M. Haywood

The Canada–France Imaging Survey: First Results from the u-Band Component

The Canada-France Imaging Survey (CFIS) will map the northern high Galactic latitude sky in the

Bars and boxy/peanut bulges in thin and thick discs - I. Morphology and line-of-sight velocities of a fiducial model

u

Bar quenching in gas-rich galaxies

-band (CFIS-u, 10,000

In Disguise or Out of Reach: First Clues about In Situ and Accreted Stars in the Stellar Halo of the Milky Way from Gaia DR2

, {rm deg^2}

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

) and in the

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

r

Phylogeny of the Milky Way’s inner disk and bulge populations: Implications for gas accretion, (the lack of) inside-out thick disk formation, and quenching

-band (CFIS-r, 5,000

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

, {rm deg^2}

On the kinematic detection of accreted streams in the Gaia era: a cautionary tale

), enabling a host of stand-alone science investigations, and providing some of the ground-based data necessary for photometric redshift determination for the Euclid mission. In this first contribution we present the

Galactic Planetary Nebulae as Probes of Radial Metallicity Gradients and Other Abundance Patterns

u