Julia Kennefick Data-verified
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Biography and Research Information
OverviewAI-generated summary
Julia Kennefick's research program focuses on the study of galaxies, with a particular emphasis on spiral structures and their associated environments. Her recent publications investigate the evidence for density wave theory in star formation histories and stellar clusters, the development of novel methods for measuring spiral arm pitch angles, and the use of faint local spiral galaxies to probe the low-mass end of the black hole mass function. Kennefick also studies large-scale spiral structures within galaxies, such as a 45-kpc spiral structure observed in the GLSB galaxy UGC 4599. Her work has also touched upon the hydrosphere stability of exoplanet targets, including applications to TESS targets. She has published 111 works, which have been cited 727 times, and holds an h-index of 13. Kennefick has collaborated with researchers at the University of Arkansas at Fayetteville, including Daniel Kennefick and Michael Fusco.
Metrics
- h-index: 14
- Publications: 112
- Citations: 762
Selected Publications
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The haloes and environments of nearby galaxies (<i>HERON</i>) – III. A 45-kpc spiral structure in the GLSB galaxy UGC 4599 (2023)
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Probing the Low-Mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies (2022)
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On the Hydrosphere Stability of TESS Targets: Applications to 700 d, 256 b, and 203 b (2022)
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Physical Characteristics and Classification of the Large Amplitude Variable Star V1719 Cygni (2022)
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Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters (2022)
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Spirality: A Novel Way to Measure Spiral Arm Pitch Angle (2022)
Collaboration Network
Top Collaborators
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- The haloes and environments of nearby galaxies (<i>HERON</i>) – III. A 45-kpc spiral structure in the GLSB galaxy UGC 4599
- Testing density wave theory using multi-wavelength image data and stellar cluster dynamics
- The haloes and environments of nearby galaxies (HERON) -- III. A 45 kpc spiral structure in the GLSB galaxy UGC 4599
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Probing the Low-Mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies
- Testing density wave theory using multi-wavelength image data and stellar cluster dynamics
- Probing the Low-mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Probing the Low-Mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies
- Probing the Low-mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies
- Probing the Low-Mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies
- The haloes and environments of nearby galaxies (<i>HERON</i>) – III. A 45-kpc spiral structure in the GLSB galaxy UGC 4599
- Probing the Low-mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies
- The haloes and environments of nearby galaxies (HERON) -- III. A 45 kpc spiral structure in the GLSB galaxy UGC 4599
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Probing the Low-Mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies
- Probing the Low-mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies
- The haloes and environments of nearby galaxies (<i>HERON</i>) – III. A 45-kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (HERON) -- III. A 45 kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (<i>HERON</i>) – III. A 45-kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (HERON) -- III. A 45 kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (<i>HERON</i>) – III. A 45-kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (HERON) -- III. A 45 kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (<i>HERON</i>) – III. A 45-kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (HERON) -- III. A 45 kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (<i>HERON</i>) – III. A 45-kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (HERON) -- III. A 45 kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (<i>HERON</i>) – III. A 45-kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (HERON) -- III. A 45 kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (<i>HERON</i>) – III. A 45-kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (HERON) -- III. A 45 kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (<i>HERON</i>) – III. A 45-kpc spiral structure in the GLSB galaxy UGC 4599
- The haloes and environments of nearby galaxies (HERON) -- III. A 45 kpc spiral structure in the GLSB galaxy UGC 4599
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