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Lund Observatory announces two openings for postdoctoral positions, in stellar populations and exoplanet research, respectively.

Postdoc 1 - Gaia-ESO Survey of the Milky Way

The stellar population group at the Department of astronomy and theoretical physics is engaged in the 300 night Gaia-ESO Survey that will run on the Very Large Telescope in Chile. The project is called Gaia-ESO Survey. The survey will explore all the components of the Milky Way using high resolution spectroscopy and abundance analysis of several hundred thousand stars. The survey is not only a very significant investment in observing time but also in manpower. We are looking for a postdoctral fellow who can participate in the abundance analysis within the survey.
Closing date: February 1, 2012

Announcement in English: Apply Online
Announcement in Swedish (Ledigkungörelse på svenska): Ansök online

Information about the research in the stellar population group at Lund Observatory.
Contact persons: Sofia Feltzing (sofia@astro.lu.se) and Thomas Bensby (tbensby@astro.lu.se)



Postdoc 2 - formation and evolution of planetary systems

Research on the formation and evolution of planetary systems is in rapid development, fuelled by the wealth of new observational data and the advent of more and more powerful supercomputers. Lund University invites applicants to a postdoc position within the topic of planet formation and orbital evolution of planetary systems. The succesfull applicant will work within the PEBBLE2PLANET project funded by a Starting Grant from the European Research Council.

Closing date: February 1, 2012
Announcement in English: Apply Online
Announcement in Swedish (Ledigkungörelse på svenska): Ansök online

Information about the exoplanet research at Lund Observatory.
Contact person: Anders Johansen (anders@astro.lu.se)



Lund Observatory, Box 43, SE-221 00 Lund, Sweden
Visiting address: Sölvegatan 27
Phone: +46 46 22 27300, Fax: +46 46 22 24614
Publisher: Leif Lönnblad
E-mail: webmaster@astro.lu.se
Last updated: 2011, December 13

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