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STAYS IN INTERNATIONALLY RECOGNIZED CENTRES<br />

KEY: D=Ph. D student, P=postdoctoral. G= guest, S=staff, I= invited, O=others (specify)<br />

CENTRE: Penn Astrophysics Group<br />

PLACE: University of Pennsylvania, Philadelphia, USA<br />

DATE: March 2007 LENGHT: 3 days<br />

TOPIC: Renormalizad Perturbation Theory and Halo Model KEY: G<br />

CENTRE: Max Planck Institute for Extraterrestrial Physics<br />

PLACE: Garching, Germany<br />

DATE: October 2008 LENGHT: 9 days<br />

TOPIC: modeling of Baryon Acoustic Oscillations KEY: I<br />

CENTRE: Institute for Theoretical Physics<br />

PLACE: University of Zurich – Zurich – Switzerland<br />

DATE: March 2007 LENGHT: 8 days<br />

TOPIC: nonlinear clustering and large scale structure KEY: I<br />

CENTRE: Center for Particle Physics – Fermilab<br />

PLACE: Fermi National Laboratory – Batavia – USA<br />

DATE: February 2008 LENGHT: 1 month<br />

TOPIC: Clustering of Clusters, Dark Enery Survey KEY: I<br />

CENTRE: Service de Physique Théorique<br />

PLACE: CEA / Saclay – France<br />

DATE: March 2007 LENGHT: 8 days<br />

TOPIC: Higher order statistics in Renormalizad Perturbation Theory KEY: I<br />

CENTRE: Service de Physique Théorique<br />

PLACE: CEA / Saclay – France<br />

DATE: December 2006 LENGHT: 5 days<br />

TOPIC: Higher order statistics in Renormalizad Perturbation Theory KEY: I<br />

CENTRE: Institute of Space Science (ICE/CSIC) – Group of Astrophysics and Cosmology<br />

PLACE: Bellaterra – Spain<br />

DATE: October 2006 LENGHT: 3 months<br />

TOPIC: N-body simulations, large scales, Measure of Baryon Acoustic Oscillations KEY: D<br />

CENTRE: Theoretical Division - Los Alamos National Laboratory<br />

PLACE: Los Alamos – USA<br />

DATE: May 2003 LENGHT: 9 days<br />

TOPIC: Dynamical Casimir Effect KEY: I

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