# The POLARBEAR Fourier Transform Spectrometer Calibrator and   Spectroscopic Characterization of the POLARBEAR Instrument

**Authors:** Frederick Matsuda, Lindsay Lowry, Aritoki Suzuki, Mario Aguilar, Faundez, Kam Arnold, Darcy Barron, Federico Bianchini, Kolen Cheung, Yuji, Chinone, Tucker Elleflot, Giulio Fabbian, Neil Goeckner-Wald, Masaya, Hasegawa, Daisuke Kaneko, Nobuhiko Katayama, Brian Keating, Adrian Lee,, Martin Navaroli, Haruki Nishino, Hans Paar, Giuseppe Puglisi, Paul Richards,, Joseph Seibert, Praween Siritanasak, Osamu Tajima, Sayuri Takatori, Calvin, Tsai, Ben Westbrook

arXiv: 1904.02901 · 2020-01-28

## TL;DR

This paper details the design, construction, and in-field use of the POLARBEAR Fourier Transform Spectrometer (FTS) for calibrating and characterizing the POLARBEAR CMB polarization experiment, highlighting its unique features and future applications.

## Contribution

The paper introduces a novel FTS calibrator with high throughput and continuous modulation, optimized for in-field spectral characterization of CMB instruments.

## Key findings

- Achieved high SNR spectral measurements for 69% of detectors
- Designed a parabolic mirror mimicking the telescope's primary reflector
- Demonstrated in-field calibration of the POLARBEAR receiver

## Abstract

We describe the Fourier Transform Spectrometer (FTS) used for in-field testing of the POLARBEAR receiver, an experiment located in the Atacama Desert of Chile which measures the cosmic microwave background (CMB) polarization. The POLARBEAR-FTS (PB-FTS) is a Martin-Puplett interferometer designed to couple to the Huan Tran Telescope (HTT) on which the POLARBEAR receiver is installed. The PB-FTS measured the spectral response of the POLARBEAR receiver with signal-to-noise ratio (SNR) $>20$ for $\sim$69% of the focal plane detectors due to three features: a high throughput of 15.1 steradian cm$^{2}$, optimized optical coupling to the POLARBEAR optics using a custom designed output parabolic mirror, and a continuously modulated output polarizer. The PB-FTS parabolic mirror is designed to mimic the shape of the 2.5 m-diameter HTT primary reflector which allows for optimum optical coupling to the POLARBEAR receiver, reducing aberrations and systematics. One polarizing grid is placed at the output of the PB-FTS, and modulated via continuous rotation. This modulation allows for decomposition of the signal into different harmonics that can be used to probe potentially pernicious sources of systematic error in a polarization-sensitive instrument. The high throughput and continuous output polarizer modulation features are unique compared to other FTS calibrators used in the CMB field. In-field characterization of the POLARBEAR receiver was accomplished using the PB-FTS in April 2014. We discuss the design, construction, and operation of the PB-FTS and present the spectral characterization of the POLARBEAR receiver. We introduce future applications for the PB-FTS in the next-generation CMB experiment, the Simons Array.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1904.02901/full.md

## Figures

28 figures with captions in the complete paper: https://tomesphere.com/paper/1904.02901/full.md

## References

29 references — full list in the complete paper: https://tomesphere.com/paper/1904.02901/full.md

---
Source: https://tomesphere.com/paper/1904.02901