activity
19952020
most citedThe New Galaxy: Signatures of its Formation

1.2k citations · 5.3k across the 66 of their papers we have counts for

collaborators

66 papers

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★ 17 cited

Resolving the Disc-Halo Degeneracy II: NGC 6946

S. Aniyan, A. A. Ponomareva, K. C. Freeman +5

The mass-to-light ratio (M/L) is a key parameter in decomposing galactic rotation curves into contributions from the baryonic components and the dark halo of a galaxy. One direct o…

astro-ph.SR2019★ 24 cited

The GALAH Survey: Temporal Chemical Enrichment of the Galactic Disk

Jane Lin, Martin Asplund, Yuan-Sen Ting +22

We present isochrone ages and initial bulk metallicities (, by accounting for diffusion) of 163,722 stars from the GALAH Data Release 2, mainly composed of main…

astro-ph.GA2018★ 9 cited

Near-identical star formation rate densities from H and FUV at redshift zero

Fiona M. Audcent-Ross, Gerhardt R. Meurer, O. I. Wong +27

For the first time both H and far-ultraviolet (FUV) observations from an HI-selected sample are used to determine the dust-corrected star formation rate density (SFRD: )…

astro-ph.SR2018★ 124 cited

The GALAH survey: An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS

S. Buder, K. Lind, M. K. Ness +31

The overlap between the spectroscopic Galactic Archaeology with HERMES (GALAH) survey & provides a high-dimensional chemodynamical space of unprecedented size. We present a…