Ding, Junjia, Ade, Peter A. R. ![]() ![]() |
Preview |
PDF
- Published Version
Download (1MB) | Preview |
Abstract
In this paper, we describe the optimization of transition-edge-sensor (TES) detector arrays for the third-generation camera for the South Pole Telescope. The camera, which contains ~16 000 detectors, will make high-angular-resolution maps of the temperature and polarization of the cosmic microwave background. Our key results are scatter in the transition temperature of Ti/Au TESs is reduced by fabricating the TESs on a thin Ti(5 nm)/Au(5 nm) buffer layer and the thermal conductivity of the legs that support our detector islands is dominated by the SiOx dielectric in the microstrip transmission lines that run along the legs.
Item Type: | Article |
---|---|
Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | IEEE |
ISSN: | 1051-8223 |
Date of First Compliant Deposit: | 6 July 2017 |
Date of Acceptance: | 8 December 2016 |
Last Modified: | 04 May 2023 20:26 |
URI: | https://orca.cardiff.ac.uk/id/eprint/102146 |
Citation Data
Cited 15 times in Scopus. View in Scopus. Powered By Scopus® Data
Actions (repository staff only)
![]() |
Edit Item |