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The Simons Observatory: A fully remote controlled calibration system with a sparse wire grid for cosmic microwave
Masaaki Murata1, Hironobu Nakata2, Kengo Iijima1
1Department of Physics, The University of Tokyo, Tokyo 113-0033, Japan.
The Review of Scientific Instruments
|December 18, 2023
Summary
A new remote-controlled calibration system uses a sparse wire grid to precisely calibrate cosmic microwave background (CMB) polarization angles. This system enables regular, automated calibrations, improving accuracy for CMB observations.
Area of Science:
- Cosmology and Astrophysics
- Instrumental Development
Background:
- Accurate calibration of detector polarization angles is crucial for cosmic microwave background (CMB) observations.
- Previous sparse wire grid calibrators lacked remote-controlled capabilities for regular calibration.
Purpose of the Study:
- To develop a fully remote-controlled calibration system for CMB polarization observations.
- To enable regular and automated calibration of detector polarization angles.
Main Methods:
- A sparse wire grid reflects linearly polarized light along the wire direction.
- Two electric linear actuators remotely position the grid on the telescope's optical axis.
- A motor rotates the grid, with a rotary encoder and gravity sensor monitoring wire direction.
Main Results:
- Achieved detector polarization angle calibration with an expected systematic error of 0.08°.
- Developed a novel remote-controlled system for sparse wire grid calibrators.
Conclusions:
- The new system allows for regular, automated calibration, a significant advancement for CMB experiments.
- The system will be implemented in small-aperture telescopes at Simons Observatory, enhancing data quality.

