Development and Characterization of KID-Based SPIAKID Instrument
Journal article, 2026

The SpectroPhotometric Imaging in Astronomy with Kinetic Inductance Detectors (SPIAKID) instrument is designed and currently being developed to explore ultra-faint dwarf (UFD) galaxies in the optical and near-infrared bands. We envisage to install SPIAKID at the New Technology Telescope (NTT) in Chile as a guest instrument and targets a field of view of 2' × 2', which can be achieved using four 20,000-pixel arrays at the focal plane. Each array is divided into 10 subarrays, with 2,000 pixels per feedline. The superconducting kinetic inductance detector (KID) comprises a TiN/Ti/TiN trilayer meander and an Nb interdigitated capacitor. In a newly developed anti-vibration dilution cryostat, 10 readout lines were constructed utilizing 10 low-noise amplifiers (LNAs). The performance of the device is characterized using a vector network analyzer (VNA) and a homodyne scheme at various temperatures between 20 and 495 mK, producing preliminary results of pulse response and energy resolution (energy resolving power) under illumination delivered through an optical fiber at 405 nm. The measured resonant frequencies of the KIDs range from 3.8 to 8.5 GHz. The energy resolution of the resonator initially improves with increasing temperature but subsequently degrades. So far, the best measured energy resolution is 2.5 at 275 mK and 405 nm.

kinetic inductance detector

single photon

KID

SPIAKID

energy resolution

Author

Zhaohang Peng

Paris Observatory

Paris Descartes University

Faouzi Boussaha

Paris Observatory

Piercarlo Bonifacio

Observatoire de Paris-Meudon

Jie Hu

Chinese Academy of Sciences

Paul Nicaise

Chalmers, Microtechnology and Nanoscience (MC2), Quantum Technology

Paris Observatory

Chinese Academy of Sciences

Christine Chaumont

Paris Observatory

Florent Reix

Paris Observatory

Josiane Firminy

Paris Observatory

Elisabetta Caffau

Observatoire de Paris-Meudon

Cyril Pannetier

Paris Observatory

Jean Philippe Amans

Paris Observatory

Moustapha Dekkali

Observatoire de Paris-Meudon

Thibaut Vacelet

Observatoire de Paris-Meudon

Alexine Marret

Chinese Academy of Sciences

David Horville

Chinese Academy of Sciences

M. Piat

Paris Descartes University

IEEE Transactions on Applied Superconductivity

1051-8223 (ISSN) 15582515 (eISSN)

Vol. In Press

Subject Categories (SSIF 2025)

Other Electrical Engineering, Electronic Engineering, Information Engineering

Astronomy, Astrophysics, and Cosmology

DOI

10.1109/TASC.2026.3696967

More information

Latest update

6/11/2026