DWDM Single Ppt Notes
90 Pitch Class
Star formation at high redshift (2 < z < 7) Methods for deriving star formation rates UV continuum = ionizing photons (dust obscuration?) Ly = ionizing.
[email protected], slide 1 German Aerospace CenterMicrowaves and Radar Institute Methodology for obtaining physical parameters from fully polarimetric.
Yanchun Liang (NAOC, China) 2005-08, Lijiang
Cosmology with the XMM Cluster Survey (XCS) Martin Sahlén, University of Sussex with Pedro Viana (Porto), Andrew Liddle, Kathy Romer (PI) and others (XCS.
School/Workshop on parallel computing in astrophysics: 19-23 April, 2010, Santiago, Chile.
Better Ness
High Redshift Radio Galaxies: The most massive galaxies up to z>5?
Star formation at high redshift (2 < z < 7)
