activity
20122026
most citedThe GALAH+ Survey: Third Data Release

626 citations · 4.9k across the 107 of their papers we have counts for

collaborators
Showing 2022Show all

10 papers · 1 filter

astro-ph.GA2022★ 13 cited

The impact of carbon and oxygen abundances on the metal-poor initial mass function

Piyush Sharda, Anish M. Amarsi, Kathryn Grasha +5

Star formation models predict that the metal-poor initial mass function (IMF) can be substantially different from that observed in the metal-rich Milky Way. This changeover occurs…

astro-ph.GA2022★ 81 cited

The Gaia-ESO survey: mapping the shape and evolution of the radial abundance gradients with open clusters

L. Magrini, C. Viscasillas Vazquez, L. Spina +27

The spatial distribution of elemental abundances and their time evolution are among the major constraints to disentangle the scenarios of formation and evolution of the Galaxy. We…

astro-ph.GA2022★ 9 cited

Spectroscopic follow-up of statistically selected extremely metal-poor star candidates from GALAH DR3

G. S. Da Costa, M. S. Bessell, Thomas Nordlander +5

The advent of large-scale stellar spectroscopic surveys naturally leads to the implementation of machine learning techniques to isolate, for example, small sub-samples of potential…

astro-ph.SR2022★ 5 cited

A high-resolution spectroscopic search for multiple populations in the 2 Gyr old cluster NGC 1846

Wei Shen Oh, Thomas Nordlander, Gary Da Costa +1

We present detailed C, O, Na, Mg, Si, Ca, Ti, V, Fe, Zr, Ba, and Eu abundance measurements for 20 red giant branch (RGB) stars in the LMC star cluster NGC 1846 ([Fe/H] = -0.59). Th…

astro-ph.GA2022★ 8 cited

A method for identifying metal-poor stars with Gaia BP/RP spectra

Theodora Xylakis-Dornbusch, Norbert Christlieb, Karin Lind +1

Context. The study of the oldest and most metal-poor stars in our Galaxy promotes our understanding of the Galactic chemical evolution and the beginning of Galaxy and star formatio…

astro-ph.SR2022★ 44 cited

Non-LTE abundance corrections for late-type stars from 2000Å to 3μm: I. Na, Mg, and Al

K. Lind, T. Nordlander, A. Wehrhahn +6

It is well known that cool star atmospheres depart from local thermodynamic equilibrium (LTE). Accurate abundance determination requires taking those effects into account, but the…

astro-ph.EP2022

The Volatile Carbon to Oxygen Ratio as a Tracer for the Formation Locations of Interstellar Comets

Darryl Z. Seligman, Leslie A. Rogers, Samuel H. C. Cabot +13

Based on the occurrence rates implied by the discoveries of 1I/`Oumuamua and 2I/Borisov, the forthcoming Rubin Observatory Legacy Survey of Space and Time (LSST) should detect $\ge…

astro-ph.IM2022

Emu: A Case Study for TDI-like Imaging for Infrared Observation from Space

Joice Mathew, James Gilbert, Robert Sharp +14

A wide-field zenith-looking telescope operating in a mode similar to Time-Delay-Integration (TDI) or drift scan imaging can perform an infrared sky survey without active pointing c…

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.SR2022★ 18 cited

Chemical Properties of the Local Disk and Halo. II. Abundances of 3745 M dwarfs and Subdwarfs from Improved Model Fitting of Low-Resolution Spectra

Neda Hejazi, Sebastien Lepine, Thomas Nordlander

We present a model-fit pipeline to determine the stellar parameters of M-type dwarfs, which is an improvement upon our previous work described in Hejazi et al. 2020. We apply this…