activity
20182021
most citedThe dynamics of the globular cluster NGC3201 out to the Jacobi radius

30 citations · 56 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202130 cited

The dynamics of the globular cluster NGC3201 out to the Jacobi radius

Zhen Wan, William Oliver, Holger Baumgardt +7

As part of a chemo-dynamical survey of five nearby globular clusters with 2dF/AAOmega on the AAT, we have obtained kinematic information for the globular cluster NGC3201. Our new o…

astro-ph.GA2020

The GALAH+ Survey: Third Data Release

Sven Buder, Sanjib Sharma, Janez Kos +44

The ensemble of chemical element abundance measurements for stars, along with precision distances and orbit properties, provides high-dimensional data to study the evolution of the…

astro-ph.GA201926 cited

The GALAH Survey: Chemically tagging the Fimbulthul stream to the globular cluster Centauri

Jeffrey D. Simpson, Sarah L. Martell, Gary Da Costa +17

Using kinematics from Gaia and the large elemental abundance space of the second data release of the GALAH survey, we identify two new members of the Fimbulthul stellar stream, and…

astro-ph.GA2019

The Great Escape: Discovery of a nearby 1700 km/s star ejected from the Milky Way by Sgr A*

Sergey E. Koposov, Douglas Boubert, Ting S. Li +17

We present the serendipitous discovery of the fastest Main Sequence hyper-velocity star (HVS) by the Southern Stellar Stream Spectroscopic Survey (S5). The star S5-HVS1 is a $\sim…

astro-ph.GA2019

The Southern Stellar Stream Spectroscopic Survey (): Overview, Target Selection, Data Reduction, Validation, and Early Science

T. S. Li, S. E. Koposov, D. B. Zucker +29

We introduce the Southern Stellar Stream Spectroscopy Survey (), an on-going program to map the kinematics and chemistry of stellar streams in the Southern Hemisphere. The i…

astro-ph.SR2018

The GALAH Survey: Verifying abundance trends in the open cluster M67 using non-LTE spectroscopy

Xudong Gao, Karin Lind, Anish M. Amarsi +28

Open cluster members are coeval and share the same initial bulk chemical compositions. Consequently, differences in surface abundances between members of a cluster that are at diff…