From Darkness, Light: Computing Cosmological Reionization
1 Astronomy Applications in the TeraGrid Environment Roy Williams, Caltech with thanks for material to: Sandra Bittner, ANL; Sharon Brunett, Caltech; Derek.
Using the Grid for Astronomical Data Roy Williams, Caltech.
Was different at high redshift? DESY 2004 John Webb, School of Physics, University of New South Wales, Sydney, Australia e 2 /ħc.
Assigning a distance by redshift The Hubble law lets us use a simple spectrum of a galaxy to figure out where it is along the line-of-sight. Higher redshifts.
John Webb (UNSW) - Analysis; Fearless Leader Steve Curran (UNSW)- QSO (mm and radio) obs. Vladimir Dzuba (UNSW)- Computing atomic parameters Victor Flambaum.
Galactic Gas Kinematics and High Velocity Clouds at z~1 Chris Churchill (Penn State) Mg II 2796,2803 absorption from galaxies and ??? in quasar spectra.
Lecture 3: The Highest Redshift Quasars: Early Black Hole Evolution and the End of Reionization Xiaohui Fan AGN Summer School, USTC May 25, 2007 Background:
SIGRAV Graduate School in Contemporary Relativity and Gravitational Physics
Lyman- quasar spectra as cosmological probes MATTEO VIEL INAF & INFN – Trieste.
Evidence For Cosmological Evolution of the Fine Structure Constant?
2 nd Summer School in Astronomy Luka Č Popović Belgrade, 30.09. 2008.
