This National Science Foundation (NSF) Mathematical and Physical Sciences Program (CFDA 47.049) Project Grant award provides $251,928 to the University of Chicago to conduct collaborative research on combining galaxy and cosmic microwave background surveys to obtain precise and robust constraints on cosmology - the distribution of matter throughout the universe. The research team will analyze complementary measurements of galaxy positions, gravitational lensing of galaxies, gravitational lensing...
This Project Grant award, provided by the National Science Foundation (NSF) under the Integrative Activities program (CFDA 47.083), aims to establish a collaboration between the University of Hawaii (UH) and Duke University to advance supernova cosmology research. The $277,608 award will support activities to: Leverage UH-led supernova discovery surveys, such as Pan-STARRS and ATLAS, to significantly reduce key systematic uncertainties in cosmological parameters. This will be achieved by...
The University of Chicago received a $366,748 Project Grant award from the National Science Foundation Division of Astronomical Sciences on September 1, 2021 to complete the project by August 31, 2024. The grant supports collaborative research on cosmic shear measurements on extremely large scales using the Dark Energy Camera. This award falls under the NSF's Mathematical and Physical Sciences program (CFDA 47.049), which aims to promote progress in these fields and strengthen the national...
This federal Project Grant award from the National Science Foundation's (NSF) Mathematical and Physical Sciences program, with CFDA number 47.049, will provide $788,071 to the University of Hawaii (UH) for the "Cosmology in the Local Volume with Hawaii Supernova Flows" research project. The primary goals of this 3-year project are to significantly expand the Hawaii Supernova Flows Survey by using over 3,000 new Type Ia supernovae to map the largest structures in the universe out to 300...
This $717,600 National Science Foundation project grant, funded under the Mathematical and Physical Sciences program (CFDA 47.049), supports research to better understand the nature of dark energy and the expansion of the universe. The principal investigator will use the Young Supernova Experiment to measure a uniform sample of Type Ia supernovae in the nearby universe and develop novel methods for determining cosmological parameters. They will also identify Type Ia supernovae in distant...
This three-year, four hundred twenty-six thousand seven hundred forty-eight dollar Project Grant from the National Science Foundation Division of Astronomical Sciences will fund research at Cornell University to combine measurements from cosmic microwave background experiments and galaxy clustering surveys to probe the nature of gravity, dark matter, and neutrinos in the universe. Key products will include the highest signal-to-noise pairwise kinematic Sunyaev-Zeldovich measurements to date...
This Project Grant award of $605,057 from the National Science Foundation's (NSF) Mathematical and Physical Sciences program (CFDA 47.049) supports research by Professor Blazek's team at Northeastern University. The research aims to advance the scientific understanding of dark energy and dark matter through improved modeling and analysis of galaxy data from the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST). Key focus areas include determining galaxy formation processes,...
This $457,976 Project Grant awarded by the National Science Foundation's (NSF) Division of Astronomical Sciences under the Mathematical and Physical Sciences program (CFDA 47.049) supports research to develop a novel framework for constraining models of baryonic feedback in the universe. The research team at the University of Chicago will apply artificial intelligence and machine learning techniques to data from cosmic microwave background and galaxy surveys to gain insights into the...
The National Science Foundation (NSF) awarded a $291,840 Project Grant under the Mathematical and Physical Sciences Federal Grant Program (CFDA 47.049) to the University of Chicago. The grant supports collaborative research to develop and apply new techniques for precisely measuring the motions of faint stars using ground-based survey telescopes, including the Dark Energy Camera (DECam) on the NSF's 4-meter Blanco Telescope. The research aims to provide the most accurate measurements of the...
This National Science Foundation award provides $345,251 to the University of Maryland, College Park under the Mathematical and Physical Sciences federal grant program (CFDA 47.049) to develop a framework for interpreting panchromatic observations of galaxy cluster halos. Working with the University of California, Santa Cruz, the awardees will use large cosmological simulations and machine learning techniques to understand the complex covariances of dark matter halo properties as traced by...
This $345,303 project grant award from the National Science Foundation's (NSF) Mathematical and Physical Sciences program supports collaborative research by scientists at the University of Hawaii and the University of Chicago. The researchers will analyze data from multiple state-of-the-art astronomical surveys, including the Dark Energy Survey (DES), South Pole Telescope (SPT), and Atacama Cosmology Telescope (ACT), to obtain precise and unbiased constraints on the properties of the universe. Key research activities include measuring the distribution of matter throughout the cosmos using techniques like gravitational lensing, and assessing potential tensions between late-time matter distribution measurements and early-universe predictions. The award also supports the development of new teaching modules to provide high school and undergraduate students hands-on experience with real astronomy data and data science. This research program aims to improve our understanding of the origin, future, and composition of the universe by leveraging complementary observational data.