Table 2: Monochromatic flux densities in [Jy] of the stellar calibrators at the TIMMI2 central filter wavelengths. Note: The key wavelengths were taken from http://www.ls.eso.org/lasilla/sciops/3p6/timmi/Filters. The model fluxes were taken from http://www.iso.vilspa.esa.es/users/expl_lib/ISO/wwwcal/isoprep/cohen/templates/ and interpolated to the central filter wavelengths.
Filter/Wavelength [ $\mu$ m]

Star N1 N8.9 N9.8 N10.4 N2 N11.9 N12.9 Q1

8.70 8.73 9.68 10.38 10.68 11.66 12.35 17.72

HD 47105 9.16 9.08 7.47 6.52 6.17 5.19 4.58 2.27

HD 123139 69.97 69.51 57.37 50.09 47.61 40.08 35.59 17.63

HD 196171 25.58 25.42 20.98 18.32 17.41 14.65 13.01 6.45

**Table 2:** Monochromatic flux densities in [Jy] of the stellar calibrators at the TIMMI2 central filter wavelengths. Note: The key wavelengths were taken from http://www.ls.eso.org/lasilla/sciops/3p6/timmi/Filters. The model fluxes were taken from http://www.iso.vilspa.esa.es/users/expl_lib/ISO/wwwcal/isoprep/cohen/templates/ and interpolated to the central filter wavelengths.
	Filter/Wavelength [ $\mu$ m]
Star	N1	N8.9	N9.8	N10.4	N2	N11.9	N12.9	Q1
	8.70	8.73	9.68	10.38	10.68	11.66	12.35	17.72
HD 47105	9.16	9.08	7.47	6.52	6.17	5.19	4.58	2.27
HD 123139	69.97	69.51	57.37	50.09	47.61	40.08	35.59	17.63
HD 196171	25.58	25.42	20.98	18.32	17.41	14.65	13.01	6.45

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Thermophysical model description
	4 Thermophysical modelling on the combined dataset
	5 Thermophysical modelling of the new dataset
	6 Discussion
	7 Conclusion
	References