Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011jkas...44..125h&link_type=abstract
Journal of the Korean Astronomical Society, vol. 44, no. 4, pp. 125-134
Astronomy and Astrophysics
Astronomy
Stars: Late-Type, Methods: Observational, Methods: Data Analysis
Scientific paper
We present medium resolution (R = 5000-6000) spectra in the near-infrared band, 1.4-1.8 μm, for template stars in G, K, and M types observed by the echelle spectrometer, IRCS, at the SUBARU 8.2 m telescope. The identification of lines is based on the spectra of Arcturus (K2 III) in the literature. We measured the equivalent of widths and compared our results to those of Meyer et al. (1998). We conclude that our spectral resolution (R = 6000) data can investigate more accurately the properties of lines in stellar spectra. The library of the template stellar spectra in ASCII format are available for download on the World Wide Web.
Daniel Jaffe T.
Ho Luis C.
Huynh Anh Nguyen Le
Im Myungshin
Kang Wonseok
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