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Updated: Jun 1, 2026

Fabrication and Characterization of Superconducting Resonators
Published on: May 21, 2016
Calibration system with cryogenically-cooled loads for cosmic microwave background polarization detectors
M Hasegawa1, O Tajima, Y Chinone
1Institute of Particle and Nuclear Studies, High Energy Accelerator Research Organization (KEK), Oho, Tsukuba, Ibaraki, 305-0801, Japan.
We developed a new lab system using cooled blackbody absorbers to calibrate cosmic microwave background (CMB) polarimeters. This method simulates real observing conditions for more accurate CMB polarization measurements.
Area of Science:
- Astrophysics
- Cosmology
- Instrumentation
Background:
- Accurate calibration of polarimeters is crucial for cosmic microwave background (CMB) polarization measurements.
- Existing calibration methods may not fully replicate the faint polarized signals observed in space.
Purpose of the Study:
- To introduce a novel laboratory system for calibrating millimeter-wave polarimeters.
- To enable the simulation of faint polarized signals (∼100 mK) in a controlled environment.
Main Methods:
- The system extends conventional metal mirror rotation techniques.
- It utilizes cryogenically-cooled blackbody absorbers to generate a slightly polarized signal.
- The design and principle of the calibration system are detailed.
Main Results:
- The system successfully generates a polarized signal at a level comparable to ground-based CMB observations.
- Demonstrated the system's utility with a coherent-type polarimeter for CMB experiments.
- The technique is applicable to both coherent and incoherent polarimeters.
Conclusions:
- This novel calibration system accurately reproduces laboratory observing conditions for polarimeters.
- It is a promising tool for next-generation cosmic microwave background polarization experiments.
- Enhances the reliability and precision of CMB polarization data analysis.
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