Characterization of a Ti/Au TES with Au/Bi absorber under AC and DC bias

23 Jul 2019, 17:45
1h 15m
Piazza Città di Lombardia (Milano)

Piazza Città di Lombardia

Milano

Piazza Città di Lombardia, 1, 20124 Milano MI
Poster Low Temperature Detector Development and Physics Poster session

Speaker

Carlos Pobes Aranda (ICMA)

Description

Transition Edge Sensors (TESs) are used as very sensitive thermometers in microcalorimeters aimed at different wavelengths detection. In particular, for soft X-ray astrophysics, science goals require very high resolution microcalorimeters which can be achieved with TESs coupled to suitable absorbers. For many applications there is also need for a high number of pixels which need to be multiplexed in the readout stage. Frequency Domain Multiplexing (FDM) is a common scheme and is the baseline proposed for the ATHENA mission. FDM requires biasing the TES in AC at MHz frequencies. Recently there has been reported degradation in performances under AC with respect to DC bias. In order to assess the performances of TESs to be used with FDM, it is thus of great interest to compare the performances of the same device under both types of bias. This means using two completely different setups and characterization protocols.
We report in this work a preliminary comparison of the characterization of a single pixel with a Ti/Au TES, performed under DC and AC bias in two different facilities. Dynamical parameters and noise are compared in both cases showing compatible results and has allowed definition of protocols for future AC/DC comparison of these devices.

Less than 5 years of experience since completion of Ph.D N
Student (Ph.D., M.Sc. or B.Sc.) N

Primary authors

Co-authors

Lourdes Fabrega (ICMAB-CSIC) Dr Agustín Camón (ICMA-CSIC) Dr Pourya Khosropanah (SRON - Netherlands Institute for Space Research) Luciano Gottardi (SRON - Netherlands Institute for Space Research) Mr Kenichiro Nagayoshi (SRON Netherlands Institute for Space Research) Mr Marcel Ridder (SRON Netherlands Institute for Space Research) Dr Marcel Bruijn (SRON - Netherlands Institute for Space Research) Dr Jian-Rong Gao (SRON - Netherlands Institute for Space Research)

Presentation Materials