Daniel Kennefick Data-verified
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Biography and Research Information
OverviewAI-generated summary
Daniel Kennefick is a professor at the University of Arkansas at Fayetteville. His research focuses on astrophysics, with a particular emphasis on gravitational waves and the study of celestial objects such as black holes and spiral galaxies. He has published work investigating gravitational wave signals from extreme mass ratio inspirals (EMRIs) and their implications for signal confusion noise in space-based observatories like LISA.
Kennefick's work also explores methods for measuring galactic properties, including the pitch angle of spiral arms. His research group studies the low-mass end of the black hole mass function by examining faint local spiral galaxies. He has also engaged in historical scholarship concerning early work on equations of motion and gravitational radiation.
Kennefick's scholarly contributions are reflected in his h-index of 23 and over 3,000 citations across 134 publications. He collaborates with researchers at the University of Arkansas, including Julia Kennefick, Daniel J Oliver, D. W. Shields, and Michael Fusco, with whom he shares multiple publications.
Metrics
- h-index: 23
- Publications: 134
- Citations: 3,163
Selected Publications
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Gravitational wave peep contributions to background signal confusion noise for LISA (2026)
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Gravitational wave peep contributions to background signal confusion noise for LISA (2026)
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A contextual analysis of the early work of Andrzej Trautman and Ivor Robinson on equations of motion and gravitational radiation (2025)
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Gravitational wave peeps from EMRIs and their implication for LISA signal confusion noise (2024)
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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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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
- 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
- Gravitational wave peeps from EMRIs and their implication for LISA signal confusion noise
- Gravitational wave peep contributions to background signal confusion noise for LISA
- Gravitational Wave Peeps from EMRIs and their Implication for LISA Signal Confusion Noise
- Gravitational wave peep contributions to background signal confusion noise for LISA
- Gravitational wave peeps from EMRIs and their implication for LISA signal confusion noise
- Gravitational wave peep contributions to background signal confusion noise for LISA
- Gravitational Wave Peeps from EMRIs and their Implication for LISA Signal Confusion Noise
- Gravitational wave peep contributions to background signal confusion noise for LISA
- Gravitational wave peeps from EMRIs and their implication for LISA signal confusion noise
- Gravitational wave peep contributions to background signal confusion noise for LISA
- Gravitational Wave Peeps from EMRIs and their Implication for LISA Signal Confusion Noise
- Gravitational wave peep contributions to background signal confusion noise for LISA
- 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
- Testing density wave theory using multi-wavelength image data and stellar cluster dynamics
- Gravitational wave peeps from EMRIs and their implication for LISA signal confusion noise
- Gravitational wave peep contributions to background signal confusion noise for LISA
- Gravitational Wave Peeps from EMRIs and their Implication for LISA Signal Confusion Noise
- 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
- 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
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
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