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 2019Show all

10 papers · 1 filter

astro-ph.SR2019★ 55 cited

PopSyCLE: A New Population Synthesis Code for Compact Object Microlensing Events

Casey Y. Lam, Jessica R. Lu, Matthew W. Hosek +2

We present a new Milky Way microlensing simulation code, dubbed PopSyCLE (Population Synthesis for Compact object Lensing Events). PopSyCLE is the first resolved microlensing simul…

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.SR2019★ 25 cited

The Quintuplet Cluster: Extended Structure and Tidal Radius

Nicholas Z. Rui, Matthew W. Hosek, Jessica R. Lu +4

The Quintuplet star cluster is one of only three known young ( Myr) massive (M M) clusters within pc of the Galactic Center. In order to explore star…

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…