Observatories & Facilities
I combine observations across the electromagnetic spectrum to study how active galactic nuclei (AGN) interact with and shape their host galaxies.
X-rays
Optical/UV
Infrared
Millimiter
Radio
IFU Spectroscopy
X-ray observations tracing hot gas, AGN emission, and high-energy processes in galactic nuclei.
Chandra X-ray Observatory
Hubble Space Telescope (HST)
High-resolution optical and ultraviolet imaging of galaxy structure and ionized gas.
James Webb Space Telescope (JWST)
Infrared observations probing dust-obscured regions and early stages of galaxy evolution.
Atacama Large Millimiter Array (ALMA)
Millimeter observations mapping cold molecular gas and star-forming regions at high spatial resolution.
Very Large Array (VLA)
Radio observations tracing jets, synchrotron emission, and large-scale AGN outflows.
MUSE
Integral field spectroscopy mapping ionized gas kinematics and excitation across galaxies.
Techniques
Spatially resolved spectroscopy
X-ray imaging and spectral analysis
Photoionization modeling
Multiwavelength
data integration
Multiwavelength Observations
From X-rays to radio, probing gas from parsec to kiloparsec scales.
Physical Modeling
Spectral and photoionization modeling to interpret observations.
Galaxy Evolution
Understanding how AGN feedback shapes galaxies over cosmic time.
Collaborations
International collaborations across observatories and research teams.
RESEARCH APPROACH
Connecting supermassive black hole accretion to galaxy evolution across spatial scales
I combine high-resolution imaging, spectroscopy, and modeling to study how energy released by active galactic nuclei shapes their host galaxies.