Project Grant 2606193
- The National Science Foundation Division of Astronomical Sciences awarded The University of Kentucky Research Foundation $421,913 on September 1, 2026, to advance CLOUDY, an open-source spectral synthesis computer program used to interpret spectroscopic observations of stars, galaxies, and other cosmic objects. CLOUDY models gas and dust across the full range of astrophysical environments, from cold molecular clouds to hot ionized plasmas, and is widely applied to interpret observations of...
- The National Science Foundation Division of Astronomical Sciences awarded The Johns Hopkins University $370,257 on September 1, 2026, under the Mathematical and Physical Sciences program (CFDA 47.049) to support collaborative research examining spatially-resolved drivers of star formation and active galactic nuclei feedback using the KILOGAS survey. The research analyzes data from 500 nearby galaxies observed with the Atacama Large Millimeter Array (ALMA) to map recent star-formation histories...
- The National Science Foundation Division of Astronomical Sciences awarded the University of Illinois $365,817 on September 1, 2026, under the Mathematical and Physical Sciences program (CFDA 47.049) to conduct collaborative research on spatially-resolved drivers of star formation and active galactic nuclei feedback using the KILOGAS survey. The research examines relationships between molecular gas, star formation, and black hole activity across 500 nearby galaxies observed with the Atacama Large...
- This Project Grant award from the National Science Foundation's (NSF) Division of Astronomical Sciences, under the Mathematical and Physical Sciences Federal Grant Program (CFDA 47.049), provides $526,998 to Yale University to conduct research on the star formation process. The primary objectives are to: Use millimeter-wave observations from the Atacama Large Millimeter Array (ALMA) to probe the structure and evolution of star-forming regions, specifically examining how material is funneled from...
- The National Science Foundation Division of Astronomical Sciences awarded the University of Florida $438,426 on September 1, 2026, under the Mathematical and Physical Sciences program (CFDA 47.049) to conduct observational research on gas flows in star formation. The research analyzes the ALMA Panta Rei large program dataset, mapping 259 star-forming clumps to trace gas flows from parsec-scale clouds to 1000 AU cores and linking observations across multiple high-resolution programs (DIHCA,...
- 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...
- The National Science Foundation Division of Astronomical Sciences awarded Associated Universities Inc. $222,386 on September 1, 2026, under the Mathematical and Physical Sciences program (CFDA 47.049) to characterize the demographics and properties of pre-main sequence stars and their protoplanetary disks. The research team will develop AI and machine learning tools for efficient forward modeling of protoplanetary disk radiative transfer models applied to Atacama Large Millimeter/Submillimeter...
- The National Science Foundation (NSF) Division of Astronomical Sciences awarded a $208,448 Project Grant to The University of Kentucky Research Foundation to develop a software tool for modeling the rest-optical emission line spectra of distant galaxies dating back to the early universe, or "cosmic dawn". The award will support collaborative research by PIs Shapley and Sanders to analyze data from hundreds of galaxies observed roughly 10 billion years ago, when the universe was forming...
- The Smithsonian Astrophysical Observatory will receive $190,606 under a Project Grant from the National Science Foundation Division of Astronomical Sciences to conduct the ALMA CMZ Exploration Survey. The Observatory will lead critical components of the Survey to map gas flows and star formation across the entire central region of the Milky Way galaxy, known as the Central Molecular Zone. Products will include a catalog of extended and compact gas and protostellar mass components in the Zone, as...
- This $228,609 National Science Foundation Project Grant supports research into understanding high-mass star formation through observations of cold, dense gas cores using the Atacama Large Millimeter/submillimeter Array (ALMA) telescope. Led by the Massachusetts Institute of Technology, the research team will conduct a systematic survey of potential starless, high-mass gas clumps within 5 kiloparsecs of Earth to reveal any embedded high-mass cores. Detailed ALMA observations will deliver...
The National Science Foundation Division of Astronomical Sciences awarded The University of Kentucky Research Foundation $447,036 on August 15, 2026, under the Mathematical and Physical Sciences program (CFDA 47.049) to conduct a multiphase astrophysics survey of molecular clouds and star formation in the Virgo galaxy cluster. The funded research uses the Atacama Large Millimeter Array (ALMA) to observe 40 galaxies in the Virgo cluster, measuring the distribution, density, and dynamical properties of giant molecular clouds as fundamental units of star formation. Researchers will integrate ALMA observations with data from the Very Large Telescope, Hubble Space Telescope, and the Very Large Array to analyze gas and stellar kinematics, linking molecular gas physics at tens of parsec scales to galaxy evolution and environmental processing in dense galaxy clusters. The project addresses how environmental processes affect star formation rates and long-term evolution in cluster galaxies by providing high-resolution, multiwavelength observations of inner galactic regions where residual star formation occurs. The work also includes training of undergraduate, graduate, and postdoctoral students, and development of public outreach materials. The award obligates $447,036 with a period of performance through July 31, 2029. Work is performed in Lexington, Kentucky. The survey results are intended to support interpretation of lower-resolution galaxy evolution studies in more distant galaxy clusters and to contextualize large observing programs targeting extreme systems under environmental effects.
Mod # | Description | ReasonForModification | Federal Obligation | Date |
|---|---|---|---|---|
| Not listed | $447.0k | 8/5/26 |