Grants & Technical Writing
2015
Wisconsin Focus on Energy Environmental and Economic Research and Development (EERD) Program
Wisconsin Building Code Analysis II
2014
American Society of Heating, Refrigeration and Air-conditioning Engineers (ASHRAE)
Development of the ASHRAE Design Guide for Dedicated Outdoor-Air Systems
U.S. Department of Energy (DOE), Office of Energy Efficiency and Renewable Energy (EERE)
Commercial Building Operational Assessment: Market Research
Minnesota Department of Commerce, Conservation Applied Research and Development (CARD)
The Energy Conservation Potential of Displacement Ventilation Technology in Minnesota Climate Conditions
Wisconsin Focus on Energy Environmental and Economic Research and Development (EERD) Program
Wisconsin Building Code Analysis: Identifying Low-Cost, High-Impact Measures
2012
NASA, Suzaku Cycle 7, 299,000 seconds (PI)
An Unbiased Sample: Constraining Redshift Evolution with Optically-selected Clusters of Galaxies II
2011
NASA, Chandra Cycle 13, 150,000 seconds, $53,416 (PI)
Expanding the Frontiers with Chandra: Observations of the Most Massive z>0.6 Cluster of Galaxies Known
NASA, Suzaku Cycle 6, 285,000 seconds (PI)
An Unbiased Sample: Constraining Redshift Evolution with Optically-selected Clusters of Galaxies
NASA, Suzaku Cycle 6, 290,000 seconds (PI)
Observing Distant Galaxy Clusters from the Spitzer SpARCS Survey with Suzaku
2010
NASA, XMM-Newton Cycle 10, 55,000 seconds (PI)
Massive Galaxy Clusters at High-redshift from the Spitzer SpARCS Survey
NASA, XMM-Newton Cycle 10, 30,000 seconds (Co-I)
Constraining Cluster Evolution at z > 1 with the SpARCS/RCS Cluster Surveys
NASA, Astrophysics Data Analysis Program, $35,419 (Co-I)
Virgo Clusters at Redshift 0.35
NASA, Suzaku Cycle 5, 134,000 seconds, $15,933 (PI)
Deciphering Cluster Observables: Tracing the Baryons in Clusters of Galaxies
2009
NASA, Chandra Cycle 11, 160,000 seconds, $70,000 (Co-I)
Massive Galaxy Clusters at High Redshift from the Spitzer SpARCS Survey
NASA, Suzaku Cycle 4, 68,000 seconds, $15,978 (PI)
Deciphering Cluster Observables: Tracing the Baryons in Clusters of Galaxies
2008
NASA, Chandra Cycle 10, 144,000 seconds, $88,653 (PI)
Deciphering Cluster Observables: Tracing the Baryons in Clusters of Galaxies
NASA, Suzaku Cycle 3, 297,000 seconds, $18,235 (PI)
Cosmology with Clusters: Constraining Physical Differences Between X-ray and Optically Selected Samples at Moderate-z
NASA, Spitzer Cycle 5, 9.9 hrs, $18,000 (Co-I)
Activity in a z~1 Supercluster
2007
NASA, Suzaku Cycle 2, 33,000 seconds, $19,667 (PI)
A Suzaku Snapshot Survey of High-redshift Galaxy Clusters from the RCS Survey
2006
NASA, GALEX Cycle 3, 46,500 seconds (31 orbits), $83,999 (PI)
Measuring Star Formation Rates in Clusters of Galaxies With GALEX
NASA, Chandra Cycle 8, archival proposal, $65,000 (PI)
Solving the Cooling Flow Mystery: Understanding Variations in Star Formation Efficiency Using the Chandra Archive
NASA, Chandra Cycle 8, 25,000 seconds, $22,999 (Co-I)
The Halo Structure of RCS2-2327.4-0204, 2006
NASA, Hubble Space Telescope Cycle 15, 22 orbits, $77,653 (Co-I)
The Halo Structure of RCS2-2327.4- 0204
2005
NASA, XMM-Newton Cycle 5, 100,000 seconds, $46,419 (Co-I)
Diagnostics and Effects of the Outburst in Hercules-A
NASA, XMM-Newton Cycle 5, 15,000 seconds, $55,418 (PI)
Mass Constraints on High Redshift Clusters of Galaxies with XMM-Newton
NASA, Suzaku Cycle 1, 180,000 seconds, $51,401 (Co-I)
Nailing Down the Hard X-ray Inverse Compton Emission from the Radio Halo in the Coma Cluster
NASA, Suzaku Cycle 1, 135,000 seconds, $42,560 (Co-I)
Hard X-ray Inverse Compton Emission and a Merger Shock Associated with the Brightest Known Radio Relic in Abell 3667
2004
American Astronomical Society International Travel Grant, $2,000
2002
NASA Graduate Student Research Program Fellowship, $90,000
2001
Women’s Forum of Colorado Foundation, $5,000
Successful Grants and Proposals (pre-2016):
