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 (2025–2026); Central Midwest Water Science Center (2024–2026)
Research Areas
Links
Biography and Research Information
OverviewAI-generated summary
Keith Doore's research primarily focuses on astrophysics, with a particular emphasis on X-ray astronomy and the study of celestial objects such as X-ray binaries and active galactic nuclei (AGN). His work investigates the luminosity functions of these objects and how they scale with galactic properties, including metallicity and stellar age. Doore has examined the relationship between AGN activity and star formation in protoclusters at high redshifts, utilizing data from instruments like the Hubble Space Telescope. His publications also touch upon the electronic properties of materials, such as the Au/MoS2 junction, and the development of computational tools for scientific analysis, including the Python package 'Ratingcurve' for fitting streamflow rating curves. Doore's scholarly contributions are reflected in his h-index of 10 and over 250 citations.
Metrics
- h-index: 10
- Publications: 34
- Citations: 252
Positions
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Statistician 2025–presentFederal Emergency Management Agency ORCID
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Statistician publications 2020–2026University of Arkansas at Fayetteville ORCID
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Data Scientist 2023–2025US Geological Survey ORCID
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Graduate Assistant 2017–2023University of Arkansas Physics ORCID
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
- X-ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-Mass X-ray Binaries in Galactic Fields
- 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
Showing 5 of 11 shared publications
- The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function
- X-ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-Mass X-ray Binaries in Galactic Fields
- 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
Showing 5 of 11 shared publications
- X-ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-Mass X-ray Binaries in Galactic Fields
- 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
Showing 5 of 9 shared publications
- The Metallicity Dependence of the High-mass X-Ray Binary Luminosity Function
- X-ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-Mass X-ray Binaries in Galactic Fields
- 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
Showing 5 of 7 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
- X-ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-Mass X-ray Binaries in Galactic Fields
- 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.
- X-ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-Mass X-ray Binaries in Galactic Fields
- 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.
- X-ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-Mass X-ray Binaries in Galactic 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
- 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
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