Table A.5: Data of the Midcourse Space eXperiment (MSX). The instrument on board MSX is the SPIRIT III (Spatial Infrared Imaging Telescope III). The approximate effective wavelengths of the 6 MSX filters are in ${\mu }$ m.
Name B1(Jy) B2(Jy) A(Jy) C(Jy) D(Jy) E(Jy)

4.29 ${\mu }$ m 4.35 ${\mu }$ m 8.28 ${\mu }$ m 12.13 ${\mu }$ m 14.65 ${\mu }$ m 21.34 ${\mu }$ m

SU Gem 8.283 7.666 7.178 7.505

U Mon
42.93 54.45 88.71 72.38 73.29

R Sct
43.12 49.27 22.02 11.82 11.09 6.350

**Table A.5:** Data of the Midcourse Space eXperiment (MSX). The instrument on board MSX is the SPIRIT III (Spatial Infrared Imaging Telescope III). The approximate effective wavelengths of the 6 MSX filters are in ${\mu }$ m.
Name	B1(Jy)	B2(Jy)	A(Jy)	C(Jy)	D(Jy)	E(Jy)
	4.29 ${\mu }$ m	4.35 ${\mu }$ m	8.28 ${\mu }$ m	12.13 ${\mu }$ m	14.65 ${\mu }$ m	21.34 ${\mu }$ m
SU Gem			8.283	7.666	7.178	7.505
U Mon		42.93	54.45	88.71	72.38	73.29
R Sct	43.12	49.27	22.02	11.82	11.09	6.350

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction: 850 ${\mu }$ m SCUBA data
	3 Spectral Energy Distributions (SEDs)
	4 An optically thin dust fit
	5 Discussion: Characteristics of the dust excess
	6 Conclusions
	References
	Online Material
	Appendix A: Photometric data