Galaxy feedback in 3D Roberto Maiolino. Feedback is the key: - reducing SF efficiency (gas heating+turbulence) - removing baryons Discrepancy between.
Ecsite 2012 - Science Centers and Planetaria as Citizen Science Platforms
Mariangela Bernardi UPitt/UPenn Galaxies Properties in the SDSS: Evolution, Environment and Mass Galaxies Properties in the SDSS: Evolution, Environment.
Is the Sodium Na D line useful? Marcel Bergmann Bo Milvang-Jensen.
Phil James Liverpool John Moores University Astrophysics Research Institute 22nd August 2007 STFC PhD Summer School, Durham The Structure of Galaxies.
Physics 10, introductory lecture A. Albrecht January 2010.
Probing dark matter clustering using the Lyman- forest Pat McDonald (CITA) COSMO06, Sep. 28, 2006.
ADASS, London Sep 23-26, 2007 VOExplorer : Visualising Data Discovery in the Virtual Observatory Jonathan Tedds University of Leicester/AstroGrid/ EuroVO.
Is the Sodium Na D line useful?
An Evolutionary Connection between AGNs and GALEX UV-excess Early-type Galaxies
Multi-wavelength Properties and Environments of the SDSS Galaxies divided into Fine Classes
Supernova Legacy Survey (SNLS) Goal: Characterize the Dark Energy equation of state “w” parameter
