Published February 22, 2008
| Version v1
Journal article
Position-Sensitive Detector with GaAs photocathode and high time resolution
Creators
- 1. Special Astropysical Observatory, Nizhnij Arkhyz, 369167 (Russian Federation)
- 2. Institute of Semiconductor Physics, Novosibirsk, 630090 (Russian Federation)
Description
The Position-Sensitive Detector (PSD) on base of GaAs photocathode and microchannel plate set has been developed. PSD consists of thick semi-conductor photocathode with quantum efficiency about 48% in the range of 4000-7500 A, two micro-channel plates, and 16-electrode collector. The detector has spatial resolution of 20-40 microns for about 5·102 pixels, time resolution of 1 μs and effective sensitivity up to 35%
Additional details
Identifiers
- DOI
- 10.1063/1.2896929;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 984
- Journal Issue
- 1
- Journal Page Range
- p. 186-193
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- The Universe at sub-second timescales
- Acronym
- Conference on high time resolution astrophysics
- Dates
- 11-13 Sep 2007
- Place
- Edinburgh, Scotland (United Kingdom)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39072404
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CHARGE-COUPLED DEVICES; GALLIUM ARSENIDES; MICROCHANNEL ELECTRON MULTIPLIERS; PHOTOCATHODES; PLATES; POSITION SENSITIVE DETECTORS; QUANTUM EFFICIENCY; SENSITIVITY; SPATIAL RESOLUTION; TELESCOPE COUNTERS; TIME RESOLUTION
- Descriptors DEC
- ARSENIC COMPOUNDS; ARSENIDES; CATHODES; EFFICIENCY; ELECTRODES; ELECTRON MULTIPLIERS; ELECTRON TUBES; GALLIUM COMPOUNDS; MEASURING INSTRUMENTS; PNICTIDES; RADIATION DETECTORS; RESOLUTION; SEMICONDUCTOR DEVICES; TIMING PROPERTIES
Optional Information
- Notes
- (c) 2008 American Institute of Physics