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Mordecai-Mark Mac Low
American Museum Natural History
$3,558,491
Attributed
$11,327,746
Total exposure
17
Grants
6
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 $3.3M · FY2006–23$5M$3.8M$2.5M$1.3M$0
'06
'07
'08
'09
'10
'11
'12
'13
'14
'15
'16
'17
'18
'19
'20
'21
'22
'23
Funding mix
By agency
NSF$11,327,746 · 17
By mechanism
—$11,327,746 · 17
Top collaborators
- Dennis Robbins3 shared
- Kathleen Saavik Ford3 shared
- Timothy A Paglione3 shared
- Denton S Ebel2 shared
- Greg L Bryan2 shared
- Jason L Maron2 shared
- Edmond A Mathez1 shared
- James D Webster1 shared
Grant awards (17)
The Untimely Deaths of Star Clusters$546,269
· FY2023 · MPS · contact PI
AstroCom NYC: A Partnership between New York City Astronomers$1,692,284
· FY2022 · MPS
AstroCom NYC: A Partnership between Astronomers in New York City$1,097,405
· FY2018 · MPS
AstroCom NYC: A Partnership between Astronomers at CUNY, AMNH, and Columbia University$1,750,814
· FY2012 · MPS
An Innovative Approach to Earth Science Teacher Preparation: Uniting Science, Informal Science Education, and Schools to Raise Student Achievement$2,800,381
· FY2011 · EDU
What Controls Star Formation in Galaxies?$451,232
· FY2011 · MPS · contact PI
Layered accretion, vortex excitation, and planet formation in circumstellar disks$460,911
· FY2010 · MPS
Support for Attendance by Early Career Astronomers, Planetary Scientists, and Earth Scientists to the 73rd Annual Meeting of the Meteoritical Society in July 2010$19,688
· FY2010 · GEO
CDI-Type I: Combined Global Physical, Chemical, and Mineralogical Models of Protoplanetary Disks$575,192
· FY2008 · MPS · contact PI
Dwarf Galaxies, Abundance Distributions and the Physics of Galaxy Formation$382,061
· FY2008 · MPS
Stellar Duets in Theory and Observations. Common envelope, planetary nebulae and the origin of close binaries$410,019
· FY2006 · MPS
New techniques for improving the accuracy of gradients for particle and grid simulations of magnetohydrodynamic turbulence.$239,174
· FY2006 · MPS
Collaborative Research: Fireworks at the Ballet: Globular Cluster Formation, Bulge Dynamics and the Role of Central Black Holes in Galaxy Mergers$221,287
· FY2003 · MPS · contact PI
Comparing Theory with Observation Using Chemical Probes of Turbulent Molecular Clouds$149,912
· FY2003 · MPS
REU Site: Research Experiences for Undergraduates in Earth Science, Planetary Science and Astrophysics at the American Museum of Natural History$148,850
· FY2003 · MPS · contact PI
New Directions in Cluster Computing: A Conference at the American Museum of Natural History "New Directions in Cluster Supercomputing"$15,000
· FY2001 · CSE
CAREER: Structure Formation and Support by Magnetized, Supersonic Turbulence in the Interstellar Medium and Star-Forming Regions$367,267
· FY2000 · MPS · contact PI