Model SEDs of stars from P. Hammersley
Calibrated spectral templated provided by Peter Hammersley
used in the absolute flux calibration of chopped
PHT-S observations. 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 chopped PHT-S observations (2.5 - 11.8 microns):
- HR 6464 (= HD 157325),
M0III, (plot)
- HR 5986 (= HD 144284),
F8IV-V, (plot)
- HR 6817 (= HD 167042),
K1III, (plot)
- HR 6847 (=HD 168009),
G2V, (plot)
- HD 132142 (= SAO 29336), K1V, (plot)
- HD 172323 (= SAO
17936), F9V, (plot)
- HD 184400 (= SAO
48555), F5, (plot)
Last update: 12-07-2000 by
Pedro Garcia-Lario