2018
DOI: 10.1007/s10909-018-2077-y
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GroundBIRD: Observation of CMB Polarization with a Rapid Scanning and MKIDs

Abstract: 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 the B-mode on large angular scales from the ground. One of the most novel characteristics of the telescope uses for this experiment is its rapid rotational scanning techniq… Show more

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Cited by 8 publications
(10 citation statements)
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“…There are multiple CMB B-mode experiments ongoing and in late planning phases at the moment, and MKIDs are considered for several of them and already utilized in some. GroundBIRD [77][78][79] is searching for the CMB B-mode polarization with a 30 cm telescope that rotates rapidly (about 20 rounds per minute) on a horizontal platform to enhance noise suppression. It uses 161 MKID pixels in two bands centered around 145 GHz (2.1 mm, 138 pixels) and 220 GHz (1.4 mm, 23 pixels) and will start observing from Teide Observatory, Tenerife soon.…”
Section: Mkid Mid-ir To Microwave Imagersmentioning
confidence: 99%
“…There are multiple CMB B-mode experiments ongoing and in late planning phases at the moment, and MKIDs are considered for several of them and already utilized in some. GroundBIRD [77][78][79] is searching for the CMB B-mode polarization with a 30 cm telescope that rotates rapidly (about 20 rounds per minute) on a horizontal platform to enhance noise suppression. It uses 161 MKID pixels in two bands centered around 145 GHz (2.1 mm, 138 pixels) and 220 GHz (1.4 mm, 23 pixels) and will start observing from Teide Observatory, Tenerife soon.…”
Section: Mkid Mid-ir To Microwave Imagersmentioning
confidence: 99%
“…( 3). This method requires that X system is lower than the contribution of the first term in Eq (5). Moreover, another contribution due to a two level system noise 20 should be low enough in the case of the phase response.…”
mentioning
confidence: 99%
“…Therefore, compared with other types of superconducting detectors, there is an advantage in constructing a large format array. In particular, the field of radio astronomy has started using antenna-coupled MKID arrays [2][3][4].…”
mentioning
confidence: 99%
“…The diagram of our setup is shown in Figure 2. Our cryostat consists of 4 K, 40 K, and 300 K thermal shields [4], and is cooled using a pulse tube refrigerator (PT415, Cryomech Co. Ltd). Magnetic shields (MS-FR, Hitachi material) were set outside of the 40 K and 300 K thermal shields; three sheets were set outside of the 40 K shield, three sheets (four sheets) were set outside the wall (bottom plate) of the 300 K shield.…”
mentioning
confidence: 99%
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