Main NASA Case Study Catalog
creation universe
Relativity
Quantum Gravity Successes
High energy Astrophysics Mat Page Mullard Space Science Lab, UCL 9. The cosmic X-ray and -ray background.
1 Dayabay RPC Detector Zhang Jiawen 2010-7-19. 2 Outline Motivation RPC introduce RPC for Daya Bay Efficiency and noise Module structure Module.
Star formation at high redshift (2 < z < 7) Methods for deriving star formation rates UV continuum = ionizing photons (dust obscuration?) Ly = ionizing.
1 SWCX: A Background Component You Should Care About Take Brad’s talk to heart. For observations of objects which cover the FOV with surface brightnesses.
LSSO-10/2007 SWCX in the XMM era K.D.Kuntz The Henry A. Rowland Department of Physics and Astronomy The Johns Hopkins University.
Measurement of B ( (nS) + ) at CLEO István Dankó Rensselaer Polytechnic Institute representing the CLEO Collaboration 1 st Meeting of the APS.
Rana Adhikari Caltech The Next Gravity Wave Interferometers.
Sub-arcsecond far-infrared observatory A science imperative.
