We are a collaborative group of
the Astronomy Department
at New Mexico State University, and
The Centre for Astrophysics
& Supercomputing at The
Swinburne University of Techonology (Australia). We are engaged in
research using the technique of quasar absorption lines to study the
kinematic, ionization, and chemical conditions of gas associated with
intermediate and high redshift galaxies and simulations to understand
the general evolution of galaxies. Our goals are to contribute to the
growing body of knowledge of the role of gas in galaxy formation and
evolution.
You can access our Hubble Space Telescope
Project Page via the link
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13398
You can access the MgII Absorber-Galaxy Catalog
via the link
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MAGIICAT
Videos of presentations of research at the 2013 Santa Cruz Galaxy Work Shop: (enjoy!):
+ "Evidence that the cool/warm CGM is self-similar with halo mass" by Chris Churchill
+ "Halo Abundance matching: accuracy and convergence" by Anatoly Klypin
+ "Radiative feedback slows high-z low-mass galaxy formation" by Daniel Ceverino
+ "Inflows, outflows and star formation in ART simulations" by Liz Klimek
+ "Simulating the tidal stripping of satellite galaxies" by Kenza Arraki
+ "Galaxy assembly with radiative feedback and local star formation" by Sebastian Trujillo-Gomez
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