English

Lumped Element Kinetic Inductance Detectors for space applications

Instrumentation and Methods for Astrophysics 2017-01-18 v1

Abstract

Kinetic Inductance Detectors (KID) are now routinely used in ground-based telescopes. Large arrays, deployed in formats up to kilopixels, exhibit state-of-the-art performance at millimeter (e.g. 120-300 GHz, NIKA and NIKA2 on the IRAM 30-meters) and sub-millimeter (e.g. 350-850 GHz AMKID on APEX) wavelengths. In view of future utilizations above the atmosphere, we have studied in detail the interaction of ionizing particles with LEKID (Lumped Element KID) arrays. We have constructed a dedicated cryogenic setup that allows to reproduce the typical observing conditions of a space-borne observatory. We will report the details and conclusions from a number of measurements. We give a brief description of our short term project, consisting in flying LEKID on a stratospheric balloon named B-SIDE.

Keywords

Cite

@article{arxiv.1606.00719,
  title  = {Lumped Element Kinetic Inductance Detectors for space applications},
  author = {Alessandro Monfardini and Jochem Baselmans and Alain Benoit and Aurelien Bideaud and Olivier Bourrion and Andrea Catalano and Martino Calvo and Antonio D'Addabbo and Simon Doyle and Johannes Goupy and Helene Le Sueur and Juan Macias-Perez and NIKA2 collaboration and SPACEKIDS collaboration and B-SIDE collaboration},
  journal= {arXiv preprint arXiv:1606.00719},
  year   = {2017}
}

Comments

To appear in the SPIE 2016 Proceedings

R2 v1 2026-06-22T14:15:59.073Z