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OBSERVATORIES & FACILITIES

Connecting supermassive black hole accretion to galaxy evolution across spatial scales

I use multiwavelength observations from space- and ground-based facilities to study AGN feedback and its role in galaxy evolution.

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Observatories & Facilities

I combine observations across the electromagnetic spectrum to study how active galactic nuclei (AGN) interact with and shape their host galaxies.

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Chandra X-ray Observatory

X-rays

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Hubble Space
Telescope

Optical/UV

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James Webb
Space Telescope

Infrared

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Atacama Large Millimiter Array
(ALMA)

Millimiter

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Very Large Array
(VLA)

Radio

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MUSE

IFU Spectroscopy

Tracing hot gas, AGN emission, and high-energy processes in galactic nuclei.
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Chandra X-ray Observatory

Hubble Space Telescope (HST)

High-resolution optical and ultraviolet imaging and spectroscopy of galaxy structure and ionized gas.
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James Webb Space Telescope (JWST)

Infrared observations probing dust-obscured regions and early stages of galaxy evolution.

Atacama Large Millimiter Array (ALMA)

Mapping cold molecular gas and star-forming regions at high spatial resolution.
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Very Large Array (VLA)

Tracing radio emission from jets, synchrotron processes, and large-scale outflows.

MUSE

Spatially resolved spectroscopy of ionized gas, mapping kinematics and excitation across galaxies.
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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.

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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.

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