Tuan Do
astro.ucla.edu
0000-0001-9554-6062
UCLA Division of Physical Sciences
43 papers found
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DETECTION OF GALACTIC CENTER SOURCE G2 AT 3.8 μm DURING PERIAPSE PASSAGE
Prospects for Measuring Supermassive Black Hole Masses With Future Extremely Large Telescopes
Efficiency Measurements and Installation of a New Grating for the OSIRIS Spectrograph at Keck Observatory
A Reconnaissance of the Possible Donor Stars to the Kepler Supernova
Properties of the remnant clockwise disk of young stars in the galactic center
Three-Dimensional Stellar Kinematics at the Galactic Center: Measuring the Nuclear Star Cluster Spatial Density Profile, Black Hole Mass, and Distance
Keck Observations of the Galactic Center Source G2: Gas Cloud or Star?
Stellar populations in the central 0.5 pc of the galaxy. II. The initial mass function
Stellar Populations in the Central 0.5 pc of the Galaxy. I. A New Method for Constructing Luminosity Functions and Surface-density Profiles
Proper motions of the arches cluster with Keck laser guide star adaptive optics: The first kinematic mass measurement of the arches
The Shortest-Known--Period Star Orbiting Our Galaxy’s Supermassive Black Hole
Measuring the stellar luminosity function and spatial density profile of the inner 0.5 pc of the Milky Way nuclear star cluster
Improving Galactic Center Astrometry by Reducing the Effects of Geometric Distortion
Physical Processes in the Vicinity of a Supermassive Black Hole
Disks in the Arches Cluster—survival in a Starburst Environment
A power-law break in the near-infrared power spectrum of the Galactic center black hole
A near-infrared variability study of the galactic black hole: a red noise source with NO detected periodicity
High angular resolution integral-field spectroscopy of the galaxy's nuclear cluster: a missing stellar cusp?
A 600 Minute Near-Infrared Light Curve of Sagittarius A
Measuring distance and properties of the Milky Way’s central supermassive black hole with stellar orbits
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