A 220–320 GHz High Image Rejection Sideband Separating Receiver for Space-Borne Observatories-Reference-Cited by-同舟云学术

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A 220–320 GHz High Image Rejection Sideband Separating Receiver for Space-Borne Observatories

Published:2024-03 Issue:2 Volume:14 Page:162-177
ISSN:2156-342X
Container-title:IEEE Transactions on Terahertz Science and Technology
language:
Short-container-title:IEEE Trans. THz Sci. Technol.

Author:

Seragi Ebrahim M. Al¹^ORCID,Rajendra Yashas L.¹^ORCID,Ahmad Waleed²^ORCID,Kaynak Mehmet³,Goldsmith Paul F.⁴^ORCID,Zeinolabdedinzadeh Saeed¹^ORCID

Affiliation:

1. School of Electrical, Computer, and Energy Engineering, Arizona State University, Tempe, AZ, USA

2. Arizona State University, Tempe, AZ, USA

3. IHP Microelectronics, Frankfurt, Germany

4. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA

Funder

Jet Propulsion Laboratory

Publisher

Institute of Electrical and Electronics Engineers (IEEE)

Link

http://xplorestaging.ieee.org/ielx7/5503871/10459091/10379818.pdf?arnumber=10379818

Reference90 articles.

1. Sub-millimeter heterodyne focal-plane arrays for high-resolution astronomical spectroscopy

2. A Calibrated Digital Sideband Separating Spectrometer for Radio Astronomy Applications

3. Design and Performance of a 600–720-GHz Sideband-Separating Receiver Using ${\hbox{AlO}}_{x}$ and AlN SIS Junctions

4. Sideband separating mixer for 600-720 GHz

5. Design of a side-band-separating heterodyne mixer for band 9 of ALMA

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