Office: Hoyle H34
Office Tel: (01223) 766096
More Info (Internal)
I am interested in understanding the old stars of the Milky Way because they reveal the early history of our Galaxy. I mostly use spectra of large stellar surveys, such as SDSS and Gaia-ESO. Their chemistry, kinematics and ages give us information of how the formation of the Milky Way was.
As a active user of those large datasets, I became very involved in the work related to the calibration of methods that analyse automatically the spectra from those surveys. I lead the spectroscopic analysis of the Gaia FGK benchmark stars, which are the pillar calibrators of Gaia and the Gaia-ESO Survey. In addition, I am one of the coordinators of the spectroscopic analysis of the South Ecliptic Pole Catalog, which is currently being employed for the commissioning phase of Gaia.
2000-2006: Undergraduate studies in Astronomy in Universidad Catolica de Chile
2006-2010: PhD in Physics in Max Planck Insitute for Astrophysics, Garching, Germany
2011-2013: Post-doctorate in Observatoire de Bordeaux, France
2013-to date: Post-doctorate in University of Cambridge
2011: 100 Chilean leader Women