Hostname: page-component-6bf8c574d5-rwnhh Total loading time: 0 Render date: 2025-02-22T08:48:49.026Z Has data issue: false hasContentIssue false
  • English
  • Français

Potential of MCP Based Photodetecting Systems for High Accuracy Astronomical Object's Observation

Published online by Cambridge University Press:  07 August 2017

I.D. Rodionov ,
M. Yu. Knizhnikov  and
E.B. Solomatin
I.D. Rodionov
Affiliation:
Reagent Research and Development Center 125190, Post Box 192, Moscow, Russia, tel. 7(095) 155 4526 e-mail: [email protected]
M. Yu. Knizhnikov
Affiliation:
Reagent Research and Development Center 125190, Post Box 192, Moscow, Russia, tel. 7(095) 155 4526 e-mail: [email protected]
E.B. Solomatin
Affiliation:
Reagent Research and Development Center 125190, Post Box 192, Moscow, Russia, tel. 7(095) 155 4526 e-mail: [email protected]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

An ideal receiver of radiation should record the arrival time and coordinates of each incoming photon. Available CCD arrays (accumulation mode) and microchannel plate detectors (photon counting mode) are mere approximations to the ideal configuration.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 166: Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry , 1995 , pp. 366
Copyright
Copyright © Kluwer 1995