Overview
An Emmy-Noether research group headed by Dr. Knud
Jahnke and funded by the German
Science Foundation DFG is in the buildup-phase at MPIA. The leading
topic of the 5 year research plan (09/2007-08/2012) is the Coevolution
of Galaxies and Black Holes.
In a number of projects the influence and interaction of the formation of
supermassive black holes in the centers of massive galaxies on the surrounding
galaxy is explored. The main aim is to constrain the relative interdependence
of galaxy interactions, induced star formation, AGN activity and its effect on
the migration of massive galaxies from. Keywords are: Starburst-merger-AGN
connection and AGN feedback.
Projects
Individual projects are:
-
Determining the Bulge- or stellar mass vs. Black Hole-mass relation of
galaxies out to
z>2 and constrain its evolution over 10 Gyrs using data from the
GEMS and COSMOS galaxy surveys
with the HST and Laser Guide Star Adaptive Optics assisted Integral Field
Spectroscopic data from SINFONI at ESO VLT.
-
Studying the incidence of merging of galaxies for active galaxies in
COSMOS in direct
comparison to inactive galaxies as a function of redshift, luminosity and
environment. A crucial aspect is finding the limits of which degree of
interaction can actually be seen in HST images as a function of time since a
galaxy merger.
- Studying the incidence, mass and ages of star-formation in AGN host
galaxies as a function of galaxy luminosity, morphology and signs of
interaction. We will use two spectroscopic datasets from FORS2 and the VIMOS IFU at ESO VLT.
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People
Beside Knud Jahnke as lead, the group is consisting of
- Dr. Katherine Inskip, postdoctoral researcher (formerly Sheffield
University, since 03/2008)
- Mauricio Cisternas, graduate student (from the Universidad
Catolica in Santiago de Chile, since 08/2008)
- Dading Nugroho, graduate student (from the Institut Teknologi Bandung,
Indonesia, since 08/2008)
- René Andrae, graduate student (from University
of Heidelberg, Germany, since 05/2009)
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