Funding
Since 2000, McNamara's group has received grants from NASA and the Department of Energy totaling more than one million dollars in direct funding to Ohio University and more than $3.4 million, overall.
  1. Spitzer Space Telescope, Cycle 2 (2005-2007): "Starbursts and Supercavities in Clusters of Galaxies"
  2. Space Telescope Science Institute (2001-2002): "Structural Properties of Brightest Cluster Galaxies"
  3. NASA Long Term Space Astrophysics (2001-2005): "A Reexamination of Cooling Flows and Radio Galaxies in the Chandra Era"
  4. Chandra General Observer Project, Cycle 1 (2000-2001): "ACIS Imaging of Cluster Cooling Flows with the Largest Star Formation Rates"
  5. Chandra General Observer Project, Cycle 2 (2001-2002): "Chandra Observations of MS0440.5+0204 & MS0839.9+2938: Cooling Flow Clusters in Formation"
  6. Chandra General Observer Project, Cycle 3 (2002-2003): "The Fate of Matter in the Moderate Cooling Flow Cluster Abell 1991"
  7. Chandra General Observer Project, Cycle 3 (2002-2003): "A Systematic Study of Cool- ing Flows and Radio Galaxies Using the Chandra Archive"
  8. Los Alamos National Laboratory, (2002-2004): "Life Cycles of Active Galaxies"
  9. Chandra General Observer Project, Cycle 4 (2003-2004): "Reduced Cooling and Feed- back in Cluster Cooling Flows"
  10. Chandra General Observer Project, Cycle 5 (2004-2005): "A Deep Look at the Radio- ICM Interaction In the Powerful Radio Galaxy Hydra A"
  11. Chandra General Observer Project, Cycle 5 (2004-2005): "A Systematic Study of Cool- ing Flows and Radio Galaxies Using the Chandra Archive II"
  12. Spitzer Space Telescope, Cycle 1 (2004-2006): "Mid-Infrared Observations of Massive Cooling Flows"
  13. XMM-Newton, AO-4 Guest Observer Award (2005-2006): "Giant Cavities and Large Scale Shocks in the Distant Cluster MS0735.6+7421,"
  14. Hubble Space Telescope Cycle 14, "The Nuclear Environment of the Galaxy Hosting the Largest Known Radio Outburst"
Ohio University Department of Physics and Astronomy | Ohio University Astrophysics