Review of PSF reconstruction methods and application to post-processing

被引:12
作者
Beltramo-Martin, O. [1 ]
Ragland, S. [2 ]
Fetick, R. [1 ,3 ]
Correia, C. [4 ]
Dupuy, T. [5 ,6 ]
Fiorentino, G. [7 ]
Fusco, T. [1 ,3 ]
Jolissaint, L. [8 ]
Kamann, S. [9 ]
Marasco, A. [10 ]
Massari, D. [11 ,12 ]
Neichel, B. [1 ]
Schreiber, L. [11 ]
Wizinowich, P. [2 ]
机构
[1] Aix Marseille Univ, CNES LAM, CNRS, 38 Rue F Joliot Curie, F-13388 Marseille, France
[2] WM Keck Observ, 65-1120 Mamalahoa Hwy, Kamuela, HI 96743 USA
[3] Paris Saclay Univ, DOTA, ONERA, F-92320 Chatillon, France
[4] Space ODT, Rua Adolfo Casais Monteiro 65, P-4050014 Porto, Portugal
[5] Univ Edinburgh, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
[6] Northern Operat Ctr, Gemini Observ, 670 N Aohoku Pl, Hilo, HI 96720 USA
[7] INAF Osservatorio Astron Roma, Via Frascati 33, I-0040 Monte Porzio Catone, Italy
[8] Univ Appl Sci Western Switzerland, CH-1401 Yverdon, Switzerland
[9] Liverpool John Moores Univ, Astrophys Res Inst, IC2,Liverpool Sci Pk,146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England
[10] INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50127 Florence, Italy
[11] INAF Osservatorio Astrofis & Sci Spazio Bologna, Via Gobetti 93-3, I-40129 Bologna, Italy
[12] Univ Groningen, Kapteyn Astron Inst, NL-9747 AD Groningen, Netherlands
来源
ADAPTIVE OPTICS SYSTEMS VII | 2020年 / 11448卷
基金
欧盟地平线“2020”;
关键词
Adaptive optics; post-processing; STATIC ABERRATIONS; PHASE-DIVERSITY; DECONVOLUTION; DOMAIN; MODEL;
D O I
10.1117/12.2560805
中图分类号
TM [电工技术]; TN [电子技术、通信技术];
学科分类号
0808 ; 0809 ;
摘要
Determining the PSF remains a key challenge for post adaptive-optics (AO) observations regarding the spatial, temporal and spectral variabilities of the AO PSF, as well as itx complex structure. This paper aims to provide a non-exhaustive but classified list of techniques and references that address this issue of PSF determination, with a particular scope on PSF reconstruction, or more generally pupil-plane-based approaches. We have compiled a large amount of references to synthesize the main messages and kept them at a top level. We also present applications of PSF reconstruction/models to post-processing, more especially PSF-fitting and deconvolution for which there is a fast progress in the community.
引用
收藏
页数:15
相关论文
共 68 条
[1]   PASSATA - Object oriented numerical simulation software for adaptive optics [J].
Agapito, G. ;
Puglisi, A. ;
Esposito, S. .
ADAPTIVE OPTICS SYSTEMS V, 2016, 9909
[2]   Image-based wavefront sensing for astronomy using neural networks [J].
Andersen, Torben ;
Owner-Petersen, Mette ;
Enmark, Anita .
JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS, 2020, 6 (03)
[3]   Estimation of atmospheric turbulence parameters from Shack-Hartmann wavefront sensor measurements [J].
Andrade, Paulo P. ;
Garcia, Paulo J. V. ;
Correia, Carlos M. ;
Kolb, Johann ;
Carvalho, Maria Ines .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2019, 483 (01) :1192-1201
[4]  
[Anonymous], 2010, ADAPTATIVE OPTICS EX
[5]   The MUSE second-generation VLT instrument [J].
Bacon, R. ;
Accardo, M. ;
Adjali, L. ;
Anwand, H. ;
Bauer, S. ;
Biswas, I. ;
Blaizot, J. ;
Boudon, D. ;
Brau-Nogue, S. ;
Brinchmann, J. ;
Caillier, P. ;
Capoani, L. ;
Carollo, C. M. ;
Contini, T. ;
Couderc, P. ;
Daguise, E. ;
Deiries, S. ;
Delabre, B. ;
Dreizler, S. ;
Dubois, J. ;
Dupieux, M. ;
Dupuy, C. ;
Emsellem, E. ;
Fechner, T. ;
Fleischmann, A. ;
Francois, M. ;
Gallou, G. ;
Gharsa, T. ;
Glindemann, A. ;
Gojak, D. ;
Guiderdoni, B. ;
Hansali, G. ;
Hahn, T. ;
Jarno, A. ;
Kelz, A. ;
Koehler, C. ;
Kosmalski, J. ;
Laurent, F. ;
Le Floch, M. ;
Lilly, S. J. ;
Lizon, J. -L ;
Loupias, M. ;
Manescau, A. ;
Monstein, C. ;
Nicklas, H. ;
Olaya, J-C ;
Pares, L. ;
Pasquini, L. ;
Pecontal-Rousset, A. ;
Pello, R. .
GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY III, 2010, 7735
[6]   The Durham Adaptive Optics Simulation Platform (DASP): Current status [J].
Basden, A. G. ;
Bharmal, N. A. ;
Jenkins, D. ;
Morris, T. J. ;
Osborn, J. ;
Peng, J. ;
Staykov, L. .
SOFTWAREX, 2018, 7 :63-69
[7]   PRIME: PSF Reconstruction and Identification for Multiple-source characterization Enhancement - application to Keck NIRC2 imager [J].
Beltramo-Martin, O. ;
Correia, C. M. ;
Ragland, S. ;
Jolissaint, L. ;
Neichel, B. ;
Fusco, T. ;
Wizinowich, P. L. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2019, 487 (04) :5450-5462
[8]  
Beltramo-Martin O., 2020, ARXIV
[9]   Optimal correction of distortion for high-angular-resolution images: Application to GeMS data [J].
Bernard, A. ;
Neichel, B. ;
Mugnier, L. M. ;
Fusco, T. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 473 (02) :2590-2607
[10]   SExtractor: Software for source extraction [J].
Bertin, E ;
Arnouts, S .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1996, 117 (02) :393-404