Model SEDs of Stars from M. Cohen et al.

Calibrated spectral templates assembled from ground-based and KAO observations from Martin Cohen et al. The individual files contain information on the original data (both spectroscopic and photometric). Details about the overall calibration program can be found in the references listed here.

- Stars used for the calibration of ISOPHOT in the short wavelength range (3-30 microns):

- Stars used for the calibration of ISOPHOT in the long wavelength range (45-240 microns):

Model SEDs of stars from P. Hammersley

Calibrated spectral templates provided by Peter Hammersley. Wavelength coverage is 1-160 microns. The visible magnitudes and near-infrared photometry observed in the GBPP have been fitted with a Kurucz model to provide the flux densities at longer wavelengths. The overall spectral energy distribution is believed to be correct within 5% . See explanatory note for more details. - Stars used for the calibration of ISOPHOT in the short wavelength range (3-30 microns):

- Stars used for the calibration of ISOPHOT in the long wavelength range (45-240 microns):


Last update: 10-07-2000 by Pedro Garcia-Lario