Tuan Do

Assistant Professor

UCLA Division of Physical Sciences

United States

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About

Dr. Tuan Do is an Assistant Professor at UCLA Division of Physical Sciences, USA. His research focuses on near-infrared astrometry and cosmology, with recent articles exploring the characteristics of the Galactic Center, including the flux distribution of Sgr A* and techniques for photometric redshift estimation. He is also involved in the study of binary star fractions among young stars and the application of Bayesian neural networks in astronomy.

Articles (19)

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2025

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2024

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2022

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2022

Collaborators (10)

Ken Shen

University of California

UNITED STATES

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Mark Gurwell

Smithsonian Institution

UNITED STATES

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Jack Singal

Associate Professor

University of Richmond

UNITED STATES

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Wolfgang Kerzendorf

Assistant Professor

Michigan State University

UNITED STATES

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Jessica Lu

University of California, Berkeley

UNITED STATES

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Michael Fitzgerald

Associate Professor

University of California, Los Angeles

UNITED STATES

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Robert Rich

Research Astronomer/Adjunct Professor

UCLA Division of Physical Sciences

UNITED STATES

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Andrea Ghez

Distinguished Professor

University of California, Los Angeles

UNITED STATES

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angela gardini

Instituto de Astrofísica de Andalucía

SPAIN

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Mark Morris

Distinguished Research Professor Emeritus

University of California, Los Angeles

UNITED STATES

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Tuan Do

Research Interests

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About

Articles (19)

The HST–Gaia Near-infrared Astrometric Reference Frame Near the Milky Way Galactic Center

The Galactic Center in Color: Measuring Extinction with High-proper-motion Stars

Orbital and Atmospheric Characterization of the 1RXS J034231.8+121622 System using High-resolution Spectroscopy Confirms that the Companion is a Low-mass Star

An Estimate of the Binary Star Fraction among Young Stars at the Galactic Center: Possible Evidence of a Radial Dependence

Improving Photometric Redshift Estimation for Cosmology with LSST Using Bayesian Neural Networks

High-resolution, Mid-infrared Color Temperature Mapping of the Central 10″ of the Galaxy

Redshift Prediction with Images for Cosmology Using a Bayesian Convolutional Neural Network with Conformal Predictions

New Evidence for a Flux-independent Spectral Index of Sgr A* in the Near-infrared

Near-infrared Flux Distribution of Sgr A* from 2005–2022: Evidence for an Enhanced Accretion Episode in 2019

The Orbital Eccentricities of Directly Imaged Companions Using Observable-based Priors: Implications for Population-level Distributions

Evidence of a Decreased Binary Fraction for Massive Stars within 20 milliparsecs of the Supermassive Black Hole at the Galactic Center

Stellar Populations in the Central 0.5 pc of Our Galaxy. III. The Dynamical Substructures

The formation history of our Galaxy’s nuclear stellar disc constrained from HST observations of the Quintuplet field

The Star Formation History of the Milky Way’s Nuclear Star Cluster

The Swansong of the Galactic Center Source X7: An Extreme Example of Tidal Evolution near the Supermassive Black Hole

Constraining a Companion of the Galactic Center Black Hole Sgr A*

Multiwavelength Variability of Sagittarius A* in 2019 July

Measuring the Orbits of the Arches and Quintuplet Clusters Using HST and Gaia: Exploring Scenarios for Star Formation near the Galactic Center

Searching for a Hypervelocity White Dwarf SN Ia Companion: A Proper-motion Survey of SN 1006

Collaborators (10)

Ken Shen

Mark Gurwell

Jack Singal

Wolfgang Kerzendorf

Jessica Lu

Michael Fitzgerald

Robert Rich

Andrea Ghez

angela gardini

Mark Morris

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