Project Grant 2408324
Award Date
9/1/24
Completion Date
8/31/27
Dollars Obligated
$153K
Federal Agency
Division of Astronomical Sciences
Federal Grant Program
47.049
Assistance Type
Project Grant
Place of Performance
Lacey, WA 98503, USA
Similar Awards
This federal Project Grant award, totaling $105,646, was provided by the National Science Foundation (NSF) under the Mathematical and Physical Sciences program (CFDA 47.049) to support a collaborative research project led by Seattle University. The research aims to confirm the origins of stars in the Milky Way's metal-poor bulge by spectroscopically measuring the elemental abundances of candidate globular cluster tidal debris stars. The project will involve obtaining detailed observations of...
This $109,108 federal Project Grant award from the National Science Foundation's (NSF) Division of Astronomical Sciences under the Mathematical and Physical Sciences (CFDA 47.049) program supports a collaborative research project titled "The Disintegration of Clusters and their Contribution to the Metal-Poor Bulge" at Western Washington University. The research aims to confirm the origin of stars from disrupted globular clusters that have contributed to the Milky Way's bulge. The...
The National Science Foundation Division of Astronomical Sciences has awarded a $644,032 Project Grant to the Massachusetts Institute of Technology (MIT) to conduct research on reconstructing the early formation history of the Milky Way galaxy. The research, funded through the NSF's Mathematical and Physical Sciences program (CFDA 47.049), will observe the oldest known metal-poor stars in the galaxy using high-resolution spectroscopy. This will allow the investigator to characterize the sites...
This three-year, $153,949 Project Grant from the National Science Foundation's Mathematical and Physical Sciences program (CFDA 47.049) supports research to create a unique catalog of open star clusters in the Milky Way disk through observations and analysis. The University of Utah will observe nearly all suitable open star clusters using spectroscopy from the Sloan Digital Sky Survey V and astrometry from the Gaia satellite. Additional high-resolution spectroscopy will measure abundances of...
This $522,357 National Science Foundation project grant under the Mathematical and Physical Sciences program (CFDA 47.049) supports research at the University of California, Merced to simulate the life cycle of star clusters from birth to death within a cosmological galactic context from September 2021 through August 2024. Key products include data analysis and publications on identifying and characterizing spiral arms in galaxies. A $25,000 subaward to Bryn Mawr College supports coordination...
This Project Grant award from the National Science Foundation (NSF) under the Mathematical and Physical Sciences program (CFDA 47.049) supports collaborative research to investigate the evolution of the Magellanic Clouds, two small dwarf galaxies that orbit the Milky Way. The $416,880 award to Montana State University will be used to map the kinematic and chemical abundance patterns across the Magellanic Clouds in order to identify evidence of past interactions and accretion of smaller...
This National Science Foundation (NSF) Project Grant award under the Mathematical and Physical Sciences program (CFDA 47.049) provides $169,884 to the University of Virginia to conduct collaborative research on discriminating between galactic feedback models using next-generation observations. The project will incorporate an existing stellar feedback model (SMUGGLE) into the AREPO cosmological simulation code to self-consistently produce thousands of simulated galaxies that can be compared...
This three-year, $357,003 National Science Foundation Project Grant under the Mathematical and Physical Sciences program (CFDA 47.049) will support continued investigations of nearby dwarf galaxies as well as expanded studies of dwarf galaxies in galaxy groups within a radius of five million parsecs. Key deliverables include mapping dark matter halos within Milky Way satellites via multi-epoch spectroscopy; analyzing detailed chemical abundance patterns at low metallicities characteristic of...
This $244,369 Project Grant awarded by the National Science Foundation's Mathematical and Physical Sciences program supports research to identify and characterize populations of massive stellar binary systems, composed of a black hole or neutron star and a massive star, in nearby low-metallicity dwarf galaxies. The project will use multiwavelength archival data to study these "high mass X-ray binaries" as analogs to similar systems that may have formed in the early universe....
This National Science Foundation (NSF) Division of Astronomical Sciences Project Grant award of $457,353 to The Ohio State University supports a program of data analysis and modeling to interpret the elemental abundance patterns of stars in the Milky Way and its dwarf satellite galaxies. The research, which runs from September 1, 2023 to August 31, 2026, aims to build a coherent picture of the stellar and galactic-scale phenomena that govern the synthesis of chemical elements. This work will...