Browse Abstracts by Speaker > Feng Yan

Wavefront sensing technologies for bioimaging
Yan Feng  1  , Yuewei Liu  2  , Zhengkun Liu  3  , François Hénault  4  , Laura Schreiber  5  , Alain Spang  6  , Antonio Ortiz  7  , Jean-Jacques Correia  8  , Monique Frain  9  , Philippe Gain  10, 11  , Gilles Thuret  10, 11  
1 : Laboratory of Biology, Engineering and Imaging for Ophthalmology (BiiO), Faculty of Medicine, Health Innovation campus, Jean Monnet University, Saint-Etienne, France
Université Jean Monnet - Saint-Etienne
2 : School of Mathematics and Statistics, Lanzhou University, Gansu 730000, China
3 : National Synchrotron Radiation Laboratory, University of Science & Technology of China, Hefei 230029, China
4 : Institut de Planétologie et d'Astrophysique de Grenoble, Université Grenoble-Alpes, CNRS UMR5274, Grenoble 38058, France
CNRS, Institute de Planétologie et d'Astrophysique
5 : INAF - Osservatorio di Astrosica e Scienza dello Spazio di Bologna, Via Gobetti 93/3, Bologna 40129, Italy
6 : Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, France
Centre National de la Recherche Scientifique - CNRS
7 : Nikon Instruments Inc., 1300 Walt Whitman Road, Melville, NY 11747-3064, USA
8 : Institut de Planétologie et d'Astrophysique de Grenoble, Université Grenoble-Alpes, CNRS UMR5274, Grenoble 38058, France
Centre National de la Recherche Scientifique - CNRS
9 : Laboratoire Matière et Systèmes Complexes, Plateforme BioEmergences, Université Paris Cité, CNRS UMR7057, Paris 75205, France
Centre National de la Recherche Scientifique - CNRS
10 : Laboratory of Biology, Engineering and Imaging for Ophthalmology (BiiO), Faculty of Medicine, Health Innovation campus, Jean Monnet University, Saint-Etienne, France
Université Jean Monnet - Saint-Etienne
11 : Ophthalmology department, University Hospital, Saint-Etienne, France
Ophthalmology department, University Hospital, Saint-Etienne, France

Most people associate adaptive optics (AO) with astronomy because of its well-known role in bolstering the imaging power of telescopes and correcting for atmospheric distortion. A wavefront sensor (WFS) is one of the basic components of an AO system, for measuring the shape of the incident wavefront. However, the AO field and thus wavefront sensing technologies have had a growing number of applications in bioimaging, many of which are driven by ophthalmic needs. WFSs can be used to evaluate optical aberrations in the human eye, which is conceptually similar to the astronomy application.

In this talk, I will demonstrate two wavefront sensing technologies. One is the so-called phase crossed-sine WFS [1-2], with a French name of PHASONG (PHase Analyseur de Surface d'Onde de Nouvelle Génération). PHASONG is based on a gradient phase filter (GPF) and a 2´2 lenslet array, provides an elegant and simple solution, high spatial resolution, high sensitivity and a wide dynamic range. Another is a novel 4D imaging technique based on a quadratically distorted (QD) grating, which had been applied for bioimaging much earlier [3-4]. The QD grating, which behaves like a multi-focus "lens" but utilizes principle of diffraction instead of refraction, can be used in simple attachments for commercial microscopes to record widefield images focused simultaneously on multiple (3~9) specimen depths, without sacrificing spatial resolution.



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