activity
19942026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 16.6k across the 111 of their papers we have counts for

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Showing 2017Show all

8 papers · 1 filter

astro-ph.GA2017★ 32 cited

What the Milky Way bulge reveals about the initial metallicity gradients in the disc

F. Fragkoudi, P. Di Matteo, M. Haywood +5

We examine the metallicity trends in the Milky Way (MW) bulge - using APOGEE DR13 data - and explore their origin by comparing two N-body models of isolated galaxies which develop…

astro-ph.GA2017★ 114 cited

Bar quenching in gas-rich galaxies

S. Khoperskov, M. Haywood, P. Di Matteo +2

Galaxy surveys have suggested that rapid and sustained decrease in the star-formation rate, "quenching", in massive disk galaxies is frequently related to the presence of a bar. Op…

astro-ph.GA2017★ 23 cited

Chemical Mapping of the Milky Way With The Canada-France Imaging Survey: A Non-parametric Metallicity-Distance Decomposition of the Galaxy

Rodrigo Ibata, Alan McConnachie, Jean-Charles Cuillandre +41

We present the chemical distribution of the Milky Way, based on 2,900 of -band photometry taken as part of the Canada-France Imaging Survey. When complete, this…

astro-ph.GA2017★ 103 cited

The Canada-France Imaging Survey: First results from the u-band component

Rodrigo Ibata, Alan McConnachie, Jean-Charles Cuillandre +41

The Canada-France Imaging Survey (CFIS) will map the northern high Galactic latitude sky in the -band ("CFIS-u", 10,000) and in the -band ("CFIS-r", 5,000$\,…

astro-ph.GA2017★ 27 cited

Effects of the selection function on metallicity trends in spectroscopic surveys of the Milky Way

G. Nandakumar, M. Schultheis, M. Hayden +3

We investigate here the effect of the selection function on the metallicity distribution function (MDF) and on the vertical metallicity gradient by studying similar lines of sight…

astro-ph.SR2017★ 108 cited

PLATO as it is: a legacy mission for Galactic archaeology

A. Miglio, C. Chiappini, B. Mosser +102

Deciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high-resolution chrono-chemo-kinematical maps of the Galaxy.…