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Projekt Druckansicht

Multi-wavelength studies of the luminous and dark mass profiles of galaxy-clusters in wide-field imaging surveys

Antragsteller Dr. Thomas Erben
Fachliche Zuordnung Astrophysik und Astronomie
Förderung Förderung von 2005 bis 2009
Projektkennung Deutsche Forschungsgemeinschaft (DFG) - Projektnummer 5449189
 
Erstellungsjahr 2012

Zusammenfassung der Projektergebnisse

After the recent determination of the fundamental cosmological constants, a profound understanding of the dark and luminous matter distribution in the Universe is one of the key problems in modern cosmology. Hereby, clusters of galaxies provide well-defined laboratory environments to study the mass distribution and galaxy evolution over wide ranges of matter and galaxy densities. Today’s widefield imaging cameras offer a unique opportunity to obtain large and statistically very well understood samples of clusters, with a selection based solely on their mass properties, using their weak gravitational lensing imprint on the shape of faint (background) galaxies. Our SPP project primarily aimed at exploiting optical wide-field imaging surveys for cluster science. It consisted of significant technical developments in the fields of data processing from state-of-the art optical wide-field imaging instruments and the extraction of photometric and morphological information from astronomical sources. Our technical developments were the basis for a great many of important scientific results. Most important are the extraction of significant samples of shear-selected galaxy-cluster candidates and the collection of large sets of high-redshift z ≈ 3 Lyman-Break galaxies.

Projektbezogene Publikationen (Auswahl)

 
 

Zusatzinformationen

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