A Study on a Delay-Line-Based Ramp-Compare ADC for Radio Astronomical Applications-Reference-Cited by-同舟云学术

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A Study on a Delay-Line-Based Ramp-Compare ADC for Radio Astronomical Applications

Published:2022-11-29 Issue: Volume: Page:
ISSN:
Container-title:2022 Asia-Pacific Microwave Conference (APMC)
language:
Short-container-title:

Author:

Nishimura Atsushi¹,Matsumoto Takeru²,Matsue Yudai³,Yonetsu Teppei²,Nakao Yuka⁴,Fujita Shinji²,Maezawa Hiroyuki²,Tachihara Kengo³,Onishi Toshikazu²,Ogawa Hideo²

Affiliation:

1. Nobeyama Radio Observatory, National Astronomical Observatory of Japan, National Institutes of Natural Sciences,Minamisaku,Nagano,Japan,384-1305

2. School of Science, Osaka Metropolitan University,Department of Physics, Graduate,Sakai,Osaka,Japan,599-8531

3. Graduate School of Science, Nagoya University,Department of Physics,Nagoya,Aichi,Japan,464-8602

4. Graduate School of Science, Osaka Prefecture University,Department of Physical Science,Sakai,Osaka,Japan,599-8531

Publisher

IEEE

Link

http://xplorestaging.ieee.org/ielx7/9999720/9999721/09999809.pdf?arnumber=9999809

Reference10 articles.

1. Development of the new multi-beam 100 GHz band SIS receiver FOREST for the Nobeyama 45-m Telescope

2. Submillimeter heterodyne arrays for APEX;MGüsten,2008

3. Argus: a 16-pixel millimeter-wave spectrometer for the Green Bank Telescope

4. Demonstration of a wideband submillimeter-wave low-noise receiver with 4–21 GHz IF output digitized by a high-speed 32 GSps ADC

5. Development of a new wideband heterodyne receiver system for the Osaka 1.85 m mm–submm telescope: Receiver development and the first light of simultaneous observations in 230 GHz and 345 GHz bands with an SIS-mixer with 4–21 GHz IF output

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