The strong background in cryogenics is inherited from previous work on super-conducting detectors, and similar technology will be used in the ATHENA mission.
Further details on previous activities can be found by following the links below.
|[Rosetta] MIDAS - Micro Imaging Dust Analysis System||[Rosetta] MIP||[Rosetta] OSIRIS|
|[STEREO] Solar Electron Proton Telescope (SEPT)||SOHO-VIRGO-LOI|
|Instrument Technology R&D|
|S-CAM 2||S-CAM 3||S-CAM 4||Active Pixel Sensor|
|STJ detectors||Optical DROIDS||X-ray DROIDS|