activity
20152021
most citedThe GALAH+ Survey: Third Data Release

626 citations · 1.5k across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2021★ 96 cited

: The Orbital and Chemical Properties of One Dozen Stellar Streams

Ting S. Li, Alexander P. Ji, Andrew B. Pace +19

We report the kinematic, orbital, and chemical properties of 12 stellar streams with no evident progenitors, using line-of-sight velocities and metallicities from the Southern Stel…

astro-ph.GA2021★ 121 cited

Measuring the Mass of the Large Magellanic Cloud with Stellar Streams Observed by

Nora Shipp, Denis Erkal, Alex Drlica-Wagner +16

Stellar streams are excellent probes of the underlying gravitational potential in which they evolve. In this work, we fit dynamical models to five streams in the Southern Galactic…

astro-ph.GA2021★ 30 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★ 626 cited

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.GA2019★ 26 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★ 133 cited

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★ 123 cited

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★ 56 cited

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…

astro-ph.GA2018★ 17 cited

The GALAH survey: Co-orbiting stars and chemical tagging

Jeffrey D. Simpson, Sarah L. Martell, Gary Da Costa +24

We present a study using the second data release of the GALAH survey of stellar parameters and elemental abundances of 15 pairs of stars identified by Oh et al 2017. They identifie…

astro-ph.SR2016★ 77 cited

The Galah Survey: Classification and diagnostics with t-SNE reduction of spectral information

G. Traven, G. Matijevič, T. Zwitter +24

Galah is an ongoing high-resolution spectroscopic survey with the goal of disentangling the formation history of the Milky Way, using the fossil remnants of disrupted star formatio…

astro-ph.IM2016★ 81 cited

The GALAH survey: The data reduction pipeline

Janez Kos, Jane Lin, Tomaž Zwitter +29

We present the data reduction procedures being used by the GALAH survey, carried out with the HERMES fibre-fed, multi-object spectrograph on the 3.9~m Anglo-Australian Telescope. G…

astro-ph.GA2015★ 91 cited

A 10 kpc stellar substructure at the edge of the Large Magellanic Cloud: perturbed outer disk or evidence for tidal stripping?

Dougal Mackey, Sergey E. Koposov, Denis Erkal +3

We report the discovery of a substantial stellar overdensity in the periphery of the Large Magellanic Cloud (LMC), found using public imaging from the first year of the Dark Energy…