Research

The environment of NGG 1277
Astronomical Data The Astronomical Data group develops, maintains and propagates advanced methods and open-source tools for the astrophysics community, especially for building probabilistic models, discovering sources in noisy data and making precise measurements. It builds these methods and tools by carrying out in-house data analysis projects that answer important scientific questions. It also hosts events and workshops that are designed to create new data analysis opportunities for members of the astronomical community.
  • CCA
  • Biomolecular Design The theory of protein folding explains how a disordered chain of amino acids spontaneously adopts a well-defined three-dimensional structure in water. The ultimate test of a theory is its successful application to the design of new physical systems with new, desired properties. In the Biomolecular Design Group, we apply the theory of protein folding to design new heteropolymers that fold into well-defined three-dimensional structures with new, useful functions, but which are built from exotic chemical building-blocks that go beyond the 20 canonical amino acids that make up natural proteins.
  • CCB
  • Cosmology Researchers at the Center for Computational Astrophysics (CCA) stand at the forefront of advancing our understanding of the universe by melding cutting-edge machine learning and data science techniques with profound cosmological inquiries. In an era where cosmology is undergoing a transformative shift, this group spearheads the development of pioneering algorithms and innovative conceptual frameworks that are tailored to the increasingly complex cosmological datasets. Harnessing the collective power of ground-based and space-based telescopes furnished with progressively sensitive cameras and instruments, researchers at CCA are at the vanguard of endeavors such as SDSS, Vera Rubin Observatory, Euclid, SPHEREX, HIRAX and Roman Space Telescope.
  • CCA
  • Graphs of recovered gravitational waveforms. The dark band shows estimates for the waveform without assuming a particular source. The light bands show results if we assume it is a binary black hole (BBH) as predicted by general relativity. They match really well
    Gravitational Wave Astronomy Since the first detection of gravitational waves in 2015, gravitational-wave astronomy has matured into a fast growing field with far reaching implications for physics and astronomy. As of LIGO-Virgo-KAGRA's fourth observing run there are over 300 likely gravitational waves detected to date. We now routinely observe mergers of black holes and neutron stars, which continue to expand our view of the extreme physics in those compact objects, as well as the lives and deaths of the stars from which they formed. Gravitational waves and their counterparts are also a promising tool for cosmology. Our discovery potential continues to grow with improving detectors.
  • CCA
  • Stars and Plasma Astrophysics The Stars & Plasma Astrophysics (SPA) Group is dedicated to developing the theoretical framework and computational methods necessary to investigate the life and death of stars, as well as the astrophysics of neutron stars and black holes. The group’s goal is to enhance our understanding of the physics of stars, their explosive deaths and the compact remnants they leave behind. To achieve this goal, we develop theoretical and computational models of stars and stellar explosions, as well as plasma in extreme conditions, that can be tested by new observations.
  • CCA
  • Advancing Research in Basic Science and MathematicsSubscribe to Flatiron Institute announcements and other foundation updates

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