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Using a hundred million galaxies in the largest galaxy catalog ever
produced, the Dark Energy Survey has placed stringent constraints on the
composition of the universe and the growth of large-scale structure.
However, with great statistical power comes great responsibility. I will
discuss how we use the images we capture to further our understanding of
the cosmos, and some of the tools that we have developed to defend
against a wide range of potential sources of contamination that, if
untreated, could lead to spurious detections of new physics.
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Seminario CFP, hibrido: Edificio 2, Sala María de Maeztu / Zoom
Coordenadas zoom: http://cfp.ciemat.es/zoomae/eventos