activity
20022014
most citedThe Nature and Origin of Substructure in the Outskirts of M31 -- II. Detailed Star Formation Histories

81 citations · 420 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2014★ 81 cited

The Nature and Origin of Substructure in the Outskirts of M31 -- II. Detailed Star Formation Histories

Edouard J. Bernard, Annette M. N. Ferguson, Jenny C. Richardson +9

While wide-field surveys of M31 have revealed much substructure at large radii, understanding the nature and origin of this material is not straightforward from morphology alone. U…

astro-ph.GA2012★ 21 cited

A Deep, Wide-Field Study of Holmberg II with Suprime-Cam: Evidence for Ram Pressure Stripping

Edouard J. Bernard, Annette M. N. Ferguson, Michael K. Barker +3

We present a deep, wide-field optical study of the M81 group dwarf galaxy Holmberg II (HoII) based on Subaru/Suprime-Cam imaging. Individual stars are resolved down to I~25.2, i.e.…

astro-ph.GA2011★ 69 cited

The Star Formation History and Dust Content in the Far Outer Disc of M31

Edouard J. Bernard, Annette M. N. Ferguson, Michael K. Barker +7

We present a detailed analysis of two fields located 26 kpc (~5 scalelengths) from the centre of M31. One field samples the major axis populations--the Outer Disc field--while the…

astro-ph.IM2009

EAGLE Spectroscopy of Resolved Stellar Populations Beyond the Local Group

Chris Evans, Yanbin Yang, Mathieu Puech +8

We give an overview of the science case for spectroscopy of resolved stellar populations beyond the Local Group with the European Extremely Large Telescope (E-ELT). In particular,…

astro-ph.IM2009

EAGLE Spectroscopy of Resolved Stellar Populations Beyond the Local Group

Chris Evans, Yanbin Yang, Mathieu Puech +8

Valuable insights into galaxy evolution can be gleaned from studies of resolved stellar populations in the local Universe. Deep photometric surveys have provided tracers of the sta…

astro-ph2008★ 63 cited

The Stellar Populations of M33's Outer Regions IV: Inflow History and Chemical Evolution

Michael K. Barker, Ata Sarajedini

We have modelled the observed color-magnitude diagram (CMD) at one location in M33's outskirts under the framework of a simple chemical evolution scenario which adopts instantaneou…