I'm interested in many topics related to galaxy evolution, particularly through studies of distant galaxies. I have used imaging and spectroscopy from a range of ground- and space-based telescopes to study the structures, kinematics, and dust content of galaxies at z~1-3, and more recently pushing to earlier times.
My work has included analysis of large samples to characterize the properties of galaxy populations over time, as well as investigations of individual galaxies using detailed spatially- and spectrally-resolved observations. I have carried out this work as a leader in and a member of multiple surveys, and have also led and contributed to development efforts of analysis tools to model and interpret these observations.
JWST Cycle 5 medium program obtaining 5.6-18um MIRI imaging in the cluster Abell 2744, to reveal the impact of dust obscuration of galaxies and black holes over most of cosmic time (PIs: Price, Whitaker, Bezanson)
JWST Cycle 4 large program taking NIRCAM medium band and MIRI imaging in the UDS, COSMOS, AEGIS, and GOODS-N fields, to study detailed galaxy SEDs across most of cosmic time
JWST Cycle 1 Treasury survey taking ultradeep NIRCam/NIRISS imaging and NIRSpec PRISM spectroscopy of the cluster Abell 2744, to study galaxies from the epoch of reionization out to cosmic dawn
JWST Cycle 2 GO program with ultradeep medium band imaging across Abell 2744, to do spatially-resolved R~15 spectrophotometry of 50,000 sources across the history of the universe
JWST Cycle 2 GO program with prism and medium resolution spectra of red, JWST-selected targets in the UDS and EGS fields
JWST Cycle 1 GO program studying chemical abundances and stellar kinematics of quiescent galaxies at 1.0 < z < 2.5 using ultra-deep medium resolution (R~1000) NIRSpec continuum spectroscopy
Keck/LRIS and MOSFIRE survey using ultradeep rest-frame optical spectroscopy to study the chemical composition and stellar kinematics of 20 massive quiescent galaxies at z~1.3-2.3
ALMA Cycle 8 Large Program constraining the gas, dust, and stars in 19 "normal" star-forming galaxies at z~4-5 on kpc scales by combining observations with ALMA, HST, JWST, and VLT
ALMA Cycle 9 program establishing a joint ALMA and JWST public legacy field with contiguous Band 6 (~1.2mm) coverage over the extended Abell 2744 cluster field
MIOP IRAM/NOEMA survey studing star formation, feedback, and quenching using the molecular gas distribution and kinematics in ~50 massive star-forming galaxies out to cosmic noon
VLT/KMOS GTO survey using IFU spectroscopy to take a census of the spatially-resolved kinematics, star formation, outflows, and nebular gas conditions in more than 700 star-forming galaxies at z~1-3
Keck/MOSFIRE large program combining multiband rest-frame optical spectroscopy with HST imaging (from 3D-HST & CANDELS) to probe the stars, gas, metals, dust, and AGN in ~1500 galaxies at z~1.5-3
HST Cycle 28 & 29 Treasury program that obtained low spectral resolution slitless grism spectra in four of the CANDELS extragalactic fields, with redshifts and emission line fluxes for ~100,000 galaxies
Galaxy dynamical modeling in 1D, 2D, or 3D using mass-based circular motions, non-circular motions, and pressure support (see, e.g., Price et al. 2021, Lee et al., 2025)
Package to calculate various profiles for deprojected, axisymmetric Sérsic mass distributions (Price et al. 2022)
Kinematic modeling for spectra taken with misaligned slits, as described in Price et al. 2016