Keith Doore
This is a likely match — the affiliation was inferred from OpenAlex, ORCID, and web sources but has not been fully confirmed. Treat with appropriate caution.
Statistician
Also affiliated: University of Northern Iowa (2015–2017); United States Geological Survey (2024–2026); Pacific Island Ecosystems Research Center (2026); Central Midwest Water Science Center (2024)
Faculty Researcher
Research Areas
Links
Biography and Research Information
OverviewAI-generated summary
Keith Doore is a statistician at the University of Arkansas at Fayetteville. His work involves the application of statistical methods to various research questions. He has been active in research and has a recent publication in 2026. His specific areas of statistical focus are not detailed in the provided information.
Metrics
- h-index: 10
- Publications: 39
- Citations: 249
Selected Publications
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SFHs of GOODS z=0-3.5 gal. with X-ray em. (2026)
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M81 post-processed results from Lightning SED fitting (2023)
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M81 post-processed results from Lightning SED fitting (2023)
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Revisiting the Properties of X-Ray Active Galactic Nuclei in the SSA22 Protocluster: Normal Supermassive Black Hole and Host-galaxy Growth for AGNs in a z = 3.09 Overdensity (2023)
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Lightning: An X-Ray to Submillimeter Galaxy SED-fitting Code with Physically Motivated Stellar, Dust, and AGN Models (2023)
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The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers (2022)
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The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields (2022)
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On the Impact of Inclination-dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields (2021)
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On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View (2021)
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On the Impact of Inclination-Dependent Attenuation on Derived Star-Formation Histories: Results from Disk Galaxies in the GOODS Fields (2021)arXiv (Cornell University) OpenAlex
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The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function (2021)
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X-ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-Mass X-ray Binaries in Galactic Fields (2020)
Collaboration Network
Top Collaborators
- The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function
- On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View
- The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields
- Revisiting the Properties of X-Ray Active Galactic Nuclei in the SSA22 Protocluster: Normal Supermassive Black Hole and Host-galaxy Growth for AGNs in a z = 3.09 Overdensity
- On the Impact of Inclination-dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
Showing 5 of 10 shared publications
- The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function
- On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View
- The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields
- Revisiting the Properties of X-Ray Active Galactic Nuclei in the SSA22 Protocluster: Normal Supermassive Black Hole and Host-galaxy Growth for AGNs in a z = 3.09 Overdensity
- On the Impact of Inclination-dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
Showing 5 of 10 shared publications
- On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View
- Revisiting the Properties of X-Ray Active Galactic Nuclei in the SSA22 Protocluster: Normal Supermassive Black Hole and Host-galaxy Growth for AGNs in a z = 3.09 Overdensity
- On the Impact of Inclination-dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
- Lightning: An X-Ray to Submillimeter Galaxy SED-fitting Code with Physically Motivated Stellar, Dust, and AGN Models
- The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
Showing 5 of 8 shared publications
- The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function
- The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields
- On the Impact of Inclination-dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
- Lightning: An X-Ray to Submillimeter Galaxy SED-fitting Code with Physically Motivated Stellar, Dust, and AGN Models
- The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
Showing 5 of 6 shared publications
- The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function
- The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields
- On the Impact of Inclination-dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
- Lightning: An X-Ray to Submillimeter Galaxy SED-fitting Code with Physically Motivated Stellar, Dust, and AGN Models
- The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
Showing 5 of 6 shared publications
- The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function
- The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields
- SFHs of GOODS z=0-3.5 gal. with X-ray em.
- The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function
- The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields
- SFHs of GOODS z=0-3.5 gal. with X-ray em.
- The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function
- The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields
- SFHs of GOODS z=0-3.5 gal. with X-ray em.
- On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View
- Revisiting the Properties of X-Ray Active Galactic Nuclei in the SSA22 Protocluster: Normal Supermassive Black Hole and Host-galaxy Growth for AGNs in a z = 3.09 Overdensity
- On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View
- Revisiting the Properties of X-Ray Active Galactic Nuclei in the SSA22 Protocluster: Normal Supermassive Black Hole and Host-galaxy Growth for AGNs in a z = 3.09 Overdensity
- On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View
- Revisiting the Properties of X-Ray Active Galactic Nuclei in the SSA22 Protocluster: Normal Supermassive Black Hole and Host-galaxy Growth for AGNs in a z = 3.09 Overdensity
- On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View
- Revisiting the Properties of X-Ray Active Galactic Nuclei in the SSA22 Protocluster: Normal Supermassive Black Hole and Host-galaxy Growth for AGNs in a z = 3.09 Overdensity
- On the Nature of AGN and Star Formation Enhancement in the z = 3.1 SSA22 Protocluster: The HST WFC3 IR View
- Revisiting the Properties of X-Ray Active Galactic Nuclei in the SSA22 Protocluster: Normal Supermassive Black Hole and Host-galaxy Growth for AGNs in a z = 3.09 Overdensity
- The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields
- SFHs of GOODS z=0-3.5 gal. with X-ray em.
- The Stellar-age Dependence of X-Ray Emission from Normal Star-forming Galaxies in the GOODS Fields
- SFHs of GOODS z=0-3.5 gal. with X-ray em.
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