to support technical development for directly imaging exoplanets

for the 51 Pegasi b Fellowship

to create a new numerical model for planetary atmosphere circulation and chemistry

for the research and related work of Teresa Paneque-Carreño in connection with the 51 Pegasi b Fellowship program

for the experimental study of radiation damage in nucleic acids under simulated M dwarf exoplanet conditions

for hidden-sector and ultralight dark matter searches using semiconductor technology

for examining whether M-Earths can sustain surface liquid water via alternative reservoirs

to test whether recalcitrant organic compounds can be used as biosignatures on ocean worlds

to investigate how the evolution of the Sun influenced early microbial life

to investigate the atmospheres of brown dwarfs and giant exoplanets

for a reconvening for the funded researchers at the Foundation

for the Direct Imaging Roundtable

for the 51 Pegasi b Review Panel

for 51 Pegasi b Science Summit expenses

for 51 Pegasi b Science Summit expenses

for 51 Pegasi b Science Summit expenses

to fund an Axion Roundtable at the Foundation

for 51 Pegasi b professional development expenses for fellows

for 51 Pegasi b Science Summit expenses

for the 51 Pegasi b Review Panel

for 51 Pegasi b Science Summit expenses

to fund the annual 51 Pegasi b Fellowship review process

to support the 2025 51 Pegasi b Summit

to assess water world habitability using liquid phase ocean chemistry & atmospheric photochemistry

to investigate how volcanic rocks contribute to chemical evolution in a prebiotic environment

for 28 nights of observing time on the Anglo-Australian Telescope to complete the Satellites Around Galactic Analogs survey

for modeling the atmospheric evolution of planets orbiting flaring M dwarf stars

to fund activities during Phase 1 of the Cosmic Axion Spin Precession Experiment (CASPEr), a search for ultra-light dark matter particles such as axions and dark photons

for equipment and initial development of the Dark Matter Radio search for ultra-light axions and hidden photons

for the construction and operation of the Phase I Dark Matter Radio experiment

to search for and characterize closely-separated binary systems of super massive black holes

for research on the formation and evolution of gas giant planets

for modeling chemistry, heat transfer, and material fluxes at the sea floor of Waterworld oceans.

to support the development of novel algorithms and computational tools for high precision radial velocity measurements in the near-infrared wavelengths

for the 2018 Emerging Researchers in Exoplanet Science Symposium

to support the development of a new computational and statistical framework for discovering and characterizing low-mass exoplanets using upcoming extremely precise spectrographs

for the Emerging Researchers in Exoplanet Science Symposium VII

for the 2024 Order of the Octopus SETI Conference

to develop technology and techniques that will advance the state-of-the-art in direct exoplanet imaging

for the 51 Pegasi b Fellowship

for the development of more sophisticated methodologies and computational tools for measuring the stellar orbits of stars near supermassive black holes to further our understanding of the physics associated with black holes

for the Keck Planet Finder Community Cadence initiative

to investigate the origin of small planets with the Keck Planet Finder

to develop novel computational modeling tools to test general relativity at the event horizon of a supermassive black hole

to apply astronomical image processing to fluorescence microscopy imagery

to fund Boston University’s activities during Phase 1 of the Cosmic Axion Spin Precession Experiment (CASPEr), a search for ultra-light dark matter particles such as axions and dark photons

to apply astronomical image processing to fluorescence microscopy imagery

for analyzing data from the Gattini-IR wide-field infrared imager

to bridge a flight delay for the GAPS experiment

to research the origins of Hot Jupiters and Super Earths