THE ISO HANDBOOK.

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 ISOCAM (2.5 - 17 microns):



Last update: 14-07-2000 by Pedro Garcia-Lario