S. Lee

ORCID: 0000-0001-6034-2238
Publications
Citations
Views
---
Saved
---
About
Contact & Profiles
Research Areas
  • Pulsars and Gravitational Waves Research
  • Gamma-ray bursts and supernovae
  • Astrophysical Phenomena and Observations
  • High-pressure geophysics and materials
  • Dark Matter and Cosmic Phenomena
  • Cosmology and Gravitation Theories
  • Astrophysics and Star Formation Studies
  • Advanced Frequency and Time Standards
  • Geophysics and Gravity Measurements
  • Magnetic confinement fusion research
  • Superconducting Materials and Applications
  • Stellar, planetary, and galactic studies
  • Galaxies: Formation, Evolution, Phenomena
  • earthquake and tectonic studies
  • Geophysics and Sensor Technology

Korea Astronomy and Space Science Institute
2005-2024

Seoul National University
2005

Abstract The Immersion GRating INfrared Spectrometer (IGRINS) is a compact, high-resolution ( R ∼ 45,000) near-infrared spectrograph spanning 1.45–2.45 μ m in single exposure. We introduce the Raw and Reduced IGRINS Spectral Archive (RRISA), which provides public data access for all non-proprietary taken at McDonald Observatory's Harlan J. Smith Telescope, Lowell Discovery Telescope (formerly Channel Telescope), Gemini South. RRISA to raw files, reduced products, cross-matched targets with...

10.1088/1538-3873/adba89 article EN cc-by Publications of the Astronomical Society of the Pacific 2025-03-01

We observed Hubble V, the brightest HII region complex in dwarf irregular galaxy NGC 6822, at near-infrared (1.8--2.4 um) wavelengths using Cooled Grating Spectrometer 4 (CGS4) United Kingdom Infra-Red Telescope (UKIRT). The line emission maps of V show typical structure a photo-dissociation (PDR) where an ionized core, traced by compact He I (2.0587 and Br_gamma (2.1661 um), is surrounded outer layer molecular hydrogen (H_2) emission. measured ratios H_2 2-1 S(1) (2.2477 / 1-0 (2.1218 from...

10.1111/j.1365-2966.2005.09259.x article EN Monthly Notices of the Royal Astronomical Society 2005-08-03
Coming Soon ...