activity
20222024
most citedA Lower Bound of Star Formation Activity in Ultra-high Redshift Galaxies Detected with JWST: Implications for Stellar Populations and Radiation Sources

127 citations · 348 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2024★ 23 cited

The Rise of Faint, Red AGN at : A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields

Dale D. Kocevski, Steven L. Finkelstein, Guillermo Barro +54

We present a sample of 341 "little red dots" (LRDs) spanning the redshift range using data from the CEERS, PRIMER, JADES, UNCOVER and NGDEEP surveys. Unlike past use of…

astro-ph.GA2023

Exploring Low-Mass Black Holes through Tidal Disruption Events in the Early Universe: Perspectives in the Era of JWST, RST, and LSST Surveys

Kohei Inayoshi, Kazumi Kashiyama, Wenxiu Li +3

The James Webb Space Telescope (JWST) has recently uncovered the presence of low-luminosity active galactic nuclei (AGNs) at . Spectroscopic observations have provided esti…

astro-ph.GA2023

Reconstruction of Cosmic Black Hole Growth and Mass Distribution from Quasar Luminosity Functions at : Implications for Faint and Low-mass Populations in JWST

Wenxiu Li, Kohei Inayoshi, Masafusa Onoue +6

The evolution of the quasar luminosity function (QLF) is fundamental to understanding the cosmic evolution of black holes (BHs) through their accretion phases. In the era of the Ja…

astro-ph.GA2023★ 24 cited

Hidden Little Monsters: Spectroscopic Identification of Low-Mass, Broad-Line AGN at with CEERS

Dale D. Kocevski, Masafusa Onoue, Kohei Inayoshi +34

We report on the discovery of two low-luminosity, broad-line AGN at identified using JWST NIRSpec spectroscopy from the CEERS Survey. We detect broad H emission from both…

astro-ph.GA2022★ 22 cited

The Assembly of Black Hole Mass and Luminosity Functions of High-redshift Quasars via Multiple Accretion Episodes

Wenxiu Li, Kohei Inayoshi, Masafusa Onoue +1

The early evolution of the quasar luminosity function (QLF) and black hole mass function (BHMF) encodes key information on the physics determining the radiative and accretion proce…

astro-ph.GA2022★ 127 cited

A Lower Bound of Star Formation Activity in Ultra-high Redshift Galaxies Detected with JWST: Implications for Stellar Populations and Radiation Sources

Kohei Inayoshi, Yuichi Harikane, Akio K. Inoue +2

Early results of JWST observations have delivered bright galaxy candidates in greater numbers than expected, enabling construction of the rest-frame UV luminosity fun…

astro-ph.GA2022★ 116 cited

A Candidate of a Least-Massive Black Hole at the First 1.1 Billion Years of the Universe

Masafusa Onoue, Kohei Inayoshi, Xuheng Ding +6

We report a candidate of a low-luminosity active galactic nucleus (AGN) at z=5 that was selected from the first near-infrared images of the JWST CEERS project. This source, named C…

astro-ph.GA2022

Radiative feedback on supermassive star formation: the massive end of the Population III initial mass function

Daisuke Toyouchi, Kohei Inayoshi, Wenxiu Li +2

Supermassive stars (SMSs) with masses of -- are invoked as possible seeds of high-redshift supermassive black holes, but it remains under de…

astro-ph.GA2022★ 36 cited

Supercritical growth pathway to overmassive black holes at cosmic dawn: coevolution with massive quasar hosts

Haojie Hu, Kohei Inayoshi, Zoltán Haiman +3

Observations of the most luminous quasars at high redshifts () have revealed that the largest supermassive black holes (SMBHs) at those epochs tend to be substantially overm…