John Silverman

Professor

Kavli Institute for the Physics and Mathematics of the Universe

Japan

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About

John Silverman is a Professor at the Kavli Institute for the Physics and Mathematics of the Universe in Japan. His research focuses on the formation and evolution of massive galaxies and black holes, particularly in the early universe with a redshift greater than 6. Recent publications include studies on quasar host galaxies, dark matter content, and multiwavelength investigations of galaxy structures utilizing the James Webb Space Telescope.

Articles (20)

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2025

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2021

Collaborators (30)

Yousuke Utsumi

准教授/Associate Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

JAPAN

John Silverman

Research Interests

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About

Articles (20)

SHELLQs. Bridging the Gap: JWST Unveils Obscured Quasars in the Most Luminous Galaxies at z > 6

A post-starburst pathway for the formation of massive galaxies and black holes at z > 6

Assessing the Dark Matter Content of Two Quasar Host Galaxies at z ∼ 6 through Gas Kinematics

Tip of the Iceberg: Overmassive Black Holes at 4 < z < 7 Found by JWST Are Not Inconsistent with the Local M BH - M ⋆ Relation

The MBH–M∗ Relation up to z ∼ 2 through Decomposition of COSMOS-Web NIRCam Images

A Multiwavelength Investigation of Spiral Structures in z > 1 Galaxies with JWST

Merging Gas-rich Galaxies That Harbor Low-luminosity Twin Quasars at z = 6.05: A Promising Progenitor of the Most Luminous Quasars

Crimson Behemoth: A massive clumpy structure hosting a dusty AGN at z=4.91

Prior-informed Active Galactic Nucleus Host Spectral Decomposition Using PyQSOFit

Dark Matter Halos of Luminous Active Galactic Nuclei from Galaxy–Galaxy Lensing with the HSC Subaru Strategic Program

Quasar Luminosity Function at z = 7

Resolving Galactic-scale Obscuration of X-Ray AGNs at z ≳ 1 with COSMOS-Web

A Machine-learning Approach to Assessing the Presence of Substructure in Quasar-host Galaxies Using the Hyper Suprime-cam Subaru Strategic Program

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 &lt; z &lt; 7.0

Concordance between Observations and Simulations in the Evolution of the Mass Relation between Supermassive Black Holes and Their Host Galaxies

The Stellar Mass versus Stellar Metallicity Relation of Star-forming Galaxies at 1.6 ≤ z ≤ 3.0 and Implications for the Evolution of the α-enhancement

Opening the Era of Quasar-host Studies at High Redshift with JWST

Inferences on Relations between Distant Supermassive Black Holes and Their Hosts Complemented by the Galaxy Fundamental Plane

Hyper Suprime-Cam Subaru Strategic Program: A Mass-dependent Slope of the Galaxy Size−Mass Relation at z < 1

Synchronized Coevolution between Supermassive Black Holes and Galaxies over the Last Seven Billion Years as Revealed by Hyper Suprime-Cam

Collaborators (30)

Yousuke Utsumi

Georgios Magdis

Simon Lilly

Yutaka Komiyama

Tadafumi Takata

Shu Wang

Takuma Izumi

Hiroyuki Ikeda

Y Fudamoto

Tilman Hartwig

Yohan Dubois

Yoshiki Matsuoka

Michele Ginolfi

Masayuki Akiyama

Ivana Damjanov

Emanuele Daddi

Kotaro Kohno

Tiziana DiMatteo

Takumi S Tanaka

Shuowen Jin

Kazushi Iwasawa

Hideki Umehata

Steven Gillman

Daichi Kashino

Tohru Nagao

Satoshi Kikuta

Si-Yue Yu

Masafusa Onoue

Michael Strauss

Masatoshi Imanishi

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Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0