activity
20092026
most citedThe GALAH Survey: Observational Overview and Gaia DR1 companion

214 citations · 1.5k across the 47 of their papers we have counts for

collaborators

48 papers

astro-ph.GA2026

Barium and europium abundances from the Gaia-ESO Survey using The Cannon

Pradosh Barun Das, Francesca Primas, Gayandhi De Silva +3

Neutron-capture element abundances encode the time-dependent interplay between slow (s-) and rapid (r-) nucleosynthetic processes and provide critical constraints on Galactic chemi…

astro-ph.GA2026

The GALAH Survey: Neutron-Capture Elemental Abundances for 350,000 Gaia-RVS spectra and the Chemodynamics of Accreted Structures

Pradosh Barun Das, Daniel B. Zucker, Aldo Mura-Guzmán +15

We present a comprehensive data-driven spectroscopic analysis of 357,415 red giant stars using Gaia DR3 Radial Velocity Spectrometer (RVS) spectra (8460-8700 A; ),…

astro-ph.GA2024★ 8 cited

The GALAH Survey: Stellar parameters and abundances for 800,000 Gaia RVS spectra using GALAH DR4 and The Cannon

Pradosh Barun Das, Daniel B. Zucker, Gayandhi M. De Silva +15

Analysing stellar parameters and abundances from nearly one million Gaia Data Release 3 (DR3) Radial Velocity Spectrometer (RVS) spectra poses challenges due to the limited spectra…

astro-ph.SR2024

The Gasing Pangkah Collaboration: I. Asteroseismic Identification and Characterisation of a Rapidly-Rotating Engulfment Candidate

J. M. Joel Ong, Marc Teng Yen Hon, Melinda Soares-Furtado +19

We report the discovery and characterisation of TIC 350842552 ("Zvrk"), an apparently isolated, rapidly-rotating () red giant observed by TESS in…

astro-ph.GA2024

The GALAH survey: Elemental abundances in open clusters using joint effective temperature and surface gravity photometric priors

Kevin L. Beeson, Janez Kos, Richard de Grijs +10

The ability to measure precise and accurate stellar effective temperatures () and surface gravities () is essential in determining accurate and precise abund…

astro-ph.IM2023★ 1 cited

HRMOS White Paper: Science Motivation

Laura Magrini, Thomas Bensby, Anna Brucalassi +52

The High-Resolution Multi-Object Spectrograph (HRMOS) is a facility instrument that we plan to propose for the Very Large Telescope (VLT) of the European Southern Observatory (ESO)…

astro-ph.SR2023★ 1 cited

First Asteroseismic Analysis of the Globular Cluster M80: Multiple Populations and Stellar Mass Loss

Madeline Howell, Simon W. Campbell, Dennis Stello +1

Asteroseismology provides a new avenue for accurately measuring the masses of evolved globular cluster (GC) stars through the detection of their solar-like oscillations. We present…

astro-ph.IM2022★ 1 cited

CUBES: a UV spectrograph for the future

S. Covino, S. Cristiani, J. M. Alcala' +86

In spite of the advent of extremely large telescopes in the UV/optical/NIR range, the current generation of 8-10m facilities is likely to remain competitive at ground-UV wavelength…

astro-ph.IM2022★ 1 cited

The CUBES Science Case

Chris Evans, Stefano Cristiani, Cyrielle Opitom +51

We introduce the scientific motivations for the development of the Cassegrain U-Band Efficient Spectrograph (CUBES) that is now in construction for the Very Large Telescope. The as…

astro-ph.IM2022

CUBES, the Cassegrain U-Band Efficient Spectrograph

S. Cristiani, J. M. Alcalá, S. H. P. Alencar +74

In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at ground-UV wavelengths for the foreseeable future. The Casse…

astro-ph.SR2022★ 37 cited

Integrated Mass Loss of Evolved Stars in M4 using Asteroseismology

Madeline Howell, Simon W. Campbell, Dennis Stello +1

Mass loss remains a major uncertainty in stellar modelling. In low-mass stars, mass loss is most significant on the red giant branch (RGB), and will impact the star's evolutionary…

astro-ph.GA2022

The GALAH Survey: A New Sample of Extremely Metal-Poor Stars Using A Machine Learning Classification Algorithm

