September 13, 2004NVO Summer School1 Exploring VO Registries, Resources and Software with The NVO DataScope and Other VO Tools Tom McGlynn NASA/GSFC T.
TeV Gamma-ray Astronomy and UHECR-1 Trevor C. Weekes, Whipple Observatory, Harvard-Smithsonian Center for Astrophysics.
FCFM-BUAP VIII Latin American Symposium of High Energy Physics, 6-12 December 2010, Valparaiso, Chile Study of UV atmospheric background for UHECR detection.
Partially Supported by Inter-RPO WG – NESCAUM F ast A erosol S ensing T ools for N atural E vent T racking FASTNET CAPITA September 2004 Natural Aerosol.
1 Critical mechanical technologies for future gravitational-wave astronomy Joseph Giaime, Louisiana State University “LIGO is a mechanical experiment.”
Paul Sommers Fermilab PAC Nov 12, 2009
Chemical Composition of PM2.5 over N. America Big Bend (scale 0-15 ug/m3) G.Smoky Mtn. Yellowstone Mammuth Cave Sequoia ? ?
Paul Sommers Fermilab PAC Nov 12, 2009 Auger Science South and North.
Laue lenses for hard X-rays (> 60 keV) F. Frontera and A. Pisa on behalf of a Large Collaboration Rome, 18 March 2005.
Global and Local Dust over North America Direct questions to Rudolf B. Husar [email protected]@me.wustl.edu.
Humberto Salazar (FCFM-BUAP) for the Pierre Auger Collaboration, CTEQ- Fermilab School Lima, Peru, August 2012 Ultrahigh Cosmic Rays: The highest energy.
L. G. Sveshnikova1, O. N. Strelnikova, L. A. Kuzmichev, V.S. Ptuskin, V.A. Prosin, E.Korosteleva et al.