Abstract
Ultra-low-noise transition edge sensors (TES) with noise equivalent power lower than 2 × 10- 19 W/Hz1 / 2 have been fabricated by SRON, which meet the sensitivity requirements for the far-infrared SAFARI instrument on space infrared telescope for cosmology and astrophysics. Our TES detector is based on a titanium/gold (Ti/Au) thermistor on a silicon nitride (SiN) island. The island is thermally linked with SiN legs to a silicon support structure at the bath temperature. The SiN legs are very thin (250 nm), narrow (500 nm), and long (above 300 μ m); these dimensions are needed in leg-isolated bolometers to achieve the required level of sensitivity. In this paper, we describe the latest fabrication process for our TES bolometers with improved sensitivity.
| Original language | English |
|---|---|
| Pages (from-to) | 60-65 |
| Number of pages | 6 |
| Journal | Journal of Low Temperature Physics |
| Volume | 184 |
| Issue number | 1-2 |
| DOIs | |
| Publication status | Published - 1 Jul 2016 |
Keywords
- Bolometer
- SiN membrane
- Transition edge sensors
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