Kelley Michelle Hess
I am the Scientific Lead for the Swedish SKA Regional Center (SWE-SRC). My research interests are in environmentally-driven galaxy evolution, especially in the group and cluster environment. I'm an expert in extragalactic radio astronomy, but study galaxies, groups, and clusters from a multi-wavelength perspective. I'm a member of several small to large collaborations including CHILES, Apertif, WEAVE-Apertif, LADUMA, WALLABY, 4HS. I have also occasionally dabbled in OH megamasers, barred galaxies, extraplanar gas in galaxies. I contribute to developing software tools for spectral line surveys including leading the SoFiA Image Pipeline, and an Advanced Data Product pipeline for ALMA (under development).
Showing 33 publications
MeerKAT view of Hickson Compact Groups II. Hi deficiency in the cores and surrounding regions
MeerKAT view of Hickson Compact Groups I. Data description and release
WALLABY Pilot Survey: KNN identification of perturbed galaxies through H i morphometrics
The RESOLVE and ECO G3 Initiative: Drivers of H i Content and X-Ray Emission in Galaxy Groups
AMUSE-Antlia. II. Intracluster X-Ray Population in the Antlia Cluster
WEAVE First Light Observations: Origin and Dynamics of the Shock Front in Stephan's Quintet
The discovery of a z = 0.7092 OH megamaser with the MIGHTEE survey
The AMIGA sample of isolated galaxies - effects of environment on angular momentum
Photometry and kinematics of dwarf galaxies from the Apertif H i survey
Formation of a Massive Lenticular Galaxy Under the Tidal Interaction with a Group of Dwarf Galaxies
SKA Science Data Challenge 2: analysis and results
Apertif 1.4 GHz continuum observations of the Boötes field and their combined view with LOFAR
Seeing the forest and the trees: A radio investigation of the ULIRG Mrk 273
Apercal - The Apertif calibration pipeline
Characterising the Apertif primary beam response
First release of Apertif imaging survey data
The Apertif science verification campaign: Characteristics of polarised radio sources
Apertif view of the OH megamaser IRAS 10597+5926: OH 18 cm satellite lines in wide-area H i surveys
A search for radio emission from double-neutron star merger GW190425 using Apertif
Chromatic periodic activity down to 120 megahertz in a fast radio burst
Repeating fast radio bursts with WSRT/Apertif
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