millikelvin temperatures

Light with sub-millimeter and far-infrared wavelengths from deep space can travel long distances, penetrating right through dust clouds, and brings us information about the history of the universe and the origin of galaxies, stars and planets. However, the long journey has weakened these signals. So we require sensitive detectors operating at a millikelvin temperatures on a space instrument.

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superconducting detectors

Transition edge sensor (TES) bolometers are superconducting detectors taking advantage of the collapse of the superconducting state and therefore a steep increase in the resistance when its temperature even slightly increases. So, their resistance is extremely sensitive to a change of the temperature, caused by the heating power from light. When heated by incoming photons, the tiny change of the temperature can produce measurable current responses in the detector.

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reading out multiple pixels

Challenges of TES technology used in space missions are not only the sensitivity, but also reading out multiple pixels at the same time. Without this so-called multiplexing—combining the signals from many pixels into a single paired wire—their connecting wires for each pixel would generate too much heat, making it impossible to keep the detectors at the necessary temperature close to absolute zero.

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simultaneous readout 60 TES bolometers

Qian Wang, working closely with Pourya Khosropanah and other members of the SAFARI-FDM team at SRON, led by Gert de Lange, has demonstrated a frequency division multiplexing (FDM) system that can read out 60 TES bolometers simultaneously using only a single paired wire and an amplifier.  The readout noise is lower compared to previous work reported at SRON and by other laboratories, down to a Noise Equipment Power of 0.45 aW/ÖHz. The sensitivities measured in the multiplexing working mode are the same as in a single pixel mode. The researchers expect to read out at least 130 pixels simultaneously if they extend the frequency range used for the current FDM setup. The result demonstrates that the readout technology meets the requirements of the Japanese LiteBIRD space mission and that FDM technology is an option for NASA’s OST mission in the long-term.

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Publication

Q. Wang, P. Khosropanah, J. van der Kuur, G. de Lange, M. D. Audley, A. Aminaei, M. L. Ridder, A. J. van der Linden, M. P. Bruijn, F. van der Tak, and J. R. Gao, Frequency division multiplexing readout of 60 low-noise transition-edge sensor bolometers, Appl. Phys. Lett. 119, 182602 (2021); https://doi.org/10.1063/5.0065570

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