A Submillimeter Cartridge-Type Receiver: ALMA Band 8 (385-500 GHz) Qualification Model
文献类型：期刊论文
| 作者 | Satou, Naohisa1,2; Sekimoto, Yutaro1,2; Iizuka, Yoshizou1,2; Ito, Tetsuya1,2; Shan, Wen-Lei1,2,3; Kamba, Toshiaki1,2; Kumagai, Kazuyoshi1,2; Kamikura, Mamoru1,2,4; Tomimura, Yu1,2,4; Serizawa, Yasutaka1,2,4 |
| 刊名 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
 |
| 出版日期 | 2008 |
| 卷号 | 60期号:5页码:1199-1207 |
| 关键词 | instrumentation: detectors submillimeter |
| ISSN号 | 0004-6264 |
| 英文摘要 | We have developed a cartridge-type receiver covering the frequency band of 385-500GHz as a qualification model of Atacama Large Millimeter/submillimeter Array (ALMA) band 8. It receives two orthogonal polarizations and down-converts the sideband-separated signals to intermediate frequencies (IF) of between 4 and 8GHz. The cartridge-type receiver consists of cold optics, two feed horns, a wire grid, mirrors, two sideband-separating SIS mixers, cryogenic multipliers of a local oscillator (LO), cryogenic and warm IF amplifiers, a cartridge body, and sensors/wirings. These components were individually tested, and then the cartridge was integrated and tested as a complete assembly. We have also developed equipment for efficiency tests of both the components and the integrated receiver. The single sideband (SSB) noise temperature of this receiver is 100K at the band center and 300K at the band edges. The beam pattern and cross-polarization pattern are consistent with a physical optical calculation. The amplitude stability is around 3 x 10(-4) in 1 s. The phase stability is less than 2.degrees 0 on a time scale of 0.1 s to 10 min. These results are promising for a receiver in the ALMA. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | SIS MIXER ; TELESCOPE ; ARRAY |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000265243900024 |
| 公开日期 | 2011-12-29 |
| 源URL | [http://159.226.72.40/handle/332002/1793]  |
| 专题 | 紫金山天文台_毫米波和亚毫米波技术实验室 |
| 作者单位 | 1.Natl Astron Observ Japan, Adv Technol Ctr, Tokyo 1818588, Japan 2.Natl Astron Observ Japan, ALMA J Project Off, Tokyo 1818588, Japan 3.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 4.Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan |
| 推荐引用方式 GB/T 7714 | Satou, Naohisa,Sekimoto, Yutaro,Iizuka, Yoshizou,et al. A Submillimeter Cartridge-Type Receiver: ALMA Band 8 (385-500 GHz) Qualification Model[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,2008,60(5):1199-1207. |
| APA | Satou, Naohisa.,Sekimoto, Yutaro.,Iizuka, Yoshizou.,Ito, Tetsuya.,Shan, Wen-Lei.,...&Sugimoto, Masahiro.(2008).A Submillimeter Cartridge-Type Receiver: ALMA Band 8 (385-500 GHz) Qualification Model.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,60(5),1199-1207. |
| MLA | Satou, Naohisa,et al."A Submillimeter Cartridge-Type Receiver: ALMA Band 8 (385-500 GHz) Qualification Model".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 60.5(2008):1199-1207. |
入库方式： OAI收割
来源：紫金山天文台
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。