activity
20042026
most citedA New 100-GHz Band Two-Beam Sideband-Separating SIS Receiver for Z-Machine on the NRO 45-m Radio Telescope

45 citations · 227 across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.GA2026

Suppression of star formation at the centre of barred AGN galaxies

Takashi Yamamoto, Nario Kuno, Daisuke Iono +5

We measured the Concentration (C) index of Hαand CO (J = 2-1) in 17 nearby star-forming galaxies from the PHANGS survey. We have found four barred spiral galaxies with a C(Hα)/C(CO…

astro-ph.GA2026

A New Framework for Multi-Line Analysis Combined Kernel PCA and Kernel SHAP: A Case of NGC 1068 ALMA Band 3 Data

Hiroma Okubo, Tsutomu T. Takeuchi, Shotaro Akaho +7

We present a new framework for multi-line analysis that combines kernel principal component analysis (Kernel PCA), an unsupervised machine-learning method, and Kernel SHapley Addit…

astro-ph.GA2025

CO Multi-line Imaging of Nearby Galaxies (COMING). XI. Azimuthally averaged star formation rate and stellar mass relation with molecular gas amount

Ayumi Kajikawa, Kazuo Sorai, Kana Morokuma-Matsui +13

This study investigated the relation between the surface density of star formation rate (SFR) (), stellar mass (), and molecular gas mass ($Σ_{M_\ma…

astro-ph.GA2025

Detailed analysis of multi-line molecular distributions in the Seyfert galaxy NGC 1068: Possible effect of the AGN outflow to the starburst ring

Hiroma Okubo, Toshiki Saito, Shuro Takano +5

We apply principal component analysis (PCA) to the integrated intensity maps of 13 molecular lines of the nearby type-2 Seyfert galaxy NGC 1068 obtained by Atacama Large Millimeter…

astro-ph.GA2024

Whole-disk sampling of molecular clouds in M83

Akihiko Hirota, Jin Koda, Fumi Egusa +17

We present a catalog of clouds identified from the CO (1--0) data of M83, which was observed using Atacama Large Millimeter/submillimeter Array (ALMA) with a spatial resolut…

astro-ph.GA2024★ 8 cited

Detection of the [O I] 63 m emission line from the quasar J2054-0005

Nozomi Ishii, Takuya Hashimoto, Carl Ferkinhoff +23

We report the highest-redshift detection of [O I] 63 m from a luminous quasar, J2054-0005, at based on the Atacama Large Millimeter/sub-millimeter Array Band 9 observat…

astro-ph.GA2024★ 4 cited

ACA CO(J=2-1) Mapping of the Nearest Spiral Galaxy M33. II. Exploring the Evolution of Giant Molecular Clouds

Ayu Konishi, Kazuyuki Muraoka, Kazuki Tokuda +12

The evolution of giant molecular clouds (GMCs), the main sites of high-mass star formation, is an essential process to unravel the galaxy evolution. Using a GMC catalogue of M33 fr…

astro-ph.GA2024★ 2 cited

Quantitative analysis of the molecular gas morphology in nearby disk galaxies

Takashi Yamamoto, Daisuke Iono, Toshiki Saito +4

We present a quantitative and statistical analysis of the molecular gas morphology in 73 nearby galaxies using high spatial resolution CO ( = 2-1) data obtained from the Atacama…

astro-ph.GA2017★ 30 cited

Discovery of molecular and atomic clouds associated with the gamma-ray supernova remnant Kesteven 79

M. Kuriki, H. Sano, N. Kuno +21

We carried out CO( = 1-0) observations of the Galactic gamma-ray supernova remnant (SNR) Kesteven 79 using the Nobeyama Radio Observatory 45 m radio telescope, which has…

astro-ph.GA2014★ 9 cited

Molecular gas and nuclear activity in early-type galaxies: any link with radio-loudness?

Ranieri D. Baldi, Marcello Giroletti, Alessandro Capetti +4

Aims. We want to study the amount of molecular gas in a sample of nearby early-type galaxies (ETGs) which host low-luminosity Active Galactic Nuclei (AGN). We look for possible dif…

astro-ph.GA2014★ 2 cited

A multiwavelength analysis of the clumpy FIR-bright sources in M33

G. Natale, K. Foyle, C. D. Wilson +1

We present a multiwavelength study of a sample of far-infrared (FIR) sources detected on the Herschel broad--band maps of the nearby galaxy M33. We perform source photometry on the…

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-ph.CO2012★ 18 cited

Initial Results from the Nobeyama Molecular Gas Observations of Distant Bright Galaxies

D. Iono, B. Hatsukade, K. Kohno +37

We present initial results from the CO survey toward high redshift galaxies using the Nobeyama 45m telescope. Using the new wide bandwidth spectrometer equipped with a two-beam SIS…

astro-ph.IM2012★ 20 cited

Optimization by Smoothed Bandpass Calibration in Radio Spectroscopy

Haruka Yamaki, Seiji Kameno, Hirohisa Beppu +2

We have developed the Smoothed Bandpass Calibration (SBC) method and the best suitable scan pattern to optimize radio spectroscopic observations. Adequate spectral smoothing is app…

astro-ph.SR2010★ 19 cited

SiO Maser Spectra of V407 Cyg after the 2010 March Nova Outburst

S. Deguchi, K. Koike, N. Kuno +3

We report on the time variation of SiO maser emission from the symbiotic stellar system V407 Cyg after the classical nova outburst on 2010 March 10. Although both the SiO --0…

astro-ph2008★ 5 cited

ASTE CO(3--2) Observations of the Southern Barred Spiral Galaxy NGC 986: a Large Gaseous Bar Filled with Dense Molecular Medium

K. Kohno, T. Tosaki, R. Miura +20

We present CO(3-2) emission observations toward the 3'x3' (or 20x20kpc at a distance of 23Mpc) region of the southern barred spiral galaxy NGC 986 using the Atacama Submillimeter T…

astro-ph2007★ 19 cited

A Revised Estimate of the CO (J=1-0) Emission from the Host Galaxy of GRB 030329 Using the Nobeyama Millimeter Array

Akira Endo, Kotaro Kohno, Bunyo Hatsukade +9

A sensitive observation of the CO (J=1-0) molecular line emission in the host galaxy of GRB 030329 (z =0.1685) has been performed using the Nobeyama Millimeter Array in order to de…

astro-ph2004★ 27 cited

Nobeyama Millimeter Array Observations of GRB 030329: a Decay of Afterglow with Bumps and Molecular Gas in the Host Galaxy

K. Kohno, T. Tosaki, T. Okuda +12

Nobeyama Millimeter Array was used to observe millimeter-wave afterglow of GRB 030329 at 93 GHz and 141 GHz from 2003 April 6 to 2003 May 30. A sensitive search for CO(J=1-0) emiss…

astro-ph2004★ 19 cited

Study of the Bipolar Nebula IRAS 19312+1950. I. Mapping Observations

J. Nakashima, S. Deguchi, N. Kuno

IRAS 19312+1950 is an SiO maser source that exhibits a prominent bipolar nebulosity. Mapping observations of this object were made in the CO J=1--0, 13CO J=1--0, C18O J=1--0, CS J=…