This Project Grant award of $356,389 from the National Science Foundation's (NSF) Mathematical and Physical Sciences Program (CFDA 47.049) will fund a computational study to better understand the formation and evolution of massive galaxies. The principal investigator at the University of Massachusetts (UMass) will conduct a high-resolution simulation using the newly developed Enzo-E code to investigate key processes, including: (1) supermassive black hole formation and growth, (2) the impact...
This three-year, $130,077 Project Grant from the National Science Foundation's Division of Astronomical Sciences, under the Mathematical and Physical Sciences program (CFDA 47.049), will fund collaborative research to better understand galaxy cluster merger dynamics. The Smithsonian Institution Astrophysical Observatory will analyze observational data and hydrodynamical simulations of ten galaxy clusters to map the projected total mass density, intracluster medium emissivity and temperature,...
This National Science Foundation (NSF) grant award under the Mathematical and Physical Sciences program (CFDA 47.049) provides $270,796 to the University of Massachusetts to conduct a comprehensive survey of a large sample of candidate dusty starburst galaxies in the early universe. The main objectives are to determine accurate redshifts and positions, and define a statistically significant sample of galaxies at z > 6. This will involve deep optical and near-infrared follow-up observations to...
This Project Grant from the National Science Foundation Division of Astronomical Sciences provides $269,690 to support research and education activities under the Mathematical and Physical Sciences program (CFDA 47.049). A collaboration between the University of Nevada, University of California Los Angeles, and Arizona State University will develop advanced galaxy modeling tools and conduct cross-correlation analyses to maximize scientific return from upcoming telescopes studying the epoch of...
This National Science Foundation award provides $161,052 to the University of Massachusetts under the Mathematical and Physical Sciences program (CFDA 47.049) from September 1, 2022 through August 31, 2025. The funding supports collaborative research to develop advanced hydrodynamic galaxy simulation software to study the complex interplay between stellar winds and the circumgalactic medium surrounding massive galaxies. Researchers will incorporate a subgrid wind model into an existing...
This $539,342 Project Grant award from the National Science Foundation's (NSF) Division of Astronomical Sciences will support research into the unexpectedly high number of bright, rapidly star-forming galaxies observed at the cosmic dawn. The award recipient, Princeton University, will conduct simulations and analytical modeling to understand the physical conditions that could explain these observations, particularly in the context of massive dark matter halos at high redshift. The research aims...
This National Science Foundation (NSF) Division of Astronomical Sciences Project Grant award of $512,912 to Arizona State University (ASU) supports a 3-year research program to study the evolution of galaxies in high-redshift clusters. The project will utilize deep observations from the Atacama Large Sub/Millimeter Array (ALMA), Hubble Space Telescope (HST), and Very Large Telescope (VLT) to map star formation, measure baryon fractions, evaluate disk stability, and identify quenching...
This $206,240 project grant from the National Science Foundation Division of Astronomical Sciences will fund research and educational activities to advance understanding of galaxy formation and evolution processes through multi-wavelength studies of circumgalactic media (CGM). Specifically, the University of Colorado researchers will (1) use machine learning to interpret new X-ray data in light of hydrodynamical simulations to constrain CGM physics, (2) explore using radio and fast radio...
This Project Grant award of $598,336, provided by the National Science Foundation (NSF) under the Mathematical and Physical Sciences program (CFDA 47.049), supports the University of Connecticut's research into advancing galaxy evolution modeling and cosmological hydrodynamic simulations. The project aims to overcome limitations of current simulations by developing: 1) physically predictive models of galaxies at sub-parsec resolution to study the coevolution of supermassive black holes and...
This National Science Foundation (NSF) Division of Astronomical Sciences Project Grant award of $433,221.00 to the University of Illinois aims to advance understanding of star formation processes in galaxies. The research team will spatially resolve connections between the cold molecular gas fuel and declining star formation rates in aging galaxies, using a combination of observational data and computer simulations. They will leverage recently completed surveys and state-of-the-art...