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researcher

Jae-Woo Lee

35 papers hereh-index 18966 citations53 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author14
  • first author9
  • middle author7
  • last author3

Across the 33 of 35 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA22
  • astro-ph8
  • astro-ph.SR3
  • astro-ph.EP1
  • astro-ph.HE1
same name
  • Jae-Woo Lee — 1 paper, h 5
  • Jae-Woo Lee — 1 paper, h 4
  • Jae-Woo Lee — 1 paper, h 10
  • Jae-Woo Lee — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20022025
most citedEnrichment by supernovae in globular clusters with multiple populations

161 citations · 1k across the 34 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2020★ 13 cited

Multiple Stellar Populations of Globular Clusters from Homogeneous Ca-CN-CH-NH Photometry. VI. M3 (NGC 5272) is not a Prototypical Normal Globular Cluster

Jae-Woo Lee, Christopher Sneden

We present Ca-CN-CH-NH photometry for the well-known globular cluster (GC) M3 (NGC 5272). We show new evidence for two M3 populations with distinctly different carbon and nitrogen…

astro-ph.SR2015★ 17 cited

The Distances to Open Clusters from Main-Sequence Fitting. V. Extension of Color Calibration and Test using Cool and Metal-Rich Stars in NGC 6791

Deokkeun An, Donald M. Terndrup, Marc H. Pinsonneault +1

We extend our effort to calibrate stellar isochrones in the Johnson-Cousins (BVIC​) and the 2MASS (JHKs​) filter systems based on observations of well-studied open clusters. Us…

astro-ph.SR2013★ 77 cited

The RR Lyrae variables and Horizontal Branch of NGC6656 (M22)

Andrea Kunder, Peter B. Stetson, Santi Cassisi +10

The first calibrated broadband UBVI time-series photometry is presented for the RR Lyrae variable stars in NGC6656 (M22), with observations spanning a range of twenty-two years. We…

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