Table 2: Observations with SCUBA: $850~\mu$ m fluxes.
Name F₈₅₀

(mJy)

TW Cam 11.0 $\pm$ 2.3

RV Tau
50.3 $\pm$ 3.6

SU Gem
7.5 $\pm$ 2.5

UY CMa
2.4 $\pm$ 2.1

U Mon
181.6 $\pm$ 2.6

AC Her
99.4 $\pm$ 3.8

R Sct
2.4 $\pm$ 1.6

**Table 2:** Observations with SCUBA: $850~\mu$ m fluxes.
Name	F₈₅₀
	(mJy)
TW Cam	11.0 $\pm$ 2.3
RV Tau	50.3 $\pm$ 3.6
SU Gem	7.5 $\pm$ 2.5
UY CMa	2.4 $\pm$ 2.1
U Mon	181.6 $\pm$ 2.6
AC Her	99.4 $\pm$ 3.8
R Sct	2.4 $\pm$ 1.6

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