摘要
Transition edge sensors (TES) are the chosen detector technology for the SAFARI imaging spectrometer on the SPICA telescope. The TES are required to have an NEP of 2-3 x 10(-19) W/root Hz to take full advantage of the cooled mirror. SRON has developed TiAu TES bolometers for the short wavelength band (30-60 mu m). The TES are on SiN membranes, in which long and narrow legs act as thermal links between the TES and the bath. We present a distributed model that accounts for the heat conductance and the heat capacity in the long legs that provides a guideline for designing low noise detectors. We report our latest results that include a measured dark NEP of 4.2x10(-19) W/root Hz and a saturation power of about 10 fW.
- 出版日期2012-5