K. Dobashi

activity

20032026

most citedPlanck Early Results: All sky temperature and dust optical depth from Planck and IRAS: Constraints on the "dark gas" in our galaxy

453 citations · 2.2k across the 50 of their papers we have counts for

collaborators

Showing 2024Show all

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astro-ph.GA2024

Q-band Line Survey Observations toward a Carbon-chain-rich Clump in the Serpens South Region

Kotomi Taniguchi, Fumitaka Nakamura, Sheng-Yuan Liu +17

We have conducted Q-band (30 GHz $-$ 50 GHz) line survey observations toward a carbon-chain emission peak in the Serpens South cluster-forming region with the extended Q-band (eQ)…

astro-ph.GA2024

An ultra wide-band, high-sensitivity Q-band receiver for single-dish telescopes, eQ: rest frequency determination of CCS ( $J_{N}$ = $4_{3}$ - $3_{2}$ ) and SO ( $J_{N}$ = $1_{0}$ - $0_{1}$ ), and high-redshift CO ( $J$ = 1-0) detection

Fumitaka Nakamura, Chau-Ching Chiong, Kotomi Taniguchi +16

We report on the development and commissioning of a new Q-band receiver for the Nobeyama 45-m telescope, covering 30--50 GHz with a receiver noise temperature of about 15 K. We nam…

Q-band Line Survey Observations toward a Carbon-chain-rich Clump in the Serpens South Region

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

An ultra wide-band, high-sensitivity Q-band receiver for single-dish telescopes, eQ: rest frequency determination of CCS ( $J_{N}$ = $4_{3}$ - $3_{2}$ ) and SO ( $J_{N}$ = $1_{0}$ - $0_{1}$ ), and high-redshift CO ( $J$ = 1-0) detection