A Wideband Millimeter-Wave Corrugated Horn at 30–50 GHz Taking Advantage of All-Metal 3-D Printing Fabrication

Kang, Heau-Jo; Kaneko, Keiko; Sakai, Ryo; González, Álvaro

doi:10.1109/lawp.2023.3245642

Search citation statements

Order By: Relevance

Paper Sections

Select...

Citation Types

Supporting

Mentioning

Contrasting

Year Published

2024

Publication Types

Select...

Other2

Article1

Relationship

Self Cite0

Independent3

Authors

Journals

Cited by 3 publications

References 20 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

3-D Printed Multifocusing Truncated Gutman Lens With High-Efficient MMIC Class-F Load GaAs Rectenna for mm-Wave Battery-Free IoT Application

Shao,

Yang,

Shinohara

2024

IEEE Trans. Compon., Packag. Manufact. Technol.

View full text Add to dashboard Cite

3-D Printed Multifocusing Truncated Gutman Lens With High-Efficient MMIC Class-F Load GaAs Rectenna for mm-Wave Battery-Free IoT Application

Shao,

Yang,

Shinohara

2024

IEEE Trans. Compon., Packag. Manufact. Technol.

View full text Add to dashboard Cite

Development status of wideband millimeter-wave receivers for LMT-FINER

Kang,

Kojima,

Sakai

et al. 2024

Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII

View full text Add to dashboard Cite

Spectroscopic observations of the far-infrared [O iii] 88 µm and [C ii] 158 µm lines present a pathway to explore the mechanisms of the emergence of massive galaxies in the epoch of reionization and beyond, which is one of the most fundamental questions in astronomy. To address this question, the Far-Infrared Nebular Emission Receiver (FINER) project is developing two wideband dual-polarization sideband-separating heterodyne receivers at 120-210 GHz and 210-360 GHz for the Large Millimeter Telescope (LMT) in Mexico. Compared with Atacama Large Millimeter/submillimeter Array (ALMA), LMT provides 40% of ALMA's light-collecting area and a similar atmospheric transmittance, but FINER plans to have an instantaneous intermediate frequency (IF) of 3-21 GHz per sideband per polarization which is five times wider than current ALMA's bandwidth. Therefore, FINER is going to offer cutting-edge spectral scanning capability in the next several years.The project is currently in an active development phase. In this proceeding, the latest development status for FINER, including the optics, wideband waveguide components as well as low-noise superconductor-insulatorsuperconductor (SIS) mixers is reported.

show abstract

Layering it All: Stripline-to-Waveguide Transitions for Corrugated Horns at W-band

Nozinic,

Rämer,

Dischke

et al. 2024

2024 54th European Microwave Conference (EuMC)

View full text Add to dashboard Cite

A Wideband Millimeter-Wave Corrugated Horn at 30–50 GHz Taking Advantage of All-Metal 3-D Printing Fabrication

Cited by 3 publications

References 20 publications

3-D Printed Multifocusing Truncated Gutman Lens With High-Efficient MMIC Class-F Load GaAs Rectenna for mm-Wave Battery-Free IoT Application

3-D Printed Multifocusing Truncated Gutman Lens With High-Efficient MMIC Class-F Load GaAs Rectenna for mm-Wave Battery-Free IoT Application

Development status of wideband millimeter-wave receivers for LMT-FINER

Layering it All: Stripline-to-Waveguide Transitions for Corrugated Horns at W-band

Contact Info

Product

Resources

About