# Keck HIRES Spectroscopy of SkyMapper Commissioning Survey Candidate Extremely Metal-Poor Stars

## TL;DR

This study analyzes high-resolution spectra of 17 candidate extremely metal-poor stars from SkyMapper data, revealing their chemical compositions and identifying rare stellar types, thereby advancing understanding of early Galactic chemical evolution.

## Contribution

First high-resolution spectroscopic analysis of SkyMapper EMP candidates, providing detailed chemical abundances and identifying rare stellar populations.

## Key findings

- Three stars have [Fe/H] <= -3.0, indicating extreme metal deficiency.
- Most stars follow known abundance trends, with some showing unique low [Ba/Fe] and [Sr/Ba] ratios.
- Identification of potential r-I stars among the sample.

## Abstract

We present results from the analysis of high-resolution spectra obtained with the Keck HIRES spectrograph for a sample of 17 candidate extremely metal-poor (EMP) stars originally selected from commissioning data obtained with the SkyMapper telescope. Fourteen of the stars have not been observed previously at high dispersion. Three have [Fe/H]<=-3.0 while the remainder, with two more metal-rich exceptions, have -3.0<=[Fe/H]<=-2.0 dex. Apart from Fe, we also derive abundances for the elements C, N, Na, Mg, Al, Si, Ca, Sc, Ti, Cr, Mn, Co, Ni, and Zn, and for n-capture elements Sr, Ba, and Eu. None of the current sample of stars is found to be carbon-rich. In general our chemical abundances follow previous trends found in the literature, although we note that two of the most metal-poor stars show very low [Ba/Fe] (~-1.7) coupled with low [Sr/Ba] (~-0.3). Such stars are relatively rare in the Galactic halo. One further star, and possibly two others, meet the criteria for classification as a r-I star. This study, together with that of Jacobson et al. (2015), completes the outcomes of the SkyMapper commissioning data survey for EMP stars.