activity
20012020
most citedThe chemical composition of the Sun

9.4k citations · 12k across the 39 of their papers we have counts for

collaborators

39 papers

astro-ph.GA2020★ 54 cited

Exploring the Galaxy's halo and very metal-weak thick disk with SkyMapper and Gaia DR2

G. Cordoni, G. S. Da Costa, D. Yong +16

In this work we combine spectroscopic information from the \textit{SkyMapper survey for Extremely Metal-Poor stars} and astrometry from Gaia DR2 to investigate the kinematics of a…

astro-ph.GA2019

4MOST Consortium Survey 2: The Milky Way Halo High-Resolution Survey

N. Christlieb, C. Battistini, P. Bonifacio +19

We will study the formation history of the Milky Way, and the earliest phases of its chemical enrichment, with a sample of more than 1.5 million stars at high galactic latitude. El…

astro-ph.SR2019★ 68 cited

Chemical (in)homogeneity and atomic diffusion in the open cluster M67

F. Liu, M. Asplund, D. Yong +4

Context. The benchmark open cluster M67 is known to have solar metallicity and similar age as the Sun. It thus provides us a great opportunity to study the properties of solar twin…

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…

astro-ph.SR2018★ 84 cited

Effective temperature determinations of late-type stars based on 3D non-LTE Balmer line formation

A. M. Amarsi, T. Nordlander, P. S. Barklem +3

Hydrogen Balmer lines are commonly used as spectroscopic effective temperature diagnostics of late-type stars. However, the absolute accuracy of classical methods that are based on…

astro-ph.GA2017

The age and abundance structure of the stellar populations in the central sub-kpc of the Milky Way

T. Bensby, S. Feltzing, A. Gould +6

The four main findings about the age and abundance structure of the Milky Way bulge based on microlensed dwarf and subgiant stars are: (1) a wide metallicity distribution with dist…