Progress report on the sub-millimeter array in Taiwan: The receiver system

Ming Tang Chen; Shu Haur Chang; Chi Chung Chin; Tah Hsiung Chu; Shu-I Hu; Mao Shu Hwang; Yuh Jing Hwang; K. Y. Lo; Robert N. Martin; Pierre Martin-Cocher; Sung Shiou Shen; Shun Cheng Yang; Ming Jye Wang

doi:10.1117/12.390417

Progress report on the sub-millimeter array in Taiwan: The receiver system

Ming Tang Chen^*, Shu Haur Chang, Chi Chung Chin, Tah Hsiung Chu, Shu-I Hu, Mao Shu Hwang, Yuh Jing Hwang, K. Y. Lo, Robert N. Martin, Pierre Martin-Cocher, Sung Shiou Shen, Shun Cheng Yang, Ming Jye Wang

^*Corresponding author for this work

Institute of Electronics

Research output: Contribution to journal › Conference article › peer-review

Abstract

This is to report on our progress and current status of the Sub-Millimeter Array (SMA) project in Taiwan. In particular, we will describe the development of the SMA receiver systems. The SMA is the first major instrumentation project in the Taiwanese astronomical research community. The primary design and development of the SMA receiver system has been carried out in the receiver laboratory at the Smithsonian Astrophysical Observatory (SAO). We have undertaken the system assembly, integration and testing, and the task to fabricate the superconductor-insulator-superconductor (SIS) mixers used for our SMA receivers. The system will be initially equipped with two SIS receiver modules to cover 176-256 GHz and 250-350 GHz bands, followed with a third band of 600-720 GHz. The receiver system will be installed in the, antenna in the mid-2000. The major milestone for this project is to ship the antennas to Mauna Kea, Hawaii to join the rest of the SMA for testing interferometric observation before the end of the year 2000.

Original language	English
Pages (from-to)	247-252
Number of pages	6
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	4015
DOIs	https://doi.org/10.1117/12.390417
State	Published - 1 Jan 2000
Event	Radio Telescopes - Munich, Ger Duration: 27 Mar 2000 → 30 Mar 2000

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Chen, M. T., Chang, S. H., Chin, C. C., Chu, T. H., Hu, S-I., Hwang, M. S., Hwang, Y. J., Lo, K. Y., Martin, R. N., Martin-Cocher, P., Shen, S. S., Yang, S. C., & Wang, M. J. (2000). Progress report on the sub-millimeter array in Taiwan: The receiver system. Proceedings of SPIE - The International Society for Optical Engineering, 4015, 247-252. https://doi.org/10.1117/12.390417

Chen, Ming Tang ; Chang, Shu Haur ; Chin, Chi Chung ; Chu, Tah Hsiung ; Hu, Shu-I ; Hwang, Mao Shu ; Hwang, Yuh Jing ; Lo, K. Y. ; Martin, Robert N. ; Martin-Cocher, Pierre ; Shen, Sung Shiou ; Yang, Shun Cheng ; Wang, Ming Jye. / Progress report on the sub-millimeter array in Taiwan : The receiver system. In: Proceedings of SPIE - The International Society for Optical Engineering. 2000 ; Vol. 4015. pp. 247-252.

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title = "Progress report on the sub-millimeter array in Taiwan: The receiver system",

abstract = "This is to report on our progress and current status of the Sub-Millimeter Array (SMA) project in Taiwan. In particular, we will describe the development of the SMA receiver systems. The SMA is the first major instrumentation project in the Taiwanese astronomical research community. The primary design and development of the SMA receiver system has been carried out in the receiver laboratory at the Smithsonian Astrophysical Observatory (SAO). We have undertaken the system assembly, integration and testing, and the task to fabricate the superconductor-insulator-superconductor (SIS) mixers used for our SMA receivers. The system will be initially equipped with two SIS receiver modules to cover 176-256 GHz and 250-350 GHz bands, followed with a third band of 600-720 GHz. The receiver system will be installed in the, antenna in the mid-2000. The major milestone for this project is to ship the antennas to Mauna Kea, Hawaii to join the rest of the SMA for testing interferometric observation before the end of the year 2000.",

author = "Chen, {Ming Tang} and Chang, {Shu Haur} and Chin, {Chi Chung} and Chu, {Tah Hsiung} and Shu-I Hu and Hwang, {Mao Shu} and Hwang, {Yuh Jing} and Lo, {K. Y.} and Martin, {Robert N.} and Pierre Martin-Cocher and Shen, {Sung Shiou} and Yang, {Shun Cheng} and Wang, {Ming Jye}",

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Progress report on the sub-millimeter array in Taiwan : The receiver system. / Chen, Ming Tang; Chang, Shu Haur; Chin, Chi Chung; Chu, Tah Hsiung; Hu, Shu-I; Hwang, Mao Shu; Hwang, Yuh Jing; Lo, K. Y.; Martin, Robert N.; Martin-Cocher, Pierre; Shen, Sung Shiou; Yang, Shun Cheng; Wang, Ming Jye.

In: Proceedings of SPIE - The International Society for Optical Engineering, Vol. 4015, 01.01.2000, p. 247-252.

Research output: Contribution to journal › Conference article › peer-review

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T1 - Progress report on the sub-millimeter array in Taiwan

AU - Chen, Ming Tang

AU - Chang, Shu Haur

AU - Chin, Chi Chung

AU - Chu, Tah Hsiung

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AU - Hwang, Mao Shu

AU - Hwang, Yuh Jing

AU - Lo, K. Y.

AU - Martin, Robert N.

AU - Martin-Cocher, Pierre

AU - Shen, Sung Shiou

AU - Yang, Shun Cheng

AU - Wang, Ming Jye

PY - 2000/1/1

Y1 - 2000/1/1

N2 - This is to report on our progress and current status of the Sub-Millimeter Array (SMA) project in Taiwan. In particular, we will describe the development of the SMA receiver systems. The SMA is the first major instrumentation project in the Taiwanese astronomical research community. The primary design and development of the SMA receiver system has been carried out in the receiver laboratory at the Smithsonian Astrophysical Observatory (SAO). We have undertaken the system assembly, integration and testing, and the task to fabricate the superconductor-insulator-superconductor (SIS) mixers used for our SMA receivers. The system will be initially equipped with two SIS receiver modules to cover 176-256 GHz and 250-350 GHz bands, followed with a third band of 600-720 GHz. The receiver system will be installed in the, antenna in the mid-2000. The major milestone for this project is to ship the antennas to Mauna Kea, Hawaii to join the rest of the SMA for testing interferometric observation before the end of the year 2000.

AB - This is to report on our progress and current status of the Sub-Millimeter Array (SMA) project in Taiwan. In particular, we will describe the development of the SMA receiver systems. The SMA is the first major instrumentation project in the Taiwanese astronomical research community. The primary design and development of the SMA receiver system has been carried out in the receiver laboratory at the Smithsonian Astrophysical Observatory (SAO). We have undertaken the system assembly, integration and testing, and the task to fabricate the superconductor-insulator-superconductor (SIS) mixers used for our SMA receivers. The system will be initially equipped with two SIS receiver modules to cover 176-256 GHz and 250-350 GHz bands, followed with a third band of 600-720 GHz. The receiver system will be installed in the, antenna in the mid-2000. The major milestone for this project is to ship the antennas to Mauna Kea, Hawaii to join the rest of the SMA for testing interferometric observation before the end of the year 2000.

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Y2 - 27 March 2000 through 30 March 2000

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Progress report on the sub-millimeter array in Taiwan: The receiver system

Abstract

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