Reduced IGRINS spectra: Taurus-Auriga

This Dataset contains the averaged (over n epochs) H- and K-band IGRINS spectra of the sample of Taurus-Auriga YSOs used in López-Valdivia et al. (2021). The spectra presented are a telluric corrected spectrum with wavelength solutions derived from OH night sky emission lines at shorter wavelengths and telluric absorption lines at wavelengths greater than 2.2 μm. The number of epochs averaged for each object could be check-in the header key "N_SPECS". The name in the files is the 2MASS identification number, but we also provided the names.txt file with alternative names for all the sample. The average spectrum of each band is stored in FITS files with dimensions of 2048 px by 28 and 26 spectral orders in the H- and K-band, respectively. Every spectral order contains 4 different axes containing: No. Description 0 Final telluric corrected spectrum 1 Wavelength 2 Flux uncertainty 3 Signal-to-noise ratio