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ITP Heidelberg involvement in the Euclid Collaboration
From the ESA official website:
"Euclid is an ESA mission to map the geometry of the dark Universe. The mission will investigate the distance-redshift relationship and the evolution of cosmic structures by measuring shapes and redshifts of galaxies and clusters of galaxies out to redshifts ~2, or equivalently to a look-back time of 10 billion years. In this way, Euclid will cover the entire period over which dark energy played a significant role in accelerating the expansion."
Luca Amendola, Professor
Theory Working Group Coordinator
Valeria Pettorino, Groupleader
Theory Working Group
CMB cross correlations
Cosmological forecasts
COMMS group (public outreach and internal communications) 2010-2013
Yashar Akrami, Postdoc
Theory Working Group
WP1 - Cosmic Acceleration
WP2 - Testing Gravity
WP5 - Deviations from Homogeneity and Isotropy
WP6 - Statistical Methods and Forecasting
Santiago Casas, PhD Student
Theory Working Group
WP6 - Statistical Methods and forecasting
WP7 - Analytical approaches to non-linearities
Alejandro Guarnizo Trilleras, PhD Student
Theory Working Group
WP6 - Statistical Methods and forecasting
WP9 - Relativistic Corrections In Observations
Matteo Martinelli, Postdoc
Theory Working Group
WP1 - Cosmic acceleration
WP2 - Testing gravity
WP6 - Statistical methods and forecasting
WP8 - Probes combination
WP10 - New observational probes
Miguel Zumalacárregui, Postdoc
Theory Working Group
WP2 - Testing Gravity
WP5 - Deviations from homogeneity and isotropy
WP7 - Analytical approaches to non-linearities
Depicts: Artist's impression of Euclid
Copyright: ESA/C. Carreau