Project Grant 2605354
- The National Science Foundation Division of Astronomical Sciences awarded The Regents of the University of California $380,062 under the Mathematical and Physical Sciences federal grant program (CFDA 47.049) for the project "Adaptive Optics Astrometry for Black Hole Science" from September 1, 2021 to August 31, 2024. The University of California, Berkeley will utilize the funding to deliver products and services supporting black hole research through adaptive optics astrometry...
- This $442,985 Project Grant awarded by the National Science Foundation's (NSF) Mathematical and Physical Sciences Program (CFDA 47.049) aims to uncover the growth mechanisms of supermassive black holes. The key objectives are to: 1) Determine the merger rates of supermassive black holes and relate them to gravitational wave observations; 2) Investigate the growth of supermassive black holes during their peak activity period (known as "cosmic noon") and its connection to accretion...
- The National Science Foundation Division of Astronomical Sciences awarded the University of California, Los Angeles $422,493 on January 1, 2026, under the Mathematical and Physical Sciences program (CFDA 47.049) to develop computational tools and models explaining early galaxy formation and the role of growing black holes and star formation in the early universe. The recipient will create an analytic model of the "burstiness" in early star formation and its effects on chemical...
- The National Science Foundation Division of Astronomical Sciences awarded the University of California, San Diego $507,993 on October 1, 2026, under the Mathematical and Physical Sciences program (CFDA 47.049) to establish GROWL (Gravitational-Wave Paleontology Catalog), a unified, publicly accessible framework standardizing and comparing over 10,000 theoretical models of compact object mergers across cosmic time. The project integrates existing simulations from leading codes including COMPAS,...
- The National Science Foundation Division of Astronomical Sciences awarded Vanderbilt University $440,415 on September 1, 2026, under the Mathematical and Physical Sciences program (CFDA 47.049) to identify and characterize black holes in dwarf galaxies using Dark Energy Spectroscopic Instrument (DESI) data. The research will use DESI Data Release 1 and multiple detection methods to conduct a comprehensive, multi-wavelength census of active black holes in dwarf galaxies, applying machine learning...
- The University of California, San Diego will receive $330,903 over three years from the National Science Foundation Division of Astronomical Sciences under a Project Grant award to support research titled "COLLABORATIVE RESEARCH: CDS & E: CONSTRAINING THE UNCERTAIN PHYSICS OF GALAXY FORMATION: COSMIC RAYS, BLACK HOLES, AND BEYOND." The award falls under the Mathematical and Physical Sciences program (CFDA 47.049), which aims to promote progress in these scientific fields and...
- The National Science Foundation Division of Astronomical Sciences awarded a $496,234 Project Grant to the University of Illinois under the Mathematical and Physical Sciences federal grant program (CFDA 47.049). The grant will fund collaborative research to explore the formation and growth of supermassive black holes through variability and transients observations. Researchers will use data from the Young Supernova Experiment imaging survey to identify intermediate mass black holes and study...
- This National Science Foundation project grant of $104,875 awarded on January 1, 2023 will fund research into measuring fluctuations in radiation from active supermassive black holes and the resulting echoes from surrounding gas clouds. Led by researchers at the University of Wisconsin-Madison under the Mathematical and Physical Sciences program (CFDA 47.049), this two-year project will use reverberation mapping with multi-object spectroscopy to measure black hole masses on an unprecedented...
- The National Science Foundation Division of Astronomical Sciences awarded Drexel University $472,915 on September 1, 2026, under the Mathematical and Physical Sciences program (CFDA 47.049) to develop machine-learning methods for identifying active galactic nuclei and supermassive black holes in data from the NSF/DOE Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST). The project combines astronomy and data science to create a probabilistic latent-space model that integrates...
- This $120,000 Project Grant award, provided by the National Science Foundation (NSF) under the CFDA program 47.049 Mathematical and Physical Sciences, supports fundamental research on gravitational astrophysics and computational methods to advance scientific understanding of neutron stars, black holes, gravitational waves, and the large-scale structure of the universe. The award will fund a series of research projects at the University of California, San Diego (UCSD) focused on developing new...
The National Science Foundation Division of Astronomical Sciences awarded the University of California, San Diego $490,197 on October 1, 2026, under the Mathematical and Physical Sciences program (CFDA 47.049) to conduct a multi-year observational survey identifying black hole populations in Milky Way globular clusters. The research will use the Keck Cosmic Web Imager to systematically survey six galactic globular clusters via radial velocity measurements of stellar companions to detect new black hole candidates. The program will perform tiled exposures providing complete spatial coverage in three clusters with large observed core radii, yielding radial velocity measurements for over a thousand stars in the clusters' centers. Follow-up observations of candidate binaries identified from prior MUSE observations in three additional galactic clusters will also be performed. The project responds to predictions from N-body simulations indicating correlation between black hole population size and a globular cluster's core radius, and will provide observational constraints to test whether stellar clusters serve as sites for black hole binary mergers that produce gravitational wave sources detected by current observatories. The researchers will also present multimedia shows combining astronomy education and music performance to increase public accessibility to astronomy. Performance occurs at UC San Diego in La Jolla, California. The period of performance runs from October 1, 2026, through September 30, 2029.
Mod # | Description | ReasonForModification | Federal Obligation | Date |
|---|---|---|---|---|
| Not listed | $490.2k | 8/5/26 |