to upgrade the charge coupled device on the red channel of the Kast spectrometer on the Shane Telescope at the University of California Observatories Lick Observatory

for student fellowships and instructional support

to support a graduate student to run models, analyze data, and bridge the theory and observational research of white dwarf stars and type 1ax supernovae

for designing and convening the Exoplanet Summer Program

to support a class for physics majors intended to boost the retention of women and under-represented minorities

for the Exoplanet Summer Program (ESP), an entirely participant driven workshop, to take place within a new research initiative, the Other Worlds Laboratory (OWL)

to support initial instrument design and planning for a low-resolution robotic spectrograph for transient science

for developing and implementing the summer intensive AstroTech program

to support the transient astrophysics fellowship program

to support the development of a paleoclimate version of the Community Earth System Model (CESM)

for graduate student scholarships and instructional costs in the science communication program of the University of California, Santa Cruz

for the Advancing Theoretical Astrophysics Summer School

for the 51 Pegasi b Fellowship

to build the Planet as Exoplanet Analog Spectrograph (PEAS)

for the 51 Pegasi b Fellowship

for the Lick Observatory

for graduate student scholarships and instructional costs in the science communication program

for the 51 Pegasi b Fellowship

for graduate student support to develop atmospheric photochemistry and photoionization-driven escape software

to study exoplanet diversity and atmospheres

for the Conference for Undergraduate Women in Physics at UC Santa Cruz

for the 51 Pegasi b Fellowship

to develop and implement a predictive wavefront control system at the W.M. Keck Observatory

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

for the design and early construction of the Santa Cruz Array of Lenslets for Exoplanet Spectroscopy

for logistics funding to support the creation of a cross-disciplinary network strengthening academic connections and mentoring and research skills

for Unsolved Problems in Astrophysics – Cosmic Alchemy in the Era of Gravitational Wave Astronomy

for Unsolved Problems in Astrophysics – Touching the Stars

for the Shadow the Scientists astronomical observing outreach initiative

to support the Other World Laboratory Exoplanet Summer Program in 2019 and 2020

for the 51 Pegasi b Fellowship

for the 2023 and 2024 Exoplanet Summer Program workshops

for the 51 Pegasi b Fellowship

for the 2023-2025 Bay Area Planetary Science Conferences

for journalism training for the science communication program

to expand the AstroTech instrumentation program

for the research and related work of Emiel Por in connection with the 51 Pegasi b Fellowship program

to use novel synthetic DNA-based tracers to identify and characterize hydrologic flow pathways in agricultural to glacier-dominated environments

to support the design and construction of a zero-net-energy home to compete in the 2015 U.S Department of Energy Solar Decathlon

to support the development of statistical and computational algorithmic tools to reduce systematic errors on data taken by the Large Synoptic Survey Telescope

to support the design and construction of a zero-net-energy home to compete in the 2017 U.S. Department of Energy Solar Decathlon

to develop a modeling tool for stellar age determination across the Hertzsprung Russell (HR) diagram

for the Conference for Undergraduate Women in Physics

to develop squeezed-vacuum state amplifiers that will be coupled with thin-film superconducting cavities in an experimental infrastructure to detect axion dark matter particles with energies of 5-20 gigahertz (GHz)

to develop best practices for workshops and conferences

for the collection and analysis of M dwarf flaring data

for studying how AMO physics can inform the development of gravity theories

to support the development of a paleoclimate version of the Community Earth System Model (CESM) and to apply the P-CESM to simulate past warm climates

to support the development and application of data assimilation techniques in paleoclimate deep time

for high resolution spectroscopy and multi-dimensional atmospheric characterization of Hot Jupiter exoplanets.