Paper PC13102-67
The Terahertz Intensity Mapper: design, modeling, and characterization of the cryogenic receiver
21 June 2024 • 16:50 - 17:10 Japan Standard Time | Room G318/319, North - 3F
Abstract
The Terahertz Intensity Mapper (TIM) is a NASA-funded balloon-borne telescope that aims to measure the [CII] emission from star forming galaxies over an enormous cosmic volume. TIM’s cryogenic receiver, based on the BLAST-TNG design, utilizes a three-stage He sorption refrigerator backed by a 280-liter liquid helium tank to achieve a base temperature of 250 mK, which enables photon noise-limited performance for its MKID detectors. Two low-impedance multi-channel heat exchangers enhance cooling efficiency, contributing to a designed hold time of 20 days under ground conditions. Preliminary simulations and assembly tests showcase the cryostat's reliability, and data validation is anticipated by the summer of 2024. We will present the design and current status of the TIM cryogenic receiver and our ongoing characterization effort toward an Antarctic flight in 2026.
Presenter
Univ. of Illinois (United States)
Jianyang Fu holds Bachelor of Science degrees in Physics and Astronomy (Highest distinction) from the University of Illinois Urbana-Champaign. During this period, he contributed to the development of the readout electronics, as well as the millimeter-wave anti-reflection coatings for the SPT-3G telescope.
Currently pursuing a Ph.D. at the University of Illinois Urbana-Champaign, Mr. Fu is working on modeling, characterization, and deployment of the cryogenic receiver for the Terahertz Intensity Mapper(TIM) experiment.