Flight photon counting electron multiplying charge coupled device development for the Roman Space Telescope coronagraph instrument-Reference-Cited by-同舟云学术

Flight photon counting electron multiplying charge coupled device development for the Roman Space Telescope coronagraph instrument

Published:2023-03-19 Issue:01 Volume:9 Page:
ISSN:2329-4124
Container-title:Journal of Astronomical Telescopes, Instruments, and Systems
language:
Short-container-title:J. Astron. Telesc. Instrum. Syst.

Author:

Morrissey Patrick¹,Harding Leon²,Bush Nathan¹,Bottom Michael³,Nemati Bijan⁴,Daniel Andrew¹,Jun Bongim⁵,Martinez Luz Maria Sierra¹,Desai Niyati⁶,Barry Dave⁷,Davis Rhonda-Topaz⁷,Demers Richard⁸,Hall David⁹,Holland Andrew⁹,Turner Pete⁷,Shortt Brian¹⁰

Affiliation:

1. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, United States

2. Virginia Tech National Security Institute, Arlington, Virginia, United States

3. University of Hawaii at Manoa, Institute for Astronomy, Hilo, Hawaii, United States

4. Tellus1 Scientific, LLC, Madison, Alabama, United States

5. Northrup Grumman Mission Systems, Woodland Hills, California, United States

6. California Institute of Technology, Pasadena, California, United States

7. Teledyne-e2v, Chelmsford, United Kingdom

8. GMTO Corporation, Pasadena, California, United States

9. Open University, Centre for Electronic Imaging, Milton Keynes, United Kingdom

10. European Space Research and Technology Center, Noordwijk, The Netherlands

Publisher

SPIE-Intl Soc Optical Eng

Subject

Space and Planetary Science,Mechanical Engineering,Astronomy and Astrophysics,Instrumentation,Control and Systems Engineering,Electronic, Optical and Magnetic Materials

Reference31 articles.

1. The Roman Space Telescope coronagraph technology demonstration: current status and relevance to future missions

2. Technology advancement of the CCD201-20 EMCCD for the WFIRST coronagraph instrument: sensor characterization and radiation damage

3. The LLCCD: low-light imaging without the need for an intensifier

4. Subelectron read noise at MHz pixel rates

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