activity
19982008
most citedThe accretion origin of the Milky Way's stellar halo

448 citations · 2.5k across the 33 of their papers we have counts for

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Showing 2004 · astro-phShow all

7 papers · 2 filters

astro-ph20041 cited

A Prototype for Science Alerts

N. W. Evans, V. Belokurov

Many of the science goals of the GAIA mission, especially for bursting or time-varying phenomena like supernovae or microlensing, require an early identification, analysis and rele…

astro-ph2004

The POINT-AGAPE survey II: An Unrestricted Search for Microlensing Events towards M31

V. Belokurov, J. An, N. W. Evans +16

An automated search is carried out for microlensing events using a catalogue of 44554 variable superpixel lightcurves derived from our three-year monitoring program of M31. Each st…

astro-ph2004

Chemical Evolution in the Carina Dwarf Spheroidal

A. Koch, E. K. Grebel, D. Harbeck +5

We present metallicities for 487 red giants in the Carina dwarf spheroidal (dSph) galaxy that were obtained from FLAMES low-resolution Ca triplet (CaT) spectroscopy. We find a mean…

astro-ph2004

A photometrically and kinematically distinct core in the Sextans dwarf spheroidal galaxy

J. T. Kleyna, M. I. Wilkinson, N. W. Evans +1

We present the line of sight radial velocity dispersion profile of the Sextans dwarf spheroidal galaxy (dSph), based on a sample of 88 stars extending to about 1 degree (about 1.5…

astro-ph2004

Distant field BHB stars and the mass of the Galaxy II: Photometry and spectroscopy of UKST candidates 16<B<19.5, 11<R<52 kpc

L. Clewley, S. J. Warren, P. C. Hewett +2

This is the second in a series of papers presenting a new calculation of the mass of the Galaxy based on radial velocities and distances for a sample of faint 16 < B < 21.3 field b…

astro-ph2004

Classical novae from the POINT-AGAPE microlensing survey of M31 -- I. The nova catalogue

M. J. Darnley, M. F. Bode, E. Kerins +16

The POINT-AGAPE survey is an optical search for gravitational microlensing events towards the Andromeda Galaxy (M31). As well as microlensing, the survey is sensitive to many diffe…