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Greg L Bryan
Columbia University
$4,212,708
Attributed
$7,514,543
Total exposure
16
Grants
7
Lead (contact PI)
Attributed= this PI's even-split share of every grant they're on (the fair, additive number). Exposure = full size of all those grants.
Funding over time
peak $1.5M · FY2005–24$2M$1.5M$1M$500K$0
'05
'06
'07
'08
'09
'10
'11
'12
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'22
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'24
Funding mix
By agency
NSF$7,514,543 · 16
By mechanism
—$7,514,543 · 16
Top collaborators
- Zoltan Haiman4 shared
- Mary E Putman2 shared
- Mordecai-Mark Mac Low2 shared
- Amber D Miller1 shared
- Caleb A Scharf1 shared
- Dennis Robbins1 shared
- Frederik B Paerels1 shared
- Jeremiah P Ostriker1 shared
Grant awards (16)
Conference: First Stars VII$49,999
· FY2024 · MPS
Constraining satellite-host galaxy co-evolution with next-generation semi-analytic models$596,139
· FY2023 · MPS · contact PI
Collaborative Research: The Destruction and Growth of Halo Clouds$399,802
· FY2023 · MPS
Turning up the Heat: Using Ram Pressure Stripping in Clusters to Understand Star Formation in Extreme Conditions$442,102
· FY2021 · MPS · contact PI
Forming the First Massive Black Holes$766,826
· FY2020 · MPS
AstroCom NYC: A Partnership between Astronomers in New York City$1,097,405
· FY2018 · MPS
Collaborative Research:Framework:Software:NSCI:Enzo for the Exascale Era (Enzo-E)$439,350
· FY2018 · CSE · contact PI
CDS&E: The development of open-source software with an application to modeling the formation of globular star clusters$406,729
· FY2016 · MPS · contact PI
SI2-SSE: yt: Reusable Components for Simulating, Analyzing and Visualizing Astrophysical Systems$493,793
· FY2013 · CSE
Directly Testing the Presence of Large-Scale Multiphase Flows in the Galactic Halo$363,413
· FY2013 · MPS
Investigations of ram pressure stripping in realistic cluster environments with a multiphase ISM$302,302
· FY2009 · MPS · contact PI
Peta-Cosmology: galaxy formation and virtual astronomy$40,000
· FY2009 · CSE
Dwarf Galaxies, Abundance Distributions and the Physics of Galaxy Formation$382,061
· FY2008 · MPS
CAREER: Simulating Cosmological Galaxy Formation with Adaptive-Mesh Refinement$564,904
· FY2006 · MPS · contact PI
Feedback from the First Stars$209,571
· FY2006 · MPS · contact PI
A Multi-Wavelength Calibration of Galaxy Clusters as Cosmological Probes$960,147
· FY2005 · MPS