One-dimensional reduced optical stellar spectra obtained at the Three College
Observatory (TCO) with the eShel spectrograph on the 0.81-m telescope.
This collection includes the full supplied archive, including the stars in the
separately published hot-supergiant subset and additional stellar targets.
Wavelengths are computed from the original linear IRAF WCS in Angstroms and
served in meters. Fluxes are relative; continuum normalization is recorded only
where supplied in the metadata. Resolving power R=12000 is adopted from the
existing collection documentation, not measured separately for each spectrum.
One-dimensional reduced optical stellar spectra obtained at the Three College
Observatory (TCO) with the eShel spectrograph on the 0.81-m telescope.
This collection includes the full supplied archive, including the stars in the
separately published hot-supergiant subset and additional stellar targets.
Wavelengths are computed from the original linear IRAF WCS in Angstroms and
served in meters. Fluxes are relative; continuum normalization is recorded only
where supplied in the metadata. Resolving power R=12000 is adopted from the
existing collection documentation, not measured separately for each spectrum.
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