Charge-coupled devices for the ESA Euclid M-class Mission

J. Endicott; S. Darby; S. Bowring; D. Burt; T. Eaton; A. Grey; I. Swindells; R. Wheeler; L. Duvet; M. Cropper; D. Walton; A. Holland; N. Murray; J. Gow

doi:10.1117/12.926323

25 September 2012 Charge-coupled devices for the ESA Euclid M-class Mission

J. Endicott, S. Darby, S. Bowring, D. Burt, T. Eaton, A. Grey, I. Swindells, R. Wheeler, L. Duvet, M. Cropper, D. Walton, A. Holland, N. Murray, J. Gow

Author Affiliations +

Proceedings Volume 8453, High Energy, Optical, and Infrared Detectors for Astronomy V; 845304 (2012) https://doi.org/10.1117/12.926323
Event: SPIE Astronomical Telescopes + Instrumentation, 2012, Amsterdam, Netherlands

Abstract

The European Space Agency has funded e2v’s development of an image sensor for the visible instrument in the Euclid space telescope. Euclid has been selected for a medium class mission launch opportunity in 2020. The project aims to map the dark universe with two complementary methods; a galaxy red-shift survey and weak gravitational lensing using near infrared and visible instruments. The baseline for the visible instrument was to be the CCD203-82, which has been successfully flown on NASA’s Solar Dynamics Observatory. However, to optimise the device for Euclid, e2v have designed and manufactured the CCD273-84. This device has a higher-responsivity lower-noise amplifier, enhanced red response, parallel charge injection structures and narrower registers which improve low signal charge transfer efficiency. Development models for Euclid have been manufactured with a thinner gate dielectric than standard for improved tolerance to ionising radiation. This paper describes the imager sensor in detail and focuses on the novel aspects of the device, package and interface.

Citation Download Citation

J. Endicott, S. Darby, S. Bowring, D. Burt, T. Eaton, A. Grey, I. Swindells, R. Wheeler, L. Duvet, M. Cropper, D. Walton, A. Holland, N. Murray, and J. Gow "Charge-coupled devices for the ESA Euclid M-class Mission", Proc. SPIE 8453, High Energy, Optical, and Infrared Detectors for Astronomy V, 845304 (25 September 2012); https://doi.org/10.1117/12.926323

ACCESS THE FULL ARTICLE

INSTITUTIONAL
Select your institution to access the SPIE Digital Library.

SELECT YOUR INSTITUTION

PERSONAL
Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.

PERSONAL SIGN IN

No SPIE Account? Create one

PURCHASE THIS CONTENT

SUBSCRIBE TO DIGITAL LIBRARY

50 downloads per 1-year subscription

Members: $195

Non-members: $335 ADD TO CART

25 downloads per 1 - year subscription

Members: $145

Non-members: $250 ADD TO CART

PURCHASE SINGLE ARTICLE

Includes PDF, HTML & Video, when available