DocumentCode
1139144
Title
A High Resolution, High Frame Rate Detector Based on a Microchannel Plate Readout With the Medipix2 Counting CMOS Pixel Chip
Author
Mikulec, Bettina ; Vallerga, John V. ; McPhate, Jason B. ; Tremsin, Anton S. ; Siegmund, Oswald H W ; Clark, Allan G.
Author_Institution
Univ. of Geneva, Switzerland
Volume
52
Issue
4
fYear
2005
Firstpage
1021
Lastpage
1026
Abstract
The future of ground-based optical astronomy lies with advancements in adaptive optics (AO) to overcome the limitations that the atmosphere places on high resolution imaging. A key technology for AO systems on future very large telescopes are the wavefront sensors (WFS) which detect the optical phase error and send corrections to deformable mirrors. Telescopes with
30 m diameters will require WFS detectors that have large pixel formats (512
512), low noise
and very high frame rates (
1 kHz). These requirements have led to the idea of a bare CMOS active pixel device (the Medipix2 chip) functioning in counting mode as an anode with noiseless readout for a microchannel plate (MCP) detector and at 1 kHz continuous frame rate. First measurement results obtained with this novel detector are presented both for UV photons and beta particles.
30 m diameters will require WFS detectors that have large pixel formats (512
512), low noise
and very high frame rates (
1 kHz). These requirements have led to the idea of a bare CMOS active pixel device (the Medipix2 chip) functioning in counting mode as an anode with noiseless readout for a microchannel plate (MCP) detector and at 1 kHz continuous frame rate. First measurement results obtained with this novel detector are presented both for UV photons and beta particles.Keywords
CMOS integrated circuits; adaptive optics; astronomical telescopes; beta-ray detection; gamma-ray detection; mirrors; nuclear electronics; position sensitive particle detectors; readout electronics; wavefront sensors; Medipix2 counting CMOS pixel chip; UV photons; adaptive optics; anode; beta particles; deformable mirrors; ground-based optical astronomy; high resolution high frame rate detector; high resolution imaging; microchannel plate readout; optical phase error; photon counting; very large telescopes; wavefront sensors; Adaptive optics; Astronomy; Atmosphere; CMOS image sensors; Detectors; High-resolution imaging; Microchannel; Optical noise; Optical sensors; Telescopes; Adaptive optics; CMOS pixel chip; high frame rate; microchannel plate detector; photon counting; wavefront sensor;
fLanguage
English
Journal_Title
Nuclear Science, IEEE Transactions on
Publisher
ieee
ISSN
0018-9499
Type
jour
DOI
10.1109/TNS.2005.852694
Filename
1495799
Link To Document