GroundBIRD: Observation of CMB Polarization with a Rapid Scanning and MKIDs
GroundBIRD: Observation of CMB Polarization with a Rapid Scanning and MKIDs
复制标题
GroundBIRD:通过快速扫描和 MKID 观测 CMB 偏振
DOI:
10.1007/s10909-018-2077-y
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发表时间:
2018
影响因子:
2
通讯作者:
Nagasaki T. et al.
中科院分区:
文献类型:
--
作者:
Kutsuma Hiroki;Hattori Makoto;Kiuchi Kenji;Mima Satoru;Nagasaki Taketo;Oguri Shugo;Suzuki Junya;Tajima Osamu;Nagasaki T. et al.
Cosmic microwave background (CMB) radiation is an afterglow from the Big Bang. CMB contains rich information about the early stage of the universe. In particular, odd-parity patterns (B-mode) in the CMB polarization on a large angular scale would provide an evidence of the cosmic inflation. The aim of the GroundBIRD experiment is to observe theB-mode on large angular scales from the ground. One of the most novel characteristics of the telescope used for this experiment is its rapid rotational scanning technique. In addition, the telescope uses cold optics and microwave kinetic inductance detectors. We have developed a telescope mount with a three-axis rotation mechanism (azimuth, elevation, and boresight) and measured the vibration at the focal plane stage at 20 RPM scan rotation rate. We also performed focal plane detector tests on this mount. The tests confirmed the expected response from the geomagnetism associated with the mount rotation. We have also developed a design for the magnetic shields and a detector array on a 3-in wafer. The preparations to begin the observations at the Teide Observatory in the Canary Islands in 2018 are proceeding smoothly.