On-site performance of GroundBIRD, a CMB polarization telescope for large angular scale observations

Conference Paper (2020)
Authors

Shunsuke Honda (Kyoto University)

Jihoon Choi (Korea Astronomy and Space Science Institute)

R. T. Génova-Santos (Instituto de Astrofísica de Canarias)

Makoto Hattori (Tohoku University)

Masashi Hazumi (Graduate University for Advanced Studies (SOKENDAI), High Energy Accelerator Research Organization, Tsukuba)

Takuji Ikemitsu (Kyoto University)

Hidesato Ishida (Tohoku University, Institute of Physical and Chemical Research)

Hikaru Ishitsuka (Graduate University for Advanced Studies (SOKENDAI))

Kenichi Karatsu (TU Delft - Tera-Hertz Sensing, SRON–Netherlands Institute for Space Research)

G.B. More authors (External organisation)

Research Group
Tera-Hertz Sensing
To reference this document use:
https://doi.org/10.1117/12.2560918
More Info
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Publication Year
2020
Language
English
Research Group
Tera-Hertz Sensing
ISBN (electronic)
9781510636774
DOI:
https://doi.org/10.1117/12.2560918

Abstract

GroundBIRD is a millimeter-wave telescope to observe the polarization patterns of the cosmic microwave background (CMB). The target science topics are primordial gravitational waves from cosmic inflation and reionization optical depth. Therefore, this telescope is designed to achieve the highest sensitivity at large angular scales, ℓ = 6 - 300. For wide sky observations (∼40% full-sky), scanning at a high rotation speed (120°/s) is important to remove atmospheric fluctuations. Microwave kinetic inductance detector (MKID) is utilized with the fast GroundBIRD rotation since its good time response. We have started the commissioning run at the Teide Observatory in the Canary Islands. We report the performance of the telescope, receiver, and data acquisition system, including cooling achievements, observations of astronomical objects, and observations taken during several days ahead of our main survey observations.

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