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Seong-Kook Lee

Identifiers

  • name variant Seong-Kook Lee 0.60 · backfill

Papers (24)

  1. ODIN: Clustering Properties of Ly$\alpha$ Blobs at $z$ $\sim$ 2.4 and 3.1 astro-ph.GA · 2026 · author #18
  2. ODIN: A New Lyman Alpha Blob Selection Method, Sample, and Statistical Analysis at $z\sim3.1$ astro-ph.GA · 2025 · author #23
  3. ODIN: Characterizing the Three-dimensional Structure of Two Protocluster Complexes at $z = 3.1$ astro-ph.GA · 2025 · author #33
  4. Observational evidence for bar formation in disk galaxies via cluster-cluster interaction astro-ph.GA · 2019 · author #4
  5. The Infrared Medium-deep Survey. VI. Discovery of Faint Quasars at $z\sim5$ with a Medium-band-based Approach astro-ph.GA · 2018 · author #18
  6. The Infrared Medium-deep Survey. IV. Low Eddington Ratio of A Faint Quasar at $z\sim6$: Not Every Supermassive Black Hole is Growing Fast in the Early Universe astro-ph.GA · 2018 · author #16
  7. Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0 astro-ph.GA · 2017 · author #23
  8. The Infrared Medium-deep Survey. III. Survey of Luminous Quasars at 4.7 $\leq$ z $\leq$ 5.4 astro-ph.GA · 2017 · author #21
  9. CANDELS Sheds Light on the Environmental Quenching of Low-mass Galaxies astro-ph.GA · 2017 · author #8
  10. CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip astro-ph.GA · 2017 · author #10
  11. Relations Between the Sizes of Galaxies and their Dark Matter Halos at Redshifts $0 < z < 3$ astro-ph.GA · 2017 · author #7
  12. The evolution of star formation histories of quiescent galaxies astro-ph.GA · 2016 · author #22
  13. Evolution of Intrinsic Scatter in the SFR-Stellar Mass Correlation at 0.5<z<3 astro-ph.GA · 2016 · author #14
  14. Satellite Quenching and Galactic Conformity at 0.3 < z < 2.5 astro-ph.GA · 2015 · author #17
  15. Discovery of A Faint Quasar at z~6 and Implications for Cosmic Reionization astro-ph.GA · 2015 · author #14
  16. Evolution of Star-formation Properties of High-redshift Cluster Galaxies since $z = 2$ astro-ph.GA · 2015 · author #1
  17. Host Galaxy Properties and Black Hole Mass of Swift J164449.3+573451 from Multi-Wavelength Long-Term Monitoring and HST Data astro-ph.GA · 2015 · author #4
  18. The Evolution of the Galaxy Stellar Mass Function at z= 4-8: A Steepening Low-mass-end Slope with Increasing Redshift astro-ph.GA · 2015 · author #17
  19. The AKARI 2.5-5.0 Micron Spectral Atlas of Type-1 Active Galactic Nuclei: Black Hole Mass Estimator, Line Ratio, and Hot Dust Temperature astro-ph.GA · 2015 · author #14
  20. The Infrared Medium-Deep Survey II: How to Trigger Radio-AGN? Hints from Their Environments astro-ph.GA · 2014 · author #4
  21. Steadily Increasing Star Formation Rates in Galaxies Observed at 3 <~ z <~ 5 in the CANDELS/GOODS-S Field astro-ph.GA · 2014 · author #1
  22. Survey design for Spectral Energy Distribution fitting: a Fisher Matrix approach astro-ph.CO · 2012 · author #6
  23. Improving the Estimation of Star formation Rates and Stellar Population Ages of High-redshift Galaxies from Broadband Photometry astro-ph.CO · 2010 · author #1
  24. A Detailed Study of Photometric Redshifts for GOODS-South Galaxies astro-ph.CO · 2010 · author #10

Mentions

  • 2511.11826 #33 · arxiv_oai · confidence 0.70 Seong-Kook Lee
  • 1511.02862 #17 · backfill · confidence 0.70 Seong-Kook Lee
  • 1511.01585 #14 · backfill · confidence 0.70 Seong-Kook Lee
  • 1508.01294 #1 · backfill · confidence 0.70 Seong-Kook Lee
  • 1507.08843 #4 · backfill · confidence 0.70 Seong-Kook Lee
  • 1507.05636 #17 · backfill · confidence 0.70 Seong-Kook Lee
  • 1503.04925 #14 · backfill · confidence 0.70 Seong-Kook Lee
  • 1410.4200 #4 · backfill · confidence 0.70 Seong-Kook Lee
  • 1403.6198 #1 · backfill · confidence 0.70 Seong-Kook Lee
  • 2601.01991 #18 · arxiv_oai · confidence 0.70 Seong-Kook Lee
  • 2512.17368 #23 · arxiv_oai · confidence 0.70 Seong-Kook Lee
  • 1201.1012 #6 · backfill · confidence 0.70 Seong-Kook Lee
  • 1010.1966 #1 · backfill · confidence 0.70 Seong-Kook Lee
  • 1009.3504 #10 · backfill · confidence 0.70 Seong-Kook Lee

Frequent Coauthors