Michael Strauss

Professor, Associate Chair

Princeton University

United States

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About

Michael Strauss is a Professor and Associate Chair at Princeton University in the United States. His research areas include the origins of fast radio bursts, the formation of massive galaxies and black holes at high redshifts, and the characteristics of quasars in the early universe. He has contributed to several recent articles focusing on stellar mass distributions, quasar-galaxy mergers, and machine learning applications in astrophysics.

Articles (24)

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2021

Collaborators (40)

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

Michael Strauss

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Articles (24)

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

Unveiling the Origin of Fast Radio Bursts by Modeling the Stellar Mass and Star Formation Distributions of Their Host Galaxies

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

No Galaxy-scale [C ii] Fast Outflow in the z = 6.72 Red Quasar HSC J1205–0000

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XXI. Candidate Red Quasars at z ≥ 6 from Near-infrared Photometry

Euclid preparation

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

Discovery of Merging Twin Quasars at z = 6.05

A quasar-galaxy merger at z ∼ 6.2: Rapid host growth via the accretion of two massive satellite galaxies

A quasar-galaxy merger at z ∼ 6.2: Black hole mass and quasar properties from the NIRSpec spectrum

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVII. Black Hole Mass Distribution at z ∼ 6 Estimated via Spectral Comparison with Low-z Quasars

Cross-correlation of Luminous Red Galaxies with Machine Learning Selected Active Galactic Nuclei in HSC-SSP: Unobscured AGN Residing in More Massive Halos

Quasar Luminosity Function at z = 7

Detection of stellar light from quasar host galaxies at redshifts above 6

A general framework for removing point-spread function additive systematics in cosmological weak lensing analysis

Are Brightest Cluster Galaxies Special?

Hyper Suprime-Cam Year 3 results: Cosmology from cosmic shear power spectra

Hyper Suprime-Cam Year 3 results: Cosmology from cosmic shear two-point correlation functions

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

Optimization of the Observing Cadence for the Rubin Observatory Legacy Survey of Space and Time: A Pioneering Process of Community-focused Experimental Design

The interstellar medium distribution, gas kinematics, and system dynamics of the far-infrared luminous quasar SDSS J2310+1855 at z = 6.0

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

Optical Spectroscopy of Dual Quasar Candidates from the Subaru HSC-SSP program

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XIV. A Candidate Type II Quasar at z = 6.1292

Collaborators (40)

Yousuke Utsumi

Richard Arendt

Federica B. Bianco

Surhud More

Yutaka Komiyama

Joel Leja

Tadafumi Takata

Takuma Izumi

Melanie Habouzit

Issha Kayo

Hiroyuki Ikeda

Ken Osato

Shunsuke Baba

Markus Michael Rau

Yoshiki Matsuoka

Masayuki Akiyama

Takuya Hashimoto

Gabriele Mainetti

Ryo Terasawa

Fernando Atrio-Barandela

Kotaro Kohno

Rachel Mandelbaum

Andrew Connolly

Hironao Miyatake

Nobunari Kashikawa

John Silverman

Tianqing Zhang

Renee Hlozek

Kazushi Iwasawa

Hiranya Peiris

Arun Kannawadi

Hideki Umehata

Bram Venemans

Zeljko Ivezic

Tohru Nagao

Satoshi Kikuta

Alessandro Lupi

Masafusa Onoue

Marianne Vestergaard

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