Project Grant 2206514
- This Project Grant from the National Science Foundation Division of Astronomical Sciences provides $218,572 to San Francisco State University under the Mathematical and Physical Sciences federal grant program (CFDA 47.049) to characterize over 300 metal-poor star candidates observed in the Apache Point Observatory Galactic Evolution Experiment survey. The University will analyze and conduct follow-up observations of the metal-poor star candidates using the Lick and Keck telescopes to determine...
- The University of California Santa Cruz will receive $273,625 under a Project Grant from the National Science Foundation Division of Astronomical Sciences to develop a framework for interpreting panchromatic observations of galaxy cluster halos. The award, made under the Mathematical and Physical Sciences program (CFDA 47.049), will support collaboration between researchers at UC Santa Cruz and the University of Maryland to combine data from the Dark Energy Spectroscopic Instrument, Atacama...
- 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 Project Grant from the National Science Foundation Division of Astronomical Sciences totaling $458,054 will support research exploring the gas-phase properties of galaxies using data from the Sloan Digital Sky Survey Mapping Nearby Galaxies at Apache Point survey. Principal Investigator Scudder will analyze spatially resolved gas-phase metallicities in 10,000 galaxies from archival integral field spectra. Contamination from active galactic nuclei will be assessed. Calibration methods will...
- The National Science Foundation Division of Astronomical Sciences awarded the University of California Santa Cruz a $279,069 Project Grant under the Mathematical and Physical Sciences federal grant program (CFDA 47.049). The grant will fund a collaborative research project between University of the Pacific and University of California Santa Cruz to use spectroscopic observations of globular clusters to study the dark matter content and assembly history of the Virgo Cluster of galaxies....
- The National Science Foundation (NSF) awarded a $532,327 Project Grant under the Mathematical and Physical Sciences (CFDA 47.049) program to the University of Chicago. The funding supports a project to explore the origins of the Milky Way galaxy by analyzing the chemical fingerprints of stars in the galactic halo, which are remnants of small dwarf galaxies. The researchers will use data from the Sloan Digital Sky Survey to study approximately 400-500 metal-poor halo stars, enabling...
- This Project Grant from the National Science Foundation Division of Astronomical Sciences will support research to develop more accurate non-local thermodynamic equilibrium (non-LTE) models for analyzing spectra of metal-poor red giant stars. The University of Chicago will receive $424,475 under the award, covering the period from September 1, 2022 to August 31, 2025. The investigators will enhance existing stellar spectral analysis tools by implementing non-LTE physics and machine learning...
- This Project Grant award of $462,120.00 from the National Science Foundation (NSF) under the Mathematical and Physical Sciences (CFDA 47.049) program supports a research project focused on studying the chemical profiles of dwarf stars and their exoplanets. The key products and services to be delivered through this award include: Building a public, data-driven tool to efficiently and precisely derive stellar abundances from spectroscopic data, Measuring elemental abundances for the target lists...
- This federal Project Grant award, funded by the National Science Foundation (NSF) under the Mathematical and Physical Sciences program (CFDA 47.049), supports collaborative research to improve understanding of the final stages in the evolution of the most massive stars. The $240,810 grant, awarded to Carnegie Mellon University, will develop new tools to maximize the scientific value of data on resolved stellar populations and transient phenomena from emerging astronomical facilities like the...
- 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 Project Grant from the National Science Foundation Division of Astronomical Sciences provides $243,204 to the University of California Santa Cruz to characterize metal-poor stars in the Apache Point Observatory Galactic Evolution Experiment survey. Under the Mathematical and Physical Sciences program (CFDA 47.049), the award will fund analysis of over 300 metal-poor star candidates identified in the APOGEE survey data. Follow-up observations will be conducted at Lick and Keck Observatories to determine stellar parameters and abundances. Outreach efforts include engaging students at UC Santa Cruz and San Francisco State University, as well as public education programs on climate change and astronomy events for Latinx communities. Project results on the early nucleosynthesis and assembly of the Milky Way galaxy are expected to further the goals of the NSF program to strengthen the nation's scientific enterprise.
Mod # | Description | ReasonForModification | Federal Obligation | Date |
|---|---|---|---|---|
| Not listed | $243.2k | 8/1/22 |