4.7 Article

Integration of a Testbench for the Optical and Thermal Characterization of Near-Infrared Detectors Used in Ground and Space-Based Astronomy

出版社

IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
DOI: 10.1109/TIM.2020.3046923

关键词

Characterization setup; infrared detectors; temperature control; vacuum dewar

资金

  1. European Commission [H2020-COMPET-2016-730161]
  2. Spanish Ministerio de Ciencia, Innovacion y Universidades [PID2019-11317GB-C32, ESP2017-89838-C3-2-R]
  3. Institut de Fisica d'Altes Energies (IFAE) through the Centres de Recerca de Catalunya (CERCA) Program of the Generalitat de Catalunya

向作者/读者索取更多资源

The ASTEROID project aims to develop high-performance infrared FPAs for astronomical scientific missions in Europe and promote self-sufficiency. IFAE will lead the task of validating detector performance, including assessing the reliability between the readout integrated circuit and the MCT detector through multiple low-temperature thermal cycles.
The mercury-cadmium-tellurium (MCT) sensors are considered the ideal infrared detectors to equip the focal plane arrays (FPAs) of astronomical scientific missions. To tackle Europe to be self-sufficient on this technology and promote to reach the same maturity level attained by the current MCT sensors market leaders, the Astronomy European Infrared Detector (ASTEROID) project aims to provide Europe with the capability to manufacture high-performance infrared FPAs devoted to scientific use, space astronomy, and ground-based telescope infrastructures. The resulting detector will he a hybridized MCT array with a CdZnTe substrate of 2k x 2k pixels and 15 mu m of pixel pitch. The Institut de Fisica d'Altes Energies (IFAE) will lead the task to validate the detector performance with respect to the hybridization reliability between the readout integrated circuit (ROIC) and the MCT detector by submitting it to several low-temperature thermal cycles. After every thermal stress, the detector will be optically characterized in order to measure any performance degradation and possible problems with the pixel operability. To perform such tasks, two custom setups, focused on optical and cryo-vacuum aspects, were developed, which, used in conjunction, allows to cool down the detector from the room temperature up to similar to 30 K, while it is electro-optically characterized in terms of linearity, gain, quantum efficiency, and cosmetics defects, among others. The whole cryo-vacuum system and the optical setup are fully described in this article as part of the work packages assigned to IFAE to test the hybridized detector to assess the reliability at operating temperature and after several thermal cycles.

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