Pupil Replication

F. H P Spaan; E. Prot; V. Mourai; A. H. Greenaway

doi:10.1051/eas:2006138

Pupil Replication

F. H P Spaan, E. Prot, V. Mourai, A. H. Greenaway

School of Engineering & Physical Sciences

Research output: Contribution to journal › Article › peer-review

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. © EAS, EDP Sciences 2006.

Original language	English
Pages (from-to)	261-280
Number of pages	20
Journal	EAS Publications Series
Volume	22
DOIs	https://doi.org/10.1051/eas:2006138
Publication status	Published - 2006
Event	Astronomy with High Contrast Imaging III: Instrumental Techniques, Modeling and Data Processing - Frejus, France Duration: 16 May 2005 → 19 May 2005

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10.1051/eas:2006138

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year = "2006",

doi = "10.1051/eas:2006138",

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volume = "22",

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journal = "EAS Publications Series",

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AU - Prot, E.

AU - Mourai, V.

AU - Greenaway, A. H.

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AB - 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. © EAS, EDP Sciences 2006.

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DO - 10.1051/eas:2006138

M3 - Article

SN - 1633-4760

VL - 22

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JO - EAS Publications Series

JF - EAS Publications Series

T2 - Astronomy with High Contrast Imaging III: Instrumental Techniques, Modeling and Data Processing

Y2 - 16 May 2005 through 19 May 2005

ER -

Pupil Replication

Abstract

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