2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/1530We present a detailed spectroscopic study of a sample of bright, mostly cool, stars observed with the Short-Wavelength Spectrometer (SWS) on board the Infrared Space Observatory (ISO), which enables the accurate determination of the stellar parameters of the cool giants, but also serves as a critical review of the ISO-SWS calibration.6 pages, 3 figures, to appear in `ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy', held 2-4 February 2000, at VILSPAAstrophysicstext