Vasily Belokurov
Reader in Astrophysics
at the Institute of Astronomy, University of Cambridge

Graduated from Moscow State University, Relativistic Astrophysics Department, Sternberg Astronomical Institute.
I did my DPhil at the University of Oxford where I worked with Wyn Evans.


IDL helpline  Most Common IDL Programming Errors
 
In Soviet Russia, stars observe you!!
Support gravity, my people would.
 Contact
email: vasily at ast.cam.ac.uk
phone: +44 1223 337515
office: Hoyle H20
address: Institute of Astronomy
  Madingley Road
  Cambridge, CB30HA

 Data/Tools
Milky Way Halo
Put your objects on the map of the MW stellar halo. Also plots various satellites from these lists

Solber
a simple IDL optimization routine loosely based on genetic algorithms

Microlensing maps
Maps of microlensing optical depth towards the Bulge in three different Galaxy models

SOMs for OGLE
Unsupervised classification scheme for a large lightcurve dataset
 Press
The Gaia Sausage: the major collision that changed the Milky Way
 Cambridge University PR

A bridge of stars connects two dwarf galaxies
 Cambridge University PR

Sgr tails
 Cambridge University PR

Discovery of 4 new dwarfs
 Nature
 New Scientist
 grani.ru, elementy.ru

Discovery of CVn and Boo dwarfs
 SDSS press release
 New Scientist
 gazeta.ru

Field of Streams
 SDSS press release
 New Scientist
 grani.ru

 Research

 Plots/figures/images



 Publications
3 most recent refereed papers on ADS
May 2019 'The assembly history of the Galactic inner halo inferred from α-element patterns'
We explore the origin of the observed decline in [O/Fe] (and [Mg/Fe]) with Galactocentric distance for high-metallicity stars ([Fe/H] > -1

Apr 2019 'The origin of galactic metal-rich stellar halo components with highly eccentric orbits'
Using the astrometry from the ESA's Gaia mission, previous works have shown that the Milky Way stellar halo is dominated by metal-rich stars on highly eccentric orbits

Apr 2019 'Quantifying the smoothness of the stellar halo: a link to accretion history'
We investigate the utility of the three-dimensional two-point correlation function (3D 2PCF) in quantifying substructure in the stellar halo of the Milky Way, particularly as a means of constraining the accretion history of our Galaxy


All publications in ADS 
3 most recent ArXiv papers
2019-03-06 '4MOST Consortium Survey 1: The Milky Way Halo Low-Resolution Survey'

2019-03-06 '4MOST: Project overview and information for the First Call for Proposals'

2019-02-12 'Rediscovery of the Sixth Star Cluster in the Fornax Dwarf Spheroidal Galaxy'


All e-prints on astro-ph 
 Photos
Some are on the old Oxford homepage

Cambridge
 Barcelona, June 2006
 Santa Fe, March 2006
 Moscow, June 2005
 NYC, May 2005
 Moscow, January 2005
 Snow in Cambridge, 03/03/2005
 21, 22, 23 January 2005
 Itai's leaving do, November 2004
 Windows, 2004
  Paris, October 2004
  colour | B/W | B/W 2
 Graduation, October 2004
 Moscow, July 2004