Development of Multi-temperature Calibrator for the TES Bolometer Camera: System Design

被引:2
|
作者
Takekoshi, Tatsuya [1 ,2 ,3 ]
Ohtawara, Kazushige [2 ]
Oshima, Tai [2 ,4 ]
Ishii, Shun [2 ,5 ]
Izumi, Natsuko [2 ]
Izumi, Takuma [2 ,3 ]
Yamaguchi, Masayuki [2 ,6 ]
Suzuki, Shunta [7 ]
Muraoka, Kazuyuki [7 ]
Hirota, Akihiko [2 ,5 ]
Saito, Fumiaki [8 ]
Nakatsubo, Shunichi [9 ]
Kouchi, Akira [8 ]
Ito, Tetsuya [2 ]
Uemizu, Kazunori [2 ]
Fujii, Yasunori [2 ]
Tamura, Yoichi [10 ]
Kohno, Kotaro [3 ]
Kawabe, Ryohei [2 ,4 ]
机构
[1] Univ Electrocommun, Grad Sch Informat & Engn, Chofu, Tokyo 1828585, Japan
[2] Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan
[3] Univ Tokyo, Inst Astron, Mitaka, Tokyo 1810015, Japan
[4] SOKENDAI Grad Univ Adv Studies, Dept Astron Sci, Sch Phys Sci, Mitaka, Tokyo 1818588, Japan
[5] JAO, Santiago 7630355, Chile
[6] Univ Tokyo, Grad Sch Sci, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan
[7] Osaka Prefecture Univ, Grad Sch Sci, Sakai, Osaka 5998531, Japan
[8] Hokkaido Univ, Inst Low Temp Sci, Sapporo, Hokkaido 0600819, Japan
[9] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2525210, Japan
[10] Nagoya Univ, Dept Astrophys, Nagoya, Aichi 4648602, Japan
关键词
Sub-mm astronomy; Transition-edge sensor; Calibration;
D O I
10.1007/s10909-018-1916-1
中图分类号
O59 [应用物理学];
学科分类号
摘要
We developed a simple add-on, cryogen-free, and low-power consumption calibrator for a new transition-edge sensor (TES) bolometer camera mounted on the ASTE 10-m telescope. To measure the responsivity of the TES bolometers and accurately correct for the nonlinearity and atmospheric extinction, we designed a motor-driven rotating filter wheel system installed in front of the cryostat window. This calibrator is required to cover the loading power under various atmospheric conditions, which corresponds to precipitable water vapor (PWV) of 0.5-4 mm. For this range of PWV, 25-100 K blackbodies are necessary for the observing bands of 1.1 and 0.85 mm. To simulate the temperature range, bolometers in the cryostat are also optically coupled to the low-temperature stage (< 4K) inside the cryostat by spherical mirrors. In addition, we used moderately absorptive polystyrene plates that are placed between a spherical mirror and the cryostat window. Various combinations of filters result in eight different temperatures by the filter wheel system and simulate the atmospheric emission under various weather conditions at the ASTE site.
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页码:1003 / 1009
页数:7
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