activity
20052020
most citedHigh-Mass Cloud Cores in the eta Carinae Giant Molecular Cloud

96 citations · 321 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2020★ 11 cited

Observations of the [CI] (-) emission toward the massive star-forming region RCW38: further evidence for highly-clumped density distribution of the molecular gas

Natsuko Izumi, Yasuo Fukui, Kengo Tachihara +14

We present observations of the - fine-structure line of atomic carbon using the ASTE 10 m sub-mm telescope towards RCW38, the youngest super star cluster in the Milky…

astro-ph.IM2020★ 6 cited

Waveguide-Type Multiplexer for Multiline Observation of Atmospheric Molecules using Millimeter-Wave Spectroradiometer

Taku Nakajima, Kohei Haratani, Akira Mizuno +5

In order to better understand the variation mechanism of ozone abundance in the middle atmosphere, the simultaneous monitoring of ozone and other minor molecular species, which are…

astro-ph.IM2020★ 13 cited

DESHIMA on ASTE: On-sky Responsivity Calibration of the Integrated Superconducting Spectrometer

Tatsuya Takekoshi, Kenichi Karatsu, Junya Suzuki +36

We are developing an ultra-wideband spectroscopic instrument, DESHIMA (DEep Spectroscopic HIgh-redshift MApper), based on the technologies of an on-chip filter-bank and Microwave K…

astro-ph.IM2019★ 49 cited

First light demonstration of the integrated superconducting spectrometer

Akira Endo, Kenichi Karatsu, Yoichi Tamura +36

Ultra-wideband 3D imaging spectrometry in the millimeter-submillimeter (mm-submm) band is an essential tool for uncovering the dust-enshrouded portion of the cosmic history of star…

astro-ph.IM2018

Planar Superconductor-Insulator-Superconductor Mixer Array Receivers for Wide Field of View Astronomical Observation

Wenlei Shan, Shohei Ezaki, Jie Liu +3

We present a conceptual framework of planar SIS mixer array receivers and the studies on the required techniques. This concept features membrane-based on-chip waveguide probes and…

astro-ph.SR2016★ 21 cited

The Brightness Temperature of the Quiet Solar Chromosphere at 2.6 mm

Kazumasa Iwai, Masumi Shimojo, Shinichiro Asayama +4

The absolute brightness temperature of the Sun at millimeter wavelengths is an important diagnostic of the solar chromosphere. Because the Sun is so bright, measurement of this pro…

astro-ph.IM2016★ 8 cited

The Atacama Large Millimeter/submillimeter Array (ALMA) Band-1 Receiver

Yau De Huang, Oscar Morata, Patrick Michel Koch +29

The Atacama Large Millimeter/submillimeter Array(ALMA) Band 1 receiver covers the 35-50 GHz frequency band. Development of prototype receivers, including the key components and sub…

astro-ph.IM2013★ 45 cited

A New 100-GHz Band Two-Beam Sideband-Separating SIS Receiver for Z-Machine on the NRO 45-m Radio Telescope

Taku Nakajima, Kimihiro Kimura, Atsushi Nishimura +11

We have developed a two-beam waveguide-type dual-polarization sideband-separating SIS receiver system in the 100-GHz band for {\it z}-machine on the 45-m radio telescope at the Nob…

astro-ph2008★ 49 cited

A New 100-GHz Band Front-End System with a Waveguide-Type Dual-Polarization Sideband-Separating SIS Receiver for the NRO 45-m Radio Telescope

Taku Nakajima, Masayuki Kawamura, Kimihiro Kimura +8

We developed a waveguide-type dual-polarization sideband-separating SIS receiver system of the 100-GHz band for the 45-m radio telescope at the Nobeyama Radio Observatory, Japan. T…

astro-ph2007★ 23 cited

New 60-cm Radio Survey Telescope with the Sideband-Separating SIS Receiver for the 200 GHz Band

Taku Nakajima, Masahiro Kaiden, Jun Korogi +10

We have upgraded the 60-cm radio survey telescope located in Nobeyama, Japan. We developed a new waveguide-type sideband-separating SIS mixer for the telescope, which enables the s…

astro-ph2005★ 96 cited

High-Mass Cloud Cores in the eta Carinae Giant Molecular Cloud

Y. Yonekura, S. Asayama, K. Kimura +5

We carried out an unbiased survey for massive dense cores in the giant molecular cloud associated with eta Carinae with the NANTEN telescope in 12CO, 13CO, and C18O 1-0 emission li…