Paper
1 July 1990 DQE enhancement of MCP intensifiers for astronomy results of the MIC II program
Robert J. Airey, Timothy J. Norton, Brian L. Morgan, John L. A. Fordham, David A. Bone, J. Ralph Powell
Author Affiliations +
Abstract
The microchannel plate intensified CCD (MIC) photon counting detector system was developed to replace a common user photon counting detector, the image photon counting system (IPCS), at the Anglo Australian Telescope and at the William Herschel Telescope and the Isaac Newton Telescope at La Palma Observatory. The IPCS incorporated magnetically-focused four-stage cascade image intensifiers. This paper discusses technological aspects of the design and optimization of very high gain microchannel plate image intensifiers for such photon counting systems and particularly the optimization of device detective quantum efficiency.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Robert J. Airey, Timothy J. Norton, Brian L. Morgan, John L. A. Fordham, David A. Bone, and J. Ralph Powell "DQE enhancement of MCP intensifiers for astronomy results of the MIC II program", Proc. SPIE 1235, Instrumentation in Astronomy VII, (1 July 1990); https://doi.org/10.1117/12.19098
Lens.org Logo
CITATIONS
Cited by 4 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Microchannel plates

Ions

Photon counting

Image intensifiers

Astronomy

Charge-coupled devices

Sensors

Back to Top