Characterization of a 200-GHz SIS mixer

Chi C. Chin; Sung Shiou Shen; Shu-I Hu; Shun Cheng Yang; Robert N. Martin

doi:10.1117/12.317393

Characterization of a 200-GHz SIS mixer

Chi C. Chin, Sung Shiou Shen, Shu-I Hu, Shun Cheng Yang, Robert N. Martin

Institute of Electronics

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

Abstract

We report on the status of SIS mixers being constructed at the Institute of Astronomy and Astrophysics, Academia Sinica. These mixers will later be integrated into the receiver systems used on the ASIAA supplied antennas for the SMA project. We have reproduced the SAO design for these mixers at the 200 GHz band. We achieve acceptable noise performance across the tuning band of the mixers.

Original language	English
Pages (from-to)	587-592
Number of pages	6
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	3357
DOIs	https://doi.org/10.1117/12.317393
State	Published - 1 Dec 1998
Event	Advanced Technology MMW, Radio, and Terahertz Telescopes - Kona, HI, United States Duration: 26 Mar 1998 → 26 Mar 1998

Keywords

Heterodyne detectors
Mixers
SIS
Submillimeter waves

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title = "Characterization of a 200-GHz SIS mixer",

abstract = "We report on the status of SIS mixers being constructed at the Institute of Astronomy and Astrophysics, Academia Sinica. These mixers will later be integrated into the receiver systems used on the ASIAA supplied antennas for the SMA project. We have reproduced the SAO design for these mixers at the 200 GHz band. We achieve acceptable noise performance across the tuning band of the mixers.",

keywords = "Heterodyne detectors, Mixers, SIS, Submillimeter waves",

author = "Chin, {Chi C.} and Shen, {Sung Shiou} and Shu-I Hu and Yang, {Shun Cheng} and Martin, {Robert N.}",

year = "1998",

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T1 - Characterization of a 200-GHz SIS mixer

AU - Chin, Chi C.

AU - Shen, Sung Shiou

AU - Hu, Shu-I

AU - Yang, Shun Cheng

AU - Martin, Robert N.

PY - 1998/12/1

Y1 - 1998/12/1

N2 - We report on the status of SIS mixers being constructed at the Institute of Astronomy and Astrophysics, Academia Sinica. These mixers will later be integrated into the receiver systems used on the ASIAA supplied antennas for the SMA project. We have reproduced the SAO design for these mixers at the 200 GHz band. We achieve acceptable noise performance across the tuning band of the mixers.

AB - We report on the status of SIS mixers being constructed at the Institute of Astronomy and Astrophysics, Academia Sinica. These mixers will later be integrated into the receiver systems used on the ASIAA supplied antennas for the SMA project. We have reproduced the SAO design for these mixers at the 200 GHz band. We achieve acceptable noise performance across the tuning band of the mixers.

KW - Heterodyne detectors

KW - Mixers

KW - SIS

KW - Submillimeter waves

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U2 - 10.1117/12.317393

DO - 10.1117/12.317393

M3 - Conference article

AN - SCOPUS:58749083032

VL - 3357

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EP - 592

JO - Proceedings of SPIE - The International Society for Optical Engineering

JF - Proceedings of SPIE - The International Society for Optical Engineering

SN - 0277-786X

Y2 - 26 March 1998 through 26 March 1998

ER -

Characterization of a 200-GHz SIS mixer

Abstract

Keywords

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