activity
20132026
most citedSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6

224 citations · 4.1k across the 113 of their papers we have counts for

collaborators
Showing 2018Show all

9 papers · 1 filter

astro-ph.GA2018★ 27 cited

Kinetic energy transfer from X-ray ultrafast outflows to mm/sub-mm cold molecular outflows in Seyfert galaxies

Misaki Mizumoto, Takuma Izumi, Kotaro Kohno

UltraFast Outflows (UFOs), seen as X-ray blueshifted absorption lines in active galactic nuclei (AGNs), are considered to be a key mechanism for AGN feedback. In this scenario, UFO…

astro-ph.GA2018★ 224 cited

Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6

Yoshiki Matsuoka, Michael A. Strauss, Nobunari Kashikawa +44

We present new measurements of the quasar luminosity function (LF) at , over an unprecedentedly wide range of the rest-frame ultraviolet luminosity from …

astro-ph.GA2018★ 108 cited

Circumnuclear Multi-phase Gas in the Circinus Galaxy II: The Molecular and Atomic Obscuring Structures Revealed with ALMA

Takuma Izumi, Keiichi Wada, Ryosuke Fukushige +2

We used the Atacama Large Millimeter/Submillimeter Array (ALMA) to map the CO(3-2) and [CI](1-0) lines, as well as their underlying continuum emission, from the central …

astro-ph.GA2018★ 103 cited

A gravitationally unstable gas disk of a starburst galaxy 12 billion years ago

Ken-ichi Tadaki, Daisuke Iono, Min S. Yun +18

Submillimeter bright galaxies in the early Universe are vigorously forming stars at ~1000 times higher rate than the Milky Way. A large fraction of stars is formed in the central 1…

astro-ph.GA2018★ 3 cited

Supermassive black holes with higher Eddington ratios preferentially form in gas-rich galaxies

Takuma Izumi

The Eddington ratio () of supermassive black holes (SMBHs) is a fundamental parameter that governs the cosmic growth of SMBHs. Although gas mass accretion onto SMBHs i…

astro-ph.GA2018★ 37 cited

ALMA Multiple-Transition Observations of High Density Molecular Tracers in Ultraluminous Infrared Galaxies

Masatoshi Imanishi, Kouichiro Nakanishi, Takuma Izumi

We present the results of our ALMA observations of eleven (ultra)luminous infrared galaxies ((U)LIRGs) at J=4-3 of HCN, HCO+, HNC and J=3-2 of HNC. This is an extension of our prev…

astro-ph.GA2018★ 132 cited

Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). IV. Discovery of 41 Quasars and Luminous Galaxies at 5.7 < z < 6.9

Y. Matsuoka, K. Iwasawa, M. Onoue +44

We report discovery of 41 new high-z quasars and luminous galaxies, which were spectroscopically identified at 5.7 < z < 6.9. This is the fourth in a series of papers from the Suba…

astro-ph.GA2018★ 76 cited

Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at studied with ALMA

Takuma Izumi, Masafusa Onoue, Hikari Shirakata +26

We present our ALMA Cycle 4 measurements of the [CII] emission line and the underlying far-infrared (FIR) continuum emission from four optically low-luminosity ($M_{\rm 1450} > -25…

astro-ph.GA2018★ 128 cited

ALMA Reveals an Inhomogeneous Compact Rotating Dense Molecular Torus at the NGC 1068 Nucleus

Masatoshi Imanishi, Kouichiro Nakanishi, Takuma Izumi +1

We present the results of our ALMA Cycle 4 high-spatial-resolution (0.04-0.07") observations, at HCN J=3-2 and HCO+ J=3-2 lines, of the nucleus of NGC 1068, the nearby prototypical…