K. Honscheid
Physics and Astronomy · The Ohio State University
Publications
1,000
Citations
57,064
Est. group size
~14
Recurring co-author estimate
Active years
36
Publishing since 1991
K. Honscheid works in experimental physics and astronomy, contributing to large collaborative projects that study the universe's large-scale structure and fundamental particle interactions. Their work spans galaxy surveys mapping dark energy and cosmic structure (such as DESI and the Dark Energy Survey) as well as particle physics experiments (such as BABAR) probing rare particle decays, dark matter, and matter-antimatter asymmetry. Publications typically appear as part of large multi-author collaboration papers reporting instrument results, survey catalogs, and precision measurements.
Publication output has grown over the past decade, rising from around 36 papers per year in 2017 to a peak of about 90 in 2023, with high but slightly declining counts in the most recent years.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- DESI Data Release 1: Stellar Catalogue
The Open Journal of Astrophysics · 2026
- Dark Energy Survey: DESI-Independent Angular BAO Measurement
HAL (Le Centre pour la Communication Scientifique Directe) · 2026
- Galaxy-galaxy strong lens cand. from DELVE
Strasbourg Astronomical Data Center · 2026
- Year six photometric measurements of known Trans-Neptunian Objects and Centaurs by the Dark Energy Survey
Monthly Notices of the Royal Astronomical Society · 2025
- HEPAP Facilities Subpanel Report
2024
- A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55
The Astrophysical Journal · 2024
- Model-independent extraction of form factors and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mrow><mml:mi>c</mml:mi><mml:mi>b</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo></mml:math> in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mover accent="true"><mml:mi>B</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mo stretchy="false">→</mml:mo><mml:mi>D</mml:mi><mml:msup><mml:mo>ℓ</mml:mo><mml:mo>−</mml:mo></mml:msup><mml:msub><mml:mover accent="true"><mml:mi>ν</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mo>ℓ</mml:mo></mml:msub></mml:math> with hadronic tagging at <i>BABAR</i>
Physical review. D/Physical review. D. · 2024
- Copacabana: A Probabilistic Membership Assignment Method for Galaxy Clusters
arXiv (Cornell University) · 2024
- Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel’dovich effect with SPT-3G and DES
Physical review. D/Physical review. D. · 2023
- Identification of Galaxy–Galaxy Strong Lens Candidates in the DECam Local Volume Exploration Survey Using Machine Learning
The Astrophysical Journal · 2023
- Synchronous Rotation in the (136199) Eris–Dysnomia System
The Planetary Science Journal · 2023
- Mitigating the noise of DESI mocks using analytic control variates
The Open Journal of Astrophysics · 2023
- Measurement of additional radiation in the initial-state-radiation processes <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mi>e</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>e</mml:mi><mml:mo>−</mml:mo></mml:msup><mml:mo stretchy="false">→</mml:mo><mml:msup><mml:mi>μ</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>μ</mml:mi><mml:mo>−</mml:mo></mml:msup><mml:mi>γ</mml:mi></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mi>e</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>e</mml:mi><mml:mo>−</mml:mo></mml:msup><mml:mo stretchy="false">→</mml:mo><mml:msup><mml:mi>π</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mo>−</mml:mo></mml:msup><mml:mi>γ</mml:mi></mml:math> at <i>BABAR</i>
Physical review. D/Physical review. D. · 2023
- Search for Evidence of Baryogenesis and Dark Matter in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>B</mml:mi></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup><mml:mo stretchy="false">→</mml:mo><mml:msub><mml:mrow><mml:mi>ψ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="italic">D</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="italic">p</mml:mi></mml:mrow></mml:math> Decays at <i>BABAR</i>
Physical Review Letters · 2023
- Study of the reactions <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mi>e</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>e</mml:mi><mml:mo>−</mml:mo></mml:msup><mml:mo stretchy="false">→</mml:mo><mml:msup><mml:mi>K</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>K</mml:mi><mml:mo>−</mml:mo></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mn>0</mml:mn></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mn>0</mml:mn></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mn>0</mml:mn></mml:msup></mml:math>, <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mi>e</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>e</mml:mi><mml:mo>−</mml:mo></mml:msup><mml:mo stretchy="false">→</mml:mo><mml:msubsup><mml:mi>K</mml:mi><mml:mi>S</mml:mi><mml:mn>0</mml:mn></mml:msubsup><mml:msup><mml:mi>K</mml:mi><mml:mo>±</mml:mo></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mo>∓</mml:mo></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mn>0</mml:mn></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mn>0</mml:mn></mml:msup></mml:math>, and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mi>e</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>e</mml:mi><mml:mo>−</mml:mo></mml:msup><mml:mo stretchy="false">→</mml:mo><mml:msubsup><mml:mi>K</mml:mi><mml:mi>S</mml:mi><mml:mn>0</mml:mn></mml:msubsup><mml:msup><mml:mi>K</mml:mi><mml:mo>±</mml:mo></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mo>∓</mml:mo></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mo>−</mml:mo></mml:msup></mml:math> at center-of-mass energies from threshold to 4.5 GeV using initial-state radiation
Physical review. D/Physical review. D. · 2023
- Monthly Notices of the Royal Astronomical Society×187
- arXiv (Cornell University)×82
- Physical review. D/Physical review. D.×51
- The Astrophysical Journal×45
- The Astronomical Journal×27
- R. Miquel
Physics and Astronomy · The Ohio State University
- Paul Martini
Physics and Astronomy · The Ohio State University
- K. Honscheid
Physics and Astronomy · The Ohio State University
- Kyoung-Soo Lee
Physics and Astronomy · Purdue University West Lafayette
- M. Lima
Physics and Astronomy · The Ohio State University
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 19, 2026.
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