Ultra-wide-field retinal images in an eye with a small-aperture corneal inlay

2015 ◽  
Vol 41 (1) ◽  
pp. 234-236 ◽  
Author(s):  
Reiji Yokota ◽  
Takashi Koto ◽  
Makoto Inoue ◽  
Akito Hirakata
2013 ◽  
Vol 92 (2) ◽  
pp. e168-e169 ◽  
Author(s):  
Makoto Inoue ◽  
Hiroko Bissen-Miyajima ◽  
Hiroyuki Arai ◽  
Akito Hirakata

2019 ◽  
Vol 45 (3) ◽  
pp. 367-371 ◽  
Author(s):  
Norman Romito ◽  
Elena Basli ◽  
Isabelle Goemaere ◽  
Vincent Borderie ◽  
Laurent Laroche ◽  
...  
Keyword(s):  

2011 ◽  
Vol 27 (12) ◽  
pp. 876-880 ◽  
Author(s):  
Alois K. Dexl ◽  
Josef Ruckhofer ◽  
Wolfgang Riha ◽  
Melchior Hohensinn ◽  
Theresa Rueckl ◽  
...  

2016 ◽  
Vol 32 (6) ◽  
pp. 379-384 ◽  
Author(s):  
Estera Igras ◽  
Rónán O'Caoimh ◽  
Paul O'Brien ◽  
William Power

SciVee ◽  
2012 ◽  
Author(s):  
Francisco Sanchez Leon ◽  
Abhiram S. Vilupuru ◽  
George O. Waring, IV ◽  
Eric T. Brooker

2020 ◽  
Vol 497 (3) ◽  
pp. 4000-4008
Author(s):  
Rongyu Sun ◽  
Shengxian Yu ◽  
Peng Jia ◽  
Changyin Zhao

ABSTRACT Telescopes with a small aperture and a wide field of view are widely used and play a significant role in large-scale state-of-the-art sky survey applications, such as transient detection and near-Earth object observations. However, owing to the specific defects caused by optical aberrations, the image quality and efficiency of source detection are affected. To achieve high-accuracy position measurements, an innovative technique is proposed. First, a large number of raw images are analysed using principal component analysis. Then, the effective point spread function is reconstructed, which reflects the state of the telescope and reveals the characteristics of the imaging process. Finally, based on the point spread function model, the centroids of star images are estimated iteratively. To test the efficiency and reliability of our algorithm, a large number of simulated images are produced, and a telescope with small aperture and wide field of view is utilized to acquire the raw images. The position measurement of sources is performed using our novel method and two other common methods on these data. Based on a comparison of the results, the improvement is investigated, and it is demonstrated that our proposed technique outperforms the others on position accuracy. We explore the limitations and potential gains that may be achieved by applying this technique to custom systems designed specifically for wide-field astronomical applications.


Author(s):  
Anastasia Levenkova ◽  
Michael Kalloniatis ◽  
Angelica Ly ◽  
Arthur Ho ◽  
Arcot Sowmya

Sign in / Sign up

Export Citation Format

Share Document