activity
20032023
most citedStellar Orbits Around the Galactic Center Black Hole

805 citations · 5.3k across the 101 of their papers we have counts for

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Showing 2016Show all

7 papers · 1 filter

astro-ph.EP2016★ 51 cited

Planets Around Low-Mass Stars (PALMS). VI. Discovery of a Remarkably Red Planetary-Mass Companion to the AB Dor Moving Group Candidate 2MASS J22362452+4751425

Brendan Bowler, Michael Liu, Dimitri Mawet +11

We report the discovery of an extremely red planetary-mass companion to 2MASS J22362452+4751425, a 0.6 late-K dwarf likely belonging to the 120 Myr AB Do…

astro-ph.GA2016★ 2 cited

Observational constraints on the formation and evolution of the Milky Way nuclear star cluster with Keck and Gemini

Tuan Do, Andrea Ghez, Mark Morris +7

Due to its proximity, the Milky Way nuclear star cluster provides us with a wealth of data not available in other galactic nuclei. In particular, with adaptive optics, we can obser…

astro-ph.GA2016

Constraining the Variability and Binary Fraction of Galactic Center Young Stars

Abhimat K. Gautam, Tuan Do, Andrea M. Ghez +6

We present constraints on the variability and binarity of young stars in the central 10 arcseconds (~0.4 pc) of the Milky Way Galactic Center (GC) using Keck Adaptive Optics data o…

astro-ph.IM2016★ 5 cited

`imaka - a ground-layer adaptive optics system on Maunakea

Mark Chun, Olivier Lai, Douglas Toomey +12

We present the integration status for `imaka, the ground-layer adaptive optics (GLAO) system on the University of Hawaii 2.2-meter telescope on Maunakea, Hawaii. This wide-field GL…

astro-ph.IM2016★ 8 cited

The InfraRed Imaging Spectrograph (IRIS) for TMT: latest science cases and simulations

Shelley A. Wright, Gregory Walth, Tuan Do +36

The Thirty Meter Telescope (TMT) first light instrument IRIS (Infrared Imaging Spectrograph) will complete its preliminary design phase in 2016. The IRIS instrument design includes…

astro-ph.GA2016★ 288 cited

An Improved Distance and Mass Estimate for Sgr A* from a Multistar Orbit Analysis

A. Boehle, A. M. Ghez, R. Schödel +11

We present new, more precise measurements of the mass and distance of our Galaxy's central supermassive black hole, Sgr A*. These results stem from a new analysis that more than do…