activity
20132026
most citedAn isolated mass gap black hole or neutron star detected with astrometric microlensing

140 citations · 899 across the 43 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

29 papers · 1 filter

astro-ph.GA2026

Absolute Motion of the Infrared Counterpart to Sagittarius A* in the Gaia Celestial Reference Frame 3 and Limits on an Intermediate-mass Black Hole Companion

Rebecca A. Lewis-Merrill, Tuan Do, Matthew W. Hosek +9

We report the first proper motion and acceleration measurements of the infrared (IR) counterpart to Sagittarius A* (Sgr A*-IR), the supermassive black hole (SMBH) at the center of…

astro-ph.GA2026

A Kinematic Study of Wolf-Rayet Stars at the Galactic Center I: Binary Candidates and Constraints on the Binary Fraction

Rory O. Bentley, Tuan Do, Andrea Ghez +13

We report the binary fraction of Wolf-Rayet (WR) stars within 0.5~pc of the Galactic center obtained through the longest time-baseline (1994-2024) kinematic study of this populatio…

astro-ph.GA2026

IRS 9: The Case for a Dynamically-Ejected Star from the Galactic Center

Matthew Hosek, Tuan Do, Smadar Naoz +7

Measuring stellar motions at the Milky Way's Galactic center (GC) provides unique insight into the dynamical processes within galactic nuclei. We present proper motion measurements…

astro-ph.GA2025

The HST-Gaia Near-Infrared Astrometric Reference Frame near the Milky Way Galactic Center

Matthew W. Hosek, Tuan Do, Gregory D. Martinez +5

We present the first high-precision proper motion catalog, tied to the International Celestial Reference System (ICRS), of infrared astrometric reference stars within R 25"…

astro-ph.GA2025★ 1 cited

Structure and Dynamics of the Young Massive Star Cluster Westerlund 1

Lingfeng Wei, Matthew W. Hosek, Jessica R. Lu +8

We present a structural analysis of the young massive star cluster Westerlund 1 (Wd 1). With multi-epoch Hubble Space Telescope (HST) observations, we measure the proper motions of…

astro-ph.GA2024★ 4 cited

The Galactic Center in Color: Measuring Extinction with High-Proper-Motion Stars

Z. Haggard, A. M. Ghez, S. Sakai +6

The Milky Way's central parsec is a highly extinguished region with a population of high-proper-motion stars. We have tracked 145 stars for 10 years at wavelengths between 1…

astro-ph.GA2024

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

Abhimat K. Gautam, Tuan Do, Andrea M. Ghez +8

We present the first estimate of the intrinsic binary fraction of young stars across the central 0.4 pc surrounding the supermassive black hole (SMBH) at the Milky Way Ga…

astro-ph.GA2023★ 6 cited

The JWST Galactic Center Survey -- A White Paper

Rainer Schoedel, Steve Longmore, Jonny Henshaw +111

The inner hundred parsecs of the Milky Way hosts the nearest supermassive black hole, largest reservoir of dense gas, greatest stellar density, hundreds of massive main and post ma…

astro-ph.GA2023

Co-moving groups around massive stars in the Nuclear Stellar Disk

Á. Martínez-Arranz, R. Schödel, F. Nogueras-Lara +2

During the last 30 Myr the nuclear stellar disk in the Galactic center has been the most prolific star forming region of the Milky Way when averaged by volume. Remarkably, t…

astro-ph.GA2023

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

Grant C. Weldon, Tuan Do, Gunther Witzel +10

Sgr A* is the variable electromagnetic source associated with accretion onto the Galactic center supermassive black hole. While the near-infrared (NIR) variability of Sgr A* was sh…

astro-ph.GA2023★ 19 cited

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

R. Schoedel, F. Nogueras-Lara, M. Hosek +9

Until recently it was thought that the nuclear stellar disc at the centre of our Galaxy was formed via quasi-continuous star formation over billions of years. However, an analysis…

astro-ph.GA2023★ 20 cited

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

Devin S. Chu, Tuan Do, Andrea Ghez +12

We present the results of the first systematic search for spectroscopic binaries within the central 2 x 3 arcsec around the supermassive black hole at the center of the Milky W…

astro-ph.GA2023★ 20 cited

Stellar Populations in the Central 0.5 pc of Our Galaxy III: The Dynamical Sub-structures

