-optics astronomical imaging

M. Prato, A. La Camera, S. Bonettini +1

In this paper we propose a blind deconvolution method which applies to data perturbed by Poisson noise. The objective function is a generalized Kullback-Leibler divergence, dependi…

astro-ph.IM2012★ 7 cited

Image reconstruction for observations with a high dynamic range: LINC-NIRVANA simulations of a stellar jet

Andrea La Camera, Simone Antoniucci, Mario Bertero +3

We report the results of a simulation and reconstruction of observations of a young stellar object (YSO) jet with the LINC-NIRVANA (LN) interferometric instrument, which will be mo…