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20122025
most citedAn Improved Distance and Mass Estimate for Sgr A* from a Multistar Orbit Analysis

288 citations · 1.4k across the 23 of their papers we have counts for

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Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA2021★ 30 cited

A Spatially-Resolved Survey of Distant Quasar Host Galaxies: I. Dynamics of galactic outflows

Andrey Vayner, Shelley A. Wright, Norman Murray +6

We present observations of ionized gas outflows in eleven z radio-loud quasar host galaxies. Data was taken with the integral field spectrograph (IFS) OSIRIS and the a…

astro-ph.GA2021★ 10 cited

A Spatially-Resolved Survey of Distant Quasar Host Galaxies: II. Photoionization and Kinematics of the ISM

Andrey Vayner, Shelley A. Wright, Norman Murray +6

We present detailed observations of photoionization conditions and galaxy kinematics in eleven z radio-loud quasar host galaxies. Data was taken with OSIRIS integral fi…

astro-ph.GA2018★ 4 cited

Widespread Shocks in the Nucleus of NGC 404 Revealed by Near-infrared Integral Field Spectroscopy

A. Boehle, J. E. Larkin, L. Armus +1

We present high spatial resolution, integral field spectrograph (IFS) observations of the nearby LINER (low ionization nuclear emission line region) galaxy NGC 404 at 1.25 m (J…

astro-ph.GA2017★ 40 cited

The Post-Periapse Evolution of Galactic Center Source G1: The second case of a resolved tidal interaction with a supermassive black hole

Gunther Witzel, Breann. N. Sitarski, Andrea M. Ghez +13

We present new Adaptive Optics (AO) imaging and spectroscopic measurements of Galactic Center source G1 from W. M. Keck Observatory. Our goal is to understand its nature and relati…

astro-ph.GA2017★ 6 cited

Testing the gravitational theory with short-period stars around our Galactic Center

A. Hees, A. M. Ghez, T. Do +19

Motion of short-period stars orbiting the supermassive black hole in our Galactic Center has been monitored for more than 20 years. These observations are currently offering a new…

astro-ph.GA2017★ 271 cited

Testing General Relativity with stellar orbits around the supermassive black hole in our Galactic center

A. Hees, T. Do, A. M. Ghez +14

In this Letter, we demonstrate that short-period stars orbiting around the supermassive black hole in our Galactic Center can successfully be used to probe the gravitational theory…

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…

astro-ph.GA2013★ 4 cited

The Keplerian orbit of G2

L. Meyer, A. M. Ghez, G. Witzel +8

We give an update of the observations and analysis of G2 - the gaseous red emission-line object that is on a very eccentric orbit around the Galaxy's central black hole and predict…

astro-ph.GA2013★ 91 cited

Keck Observations of the Galactic Center Source G2: Gas Cloud or Star?

K. Phifer, T. Do, L. Meyer +8

We present new observations and analysis of G2 - the intriguing red emission-line object which is quickly approaching the Galaxy's central black hole. The observations were obtaine…

astro-ph.GA2012★ 227 cited

The Shortest Known Period Star Orbiting our Galaxy's Supermassive Black Hole

L. Meyer, A. M. Ghez, R. Schoedel +7

Stars with short orbital periods at the center of our galaxy offer a powerful and unique probe of a supermassive black hole. Over the past 17 years, the W. M. Keck Observatory has…