IGRINS Spectral Library

  • Park, Sunkyung (School of Space Research, Kyung Hee University) ;
  • Lee, Jeong-Eun (School of Space Research, Kyung Hee University) ;
  • Kang, Wonseok (National Youth Space Center) ;
  • Lee, Sang-Gak (National Youth Space Center) ;
  • Chun, Moo-Young (Korea Astronomy and Space Science Institute) ;
  • Kim, Kang-Min (Korea Astronomy and Space Science Institute) ;
  • Yuk, In-Soo (Korea Astronomy and Space Science Institute) ;
  • Lee, Jae-Joon (Korea Astronomy and Space Science Institute) ;
  • Mace, Gregory N. (Department of Astronomy, University of Texas at Austin) ;
  • Kim, Hwihyun (Korea Astronomy and Space Science Institute) ;
  • Kaplan, Kyle F. (Department of Astronomy, University of Texas at Austin) ;
  • Jaffe, Daniel T. (Department of Astronomy, University of Texas at Austin)
  • Published : 2016.10.12

Abstract

We present a library of high-resolution (R~45,000) and high signal-to-noise ratio ($S/N{\geq}200$) near-infrared spectra of 147 standard stars. High quality spectra were obtained with Immersion GRating INfrared Spectrograph (IGRINS) covering the full range of H ($1.496-1.795{\mu}m$) and K ($2.080-2.460{\mu}m$) bands. The targets are mainly selected as MK standard stars which have well-defined spectral types and luminosity classes, and cover a wide range of effective temperatures and surface gravities. The spectra were corrected for telluric absorption lines and absolute flux calibrated using Two Micron All Sky Survey (2MASS) photometry. We find new spectral indices in H and K bands and provide their EWs. We describe empirical relations between the measured EWs and stellar atmosphere parameters such as effective temperature and surface gravity.

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