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):
- HD 116405 (=
SAO 44585 = HIC 65280), A0V, (
plot)
- HD 120787 (=
SAO 16186 = HIC 67485), G3V, (
plot)
- HR 5350 (= HD 125161 = SAO 29071), A9V, (plot
)
- SAO 83309 (= HIC
70218), K5V, (plot )
- HR 5423 (= HD 127334 = SAO 45075), G5V, (plot )
- HD 132142 (= SAO 29336 = HIC 73005), K1V, (plot)
- HR 5830 (= HD 139798 = SAO 45650), F2V, (plot )
- HR 5886 (= HD 141653 = SAO 16848), A2IV, (plot )
- HR 5914 (= HD 142373 = SAO 45772), F9V, (plot )
- HR 6514 (= HD 158485 = SAO 30387), A4V, (plot )
- HR 6847 (=HD 168009 =
SAO 47343),
G2V, (plot)
- HR 7341 (= HD 181597 = SAO 48315), K1III, (plot )
- HD 184400 (= SAO
48555 = HIC 96062), F5, (plot )
- HR 7469 (= HD 185395 = SAO 31815), F4V, (plot )
- HR 7701 (= HD 191277 = SAO 18700), K3III, (plot )
- HR 7854 (= HD 195820 = SAO 32649), K0III, (plot )
Last update: 14-07-2000 by
Pedro Garcia-Lario