NuSTAR CIT JPL Columbia LLNL DSRI UCSC SLAC Spectrum The Nuclear Spectroscopic Telescope Array (NuSTAR) Hard X-ray (5 - 80 keV) Small Explorer (SMEX) mission.
Jim Ulvestad Division Director, AST October 13, 2011 Division of Astronomical Sciences.
Blois 2008 Suzy Collin-Zahn LUTH, Observatoire de Paris Meudon AGN, MASSIVE BLACK HOLES, ACCRETION AGN, MASSIVE BLACK HOLES, ACCRETION ARE AGN FACTORIES.
INTRODUCTION Who We Are: Northern Michigan University NASA Resource Center: Seaborg Math & Science Center Workshop Presenters: Debra Homeier, Seaborg Center.
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Simulating the joint evolution of quasars, galaxies and their large-scale distribution Springel et al., 2005 Presented by Eve LoCastro October 1, 2009.
USING LOW POWER RADIO GALAXIES AS BEACONS FOR CLUSTERS TO “FILL THE GAP” AT 1
Jets from stellar tidal disruptions by supermassive black holes Dimitrios Giannios Princeton University HEPRO3, Barcelona, June 30.
Byer Group From Quantum to Cosmos: Fundamental Physics Research in Space International Workshop, Washington, D.C. USA, May 22-24, 2006 Technology Development.
X. Barcons, XEUS SAGXEUS: Physics of the hot evolving Universe XEUS: The Physics of the hot Evolving Universe Xavier Barcons.
AST101 The Evolution of Galaxies. Virgo Cluster Collisions of Galaxies Outside of Clusters (the field), most galaxies are spiral or irregular In dense.
The Milky Way Galaxy Astronomy 315 Professor Lee Carkner Lecture 16.
