Title: Infrared Detection Technology
1Infrared Detection Technology Breakout Summary
Phillip Mauskopf - University of Cardiff Derek
Ives - Royal Observatory, Edinburgh Harvey Rutt -
Southampton University Larry Carr - NSLS
Brookhaven Laboratory Peter Gardner- The
University of Manchester Mike Towrie - CCLRC
Rutherford Appleton Lab Alessio Bocci - INFN-LNF
Frascati Zhi-Jun Xin - CCLRC Daresbury
Laboratory Mark Tobin - CCLRC Daresbury Laboratory
2Questions Limitations of what is available
now? Dominated by MCT - few manufacturers Photov
oltaic only to 12 um - but in big arrays PC -
good to 20 um but would be very for large
format - if possible
3Questions What could be available now? Blocked
Impurity Band - 2-100 um (but 4K, maybe slow
too) Custom MCT cheap off the shelf RT
microbolometers/pyroelectric
4Questions What is not currently addressed? High
speed array readout capability Very high
response time (ps) (including for FEL
diagnostics) Near Background Limited performance
across wider range
5- Questions
- What might be available in in the longer term?
- New readout integrated circuits - new approaches.
Do not currentlymatch our requirements. - Superconducting detectors - interesting but lots
of questions - Superconducting SPC beyond 3um
- Array construction (1D and 2D)
- Is 3 ps response really achievable
- Dynamic range?
6- Questions
- Who is based placed to develop these?
- Custom large MCT - restricted largely to military
suppliers or Qinetiq - Custom PC MCT - few other suppliers - expensive
hand made - Superconducting - requires international
industrial-academic collaborations - CCLRC capabilities for readout
7- Questions
- What new systems would have most impact?
- Longer wavelength response big arrays (beyond 12
um) - Faster readout big arrays (maybe 10x faster to
start)
- Questions
- Who might fund this?
- EU? Facility Development? INTAS? Collaboration
with instrument manufacturers? Joint projects
with other synchrotron sources? - But could be serious money...
8But... Should determine more clearly what are
the science drivers in this area. This will
determine pixel sizes, speeds, response times
wavelength range...