activity
20142019
most cited4MOST: Project overview and information for the First Call for Proposals

311 citations · 1.1k across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.IM2019★ 8 cited

4MOST Survey Strategy Plan

G. Guiglion, C. Battistini, C. P. M. Bell +30

The current status of and motivation for the 4MOST Survey Strategy, as developed by the Consortium science team, are presented here. Key elements of the strategy are described, suc…

astro-ph.IM2019★ 7 cited

4MOST Scientific Operations

C. J. Walcher, M. Banerji, C. Battistini +65

The 4MOST instrument is a multi-object spectrograph that will address Galactic and extragalactic science cases simultaneously by observing targets from a large number of different…

astro-ph.IM2019★ 311 cited

4MOST: Project overview and information for the First Call for Proposals

R. S. de Jong, O. Agertz, A. Agudo Berbel +335

We introduce the 4-metre Multi-Object Spectroscopic Telescope (4MOST), a new high-multiplex, wide-field spectroscopic survey facility under development for the four-metre-class Vis…

astro-ph.GA2019★ 22 cited

HERBS I: Metallicity and alpha enhancement along the Galactic bulge minor axis

L. Duong, M. Asplund, D. M. Nataf +3

To better understand the origin and evolution of the Milky Way bulge, we have conducted a survey of bulge red giant branch and clump stars using the HERMES spectrograph on the Angl…

astro-ph.SR2018★ 34 cited

Estimating stellar ages and metallicities from parallaxes and broadband photometry - successes and shortcomings

Louise M. Howes, Lennart Lindegren, Sofia Feltzing +2

A deep understanding of the Milky Way galaxy, its formation and evolution requires observations of huge numbers of stars. Stellar photometry, therefore, provides an economical meth…

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…