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This page is a summary of: An ultra wide-band, high-sensitivity Q-band receiver for single-dish telescopes, eQ: Rest-frequency determination of CCS (JN = 43–32) and SO (JN = 10–01) and high-redshift CO (J = 1–0) detection, Publications of the Astronomical Society of Japan, June 2024, Oxford University Press (OUP),
DOI: 10.1093/pasj/psae029.
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