Arvind C. N. Hughes, Lee R. Spitler, Daniel B. Zucker +21

Extremely Metal-Poor (EMP) stars provide a valuable probe of early chemical enrichment in the Milky Way. Here we leverage a large sample of high-resolution stellar sp…

astro-ph.GA2021★ 93 cited

The GALAH Survey: Chemical tagging and chrono-chemodynamics of accreted halo stars with GALAH+ DR3 and eDR3

Sven Buder, Karin Lind, Melissa K. Ness +27

Since the advent of astrometry, it is possible to identify massive accreted systems within the Galaxy through their unique dynamical signatures. One such system, -Saus…

astro-ph.SR2021★ 48 cited

The K2 Galactic Archaeology Program Data Release 3: Age-abundance patterns in C1-C8 and C10-C18

Joel C. Zinn, Dennis Stello, Yvonne Elsworth +28

We present the third and final data release of the K2 Galactic Archaeology Program (K2 GAP) for Campaigns C1-C8 and C10-C18. We provide asteroseismic radius and mass coefficients,…

astro-ph.GA2021★ 11 cited

The GALAH Survey: No chemical evidence of an extragalactic origin for the Nyx stream

Daniel B. Zucker, Jeffrey D. Simpson, Sarah L. Martell +20

The results from the ESA Gaia astrometric mission and deep photometric surveys have revolutionized our knowledge of the Milky Way. There are many ongoing efforts to search these da…

astro-ph.SR2020★ 17 cited

The GALAH+ Survey: A New Library of Observed Stellar Spectra Improves Radial Velocities and Hints at Motions within M67

Tomaž Zwitter, Janez Kos, Sven Buder +25

GALAH+ is a magnitude-limited survey of high resolution stellar spectra obtained by the HERMES spectrograph at the Australian Astronomical Observatory. Its third data release provi…

astro-ph.GA2020★ 9 cited

The GALAH Survey: Dependence of elemental abundances on age and metallicity for stars in the Galactic disc

Sanjib Sharma, Michael R. Hayden, Joss Bland-Hawthorn +24

Using data from the GALAH survey, we explore the dependence of elemental abundances on stellar age and metallicity among Galactic disc stars. We find that the abundance of most ele…

astro-ph.GA2020★ 38 cited

The GALAH Survey: Chemical Clocks

Michael R. Hayden, Sanjib Sharma, Joss Bland-Hawthorn +27

Previous studies have found that the elemental abundances of a star correlate directly with its age and metallicity. Using this knowledge, we derive ages for a sample of 250,000 st…

astro-ph.GA2020★ 27 cited

Combined APOGEE-GALAH stellar catalogues using the Cannon

Govind Nandakumar, Michael R. Hayden, Sanjib Sharma +21

APOGEE and GALAH are two high resolution multi-object spectroscopic surveys that provide fundamental stellar parameters and multiple elemental abundance estimates for about half a…

astro-ph.EP2020★ 13 cited

The GALAH Survey: Using Galactic Archaeology to Refine our Knowledge of TESS Target Stars

Jake T. Clark, Mathieu Clerte, Natalie R. Hinkel +29

An unprecedented number of exoplanets are being discovered by the Transiting Exoplanet Survey Satellite (TESS). Determining the orbital parameters of these exoplanets, and especial…

astro-ph.GA2020★ 57 cited

The tidal remnant of an unusually metal-poor globular cluster

Zhen Wan, Geraint F. Lewis, Ting S. Li +18

Globular clusters are some of the oldest bound stellar structures observed in the Universe. They are ubiquitous in large galaxies and are believed to trace intense star formation e…

astro-ph.SR2020★ 50 cited

The GALAH survey: A census of lithium-rich giant stars

Sarah Martell, Jeffrey Simpson, Adithya Balasubramaniam +20

We investigate the properties of 1262 red giant stars with high photospheric abundances of lithium observed by the GALAH and \Ktwo-HERMES surveys, and discuss them in the context o…

astro-ph.GA2020★ 80 cited

Fundamental relations for the velocity dispersion of stars in the Milky Way

Sanjib Sharma, Michael R. Hayden, Joss Bland-Hawthorn +34

We explore the fundamental relations governing the radial and vertical velocity dispersions of stars in the Milky Way, from combined studies of complementary surveys including GALA…

astro-ph.EP2017★ 46 cited

The K2-HERMES Survey. I. Planet Candidate Properties from K2 Campaigns 1-3

Robert A. Wittenmyer, Sanjib Sharma, Dennis Stello +31

Accurate and precise radius estimates of transiting exoplanets are critical for understanding their compositions and formation mechanisms. To know the planet, we must know the host…