Jerome John Seebeck | University of Maryland: Department of Astronomy

Jerome John Seebeck

Hear my name:

Graduate Student

jseebeck@umd.edu 1113 Physical Sciences Complex

My research is focused on observing the feedback effects of active galactic nuclei (AGN) on their host galaxies. I primarily work with data from the James Webb Space Telescope Mid-Infrared Instrument. I completed my undergraduate at Caltech working on fast radio bursts (FRBs) and young stellar objects (YSOs).

Research Areas:

Galaxies

Latest Papers

Resolving the Multiphase Outflow, Shock Signatures, and PAHs in the AGN-starburst Composite ULIRG F10565+2448 with JWST MIRI/MRS

June 10, 2026 | The Astrophysical Journal
Author(s): Kylie Yui Dan, Jerome Seebeck, Sylvain Veilleux, et. al
UMD Author(s): Jerome John Seebeck

JWST Discovery of High-velocity Mid-infrared Ionized Outflows in Ultraluminous Infrared Galaxies F11119+3257 and F05189-2524

March 1, 2026 | The Astrophysical Journal
Author(s): Jerome Seebeck, Kylie Yui Dan, Sylvain Veilleux, et. al
UMD Author(s): Jerome John Seebeck

Directly imaging the cooling flow in the Phoenix cluster

February 13, 2025 | Nature
Author(s): Michael Reefe, Michael McDonald, Marios Chatzikos, et. al
UMD Author(s): Richard Mushotzky, Jerome John Seebeck

JWST Discovery of a Very Fast Biconical Outflow of Warm Molecular Gas in the Nearby Ultraluminous Infrared Galaxy F08572+3915 NW

January 20, 2025 | The Astrophysical Journal
Author(s): Kylie Yui Dan, Jerome Seebeck, Sylvain Veilleux, et. al
UMD Author(s): Jerome John Seebeck

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Latest Papers

Resolving the Multiphase Outflow, Shock Signatures, and PAHs in the AGN-starburst Composite ULIRG F10565+2448 with JWST MIRI/MRS

JWST Discovery of High-velocity Mid-infrared Ionized Outflows in Ultraluminous Infrared Galaxies F11119+3257 and F05189-2524

Directly imaging the cooling flow in the Phoenix cluster

JWST Discovery of a Very Fast Biconical Outflow of Warm Molecular Gas in the Nearby Ultraluminous Infrared Galaxy F08572+3915 NW

Combined JWST–MUSE Integral Field Spectroscopy of the Most Luminous Quasar in the Local Universe, PDS 456

An Expanding Accretion Disk and a Warm Disk Wind as Seen in the Spectral Evolution of HBC 722

Disk Cooling and Wind Lines as Seen in the Spectral Line Evolution of V960 Mon

The time-variable temperature profile in the inner disk of V960 Mon

The Effects of Selection Biases on the Analysis of Localised Fast Radio Bursts

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