Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-01T14:10:24.877Z Has data issue: false hasContentIssue false
  • English
  • Français

Pupil Replication

Published online by Cambridge University Press:  13 October 2006

M. Carbillet ,
A. Ferrari ,
C. Aime ,
F.H.P. Spaan ,
E. Prot ,
V. Mourai  and
A.H. Greenaway
F.H.P. Spaan
Affiliation:
School of Engineering and Physical Sciences, Heriot-Watt University, Edinburgh, UK
E. Prot
Affiliation:
School of Engineering and Physical Sciences, Heriot-Watt University, Edinburgh, UK
V. Mourai
Affiliation:
School of Engineering and Physical Sciences, Heriot-Watt University, Edinburgh, UK
A.H. Greenaway
Affiliation:
School of Engineering and Physical Sciences, Heriot-Watt University, Edinburgh, UK
Get access

Abstract

Pupil Replication is a technique which could be added to many existing high contrast imaging systems to improve the inner working angle or the contrast when using Pupil Replication. The output pupil of the telescope is replicated and mapped onto the input pupil of the high contrast imaging system. This decreases the size of the image of the star on axis and thereby increases the performance of the high contrast imaging system. In this paper the viability of such a system is assessed through mathematical analysis and simulations.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 22: Astronomy with High Contrast Imaging III: Instrumental Techniques, Modeling and Data Processing , 2006 , pp. 261 - 280
Copyright
© EAS, EDP Sciences, 2006

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)