Siyao Jia, Ningyuan Xu, Jessica R. Lu +12

We measure the 3D kinematic structures of the young stars within the central 0.5 parsec of our Galactic Center using the 10 m telescopes of the W.~M.~Keck Observatory over a time s…

astro-ph.GA2022★ 42 cited

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

Zhuo Chen, Tuan Do, Andrea M. Ghez +6

We report the first star formation history study of the Milky Way's nuclear star cluster (NSC) that includes observational constraints from a large sample of stellar metallicity me…

astro-ph.GA2022★ 15 cited

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

Matthew W. Hosek, Tuan Do, Jessica R. Lu +4

We present new absolute proper motion measurements for the Arches and Quintuplet clusters, two young massive star clusters near the Galactic center. Using multi-epoch HST observati…

astro-ph.GA2022★ 140 cited

An isolated mass gap black hole or neutron star detected with astrometric microlensing

Casey Y. Lam, Jessica R. Lu, Andrzej Udalski +42

We present the analysis of five black hole candidates identified from gravitational microlensing surveys. Hubble Space Telescope astrometric data and densely sampled lightcurves fr…

astro-ph.GA2019★ 18 cited

Consistency of the Infrared Variability of Sgr A* over 22 years

Zhuo Chen, E. Gallego-Cano, T. Do +14

We report new infrared measurements of the supermassive black hole at the Galactic Center, Sgr A*, over a decade that was previously inaccessible at these wavelengths. This enables…

astro-ph.GA2019★ 97 cited

Unprecedented variability of Sgr A* in NIR

Tuan Do, Gunther Witzel, Abhimat K. Gautam +10

The electromagnetic counterpart to the Galactic center supermassive black hole, Sgr A*, has been observed in the near-infrared for over 20 years and is known to be highly variable.…

astro-ph.GA2019★ 1 cited

Astro2020 Science White Paper: Local Dwarf Galaxy Archaeology

Alexander P. Ji, Rachel Beaton, Sukanya Chakrabarti +8

Nearby dwarf galaxies are local analogues of high-redshift and metal-poor stellar populations. Most of these systems ceased star formation long ago, but they retain signatures of t…

astro-ph.GA2019★ 3 cited

Astro2020 Science White Paper: The Local Relics of of Supermassive Black Hole Seeds

Jenny E Greene, Aaron Barth, Andrea Bellini +18

We have compelling evidence for stellar-mass black holes (BHs) of ~5-80 M_sun that form through the death of massive stars. We also have compelling evidence for so-called supermass…

astro-ph.GA2019★ 9 cited

Envisioning the next decade of Galactic Center science: a laboratory for the study of the physics and astrophysics of supermassive black holes

Tuan Do, Andrea Ghez, Jessica R. Lu +38

As the closest example of a galactic nucleus, the Galactic center (GC) presents an exquisite laboratory for learning about supermassive black holes (SMBH) and their environment. We…

astro-ph.GA2019★ 1 cited

Star Formation in Different Environments: The Initial Mass Function

M. W. Hosek, J. R. Lu, M. Andersen +7

The stellar initial mass function (IMF) is a fundamental property of star formation, offering key insight into the physics driving the process as well as informing our understandin…

astro-ph.GA2019★ 33 cited

The Galactic Center: Improved Relative Astrometry for Velocities, Accelerations, and Orbits near the Supermassive Black Hole

Siyao Jia, Jessica R. Lu, S . Sakai +11

We present improved relative astrometry for stars within the central half parsec of our Galactic Center based on data obtained with the 10 m W. M. Keck Observatory from 1995 to 201…

astro-ph.GA2019★ 34 cited

The Galactic Center: An Improved Astrometric Reference Frame for Stellar Orbits around the Supermassive Black Hole

Shoko Sakai, Jessica R. Lu, Andrea Ghez +8

Precision measurements of the stars in short-period orbits around the supermassive black hole at the Galactic Center are now being used to constrain general relativistic effects, s…