Model spectra of ISO GBPP stars

• Model spectra of [most of] the GBPP stars that have been observed during the ISO PV phase or the Routine Operations Phase. Wavelength coverage is 1-160 microns, with dense gridding up to 10 microns, and sparse gridding thereafter. Stars are identified by their HIC , HR , HD or SAO numbers; those ending with "sn" were normalized to Selby narrow-band photometry, those with "tb" to TCS broadband photometry. There is one star in common. See explanatory note for more details.

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Last update: Pedro Garcia-Lario , 24-08-1999