Table 2: Parameters of the elliptical fit of the image. In the first column, the inclination of the disk (0 degree means a faced-on disk). The position angle (PA) of the disk on the sky is measured counter-clockwise from the North. The distance corresponds to the maximum distance at which the disk is detected in the 20 $\mu$ m observations. The brightness level in the last column corresponds to the brightness of the maximum distance at which the disk is detected here.
i PA Distance Brightness level

(deg) (deg) (AU) (mJy/ $^{\prime \prime }$ 2)

HD 135344 46 $\pm$ 5 100 $\pm$ 10 210 170

HD 163296 60 $\pm$ 5 105 $\pm$ 10 215 135

CQ Tau 33 $\pm$ 5 120 $\pm$ 10 290 129

**Table 2:** Parameters of the elliptical fit of the image. In the first column, the inclination of the disk (0 degree means a faced-on disk). The position angle (PA) of the disk on the sky is measured counter-clockwise from the North. The distance corresponds to the maximum distance at which the disk is detected in the 20 $\mu$ m observations. The brightness level in the last column corresponds to the brightness of the maximum distance at which the disk is detected here.
	i	PA	Distance	Brightness level
	(deg)	(deg)	(AU)	(mJy/ $^{\prime \prime }$ 2)
HD 135344	46 $\pm$ 5	100 $\pm$ 10	210	170
HD 163296	60 $\pm$ 5	105 $\pm$ 10	215	135
CQ Tau	33 $\pm$ 5	120 $\pm$ 10	290	129

Source LaTeX | All tables | In the text