Hui Kong

Physics and Astronomy · The Ohio State University

Early career · publishing since 2020

Galaxies: Formation, Evolution, Phenomena Astronomy and Astrophysical Research Cosmology and Gravitation Theories Gamma-ray bursts and supernovae Stellar, planetary, and galactic studies

Publications

Citations

667

Est. group size

Recurring co-author estimate

Active years

Publishing since 2020

Research summary

AI-generated

Hui Kong works in observational cosmology, using large galaxy surveys such as SDSS/eBOSS and DESI to measure the large-scale structure of the universe, including baryon acoustic oscillations (a standard 'ruler' distance measurement) and the growth rate of cosmic structure, which help test theories of gravity and the composition of the universe. Much of the work involves correcting for imaging and observational systematics that could bias these clustering measurements.

Galaxy clustering and large-scale structureBaryon acoustic oscillations (BAO)Tests of gravity using galaxy surveysImaging systematics correction in survey dataEmission line galaxy samples (SDSS/eBOSS/DESI)

Publication output was minimal before 2020, then rose sharply in 2020 with a cluster of survey papers, dipped to about one per year from 2021-2023, and increased again in 2024-2025, suggesting an uneven but currently active publication pace.

Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026

Publication cadence

Publications per year over the last 10 years — averaging 1.6/year recently

Recent publications

Mitigating imaging systematics for DESI 2024 emission Line Galaxies and beyond
Journal of Cosmology and Astroparticle Physics · 2025
Probing gravity with the DES-CMASS sample and BOSS spectroscopy
LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) · 2022
Probing gravity with the DES-CMASS sample and BOSS spectroscopy
Monthly Notices of the Royal Astronomical Society · 2021
The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
Monthly Notices of the Royal Astronomical Society · 2020
The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: large-scale structure catalogues and measurement of the isotropic BAO between redshift 0.6 and 1.1 for the Emission Line Galaxy Sample
Monthly Notices of the Royal Astronomical Society · 2020
Removing imaging systematics from galaxy clustering measurements with <tt>Obiwan</tt>: application to the SDSS-IV extended Baryon Oscillation Spectroscopic Survey emission-line galaxy sample
Monthly Notices of the Royal Astronomical Society · 2020

Publishes in

Monthly Notices of the Royal Astronomical Society×5
Journal of Cosmology and Astroparticle Physics×4
arXiv (Cornell University)×2
LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas)×1
eScholarship (California Digital Library)×1

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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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