Model SEDs of Stars from M. Cohen et al.

Calibrated spectral templates assembled from ground-based and KAO observations from Martin Cohen et al. calibrated absolutely via accurate broadband photometry. 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 dynamic calibration of staring PHOT-S observations (2.5 - 11.8 microns):

Model SEDs of stars from P. Hammersley

Calibrated spectral templates provided by Peter Hammersley. 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 dynamic calibration of staring PHT-S observations (2.5 - 11.8 microns):


Last update: 12-07-2000 by Pedro Garcia-Lario