ISO impact on stellar models and vice versa
  We 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. 
L. Decin (1), C. Waelkens (1), K. Eriksson (2), B. Gustafsson (2)   B.Plez (3), A.J. Sauval (4), W. Van Assche (5) and B. Va...