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Table 4:

Adopted disk outer radii.

Object
$R_{\rm {out}}$$\!\!\!\!$a (K02) $R_{\rm {out}}$$\!\!\!\!$a (AW07) $R_{\rm {g}}$$\!$b (I09) Adopted $R_{\rm {out}}$-interval
  (AU) (AU) (AU) (AU)

AA Tau
$\rm 214^{+63}_{-51}$ $\rm 400^{+600}_{-75}$ ... 200-400
CI Tau ... $225\pm 50$ ... 150-250
CW Tau ... ... ... 100-300
CX Tau ... ... ... 100-300
CY Tau $211\pm 28$ ... 230 230-330
DE Tau ... ... ... 100-300
DL Tau $\rm 152^{+28}_{-27}$ $\rm 175^{+50}_{-25}$ ... 150-250
DM Tau $220\pm 47$ $\rm 150^{+250}_{-100}$ 160 160-260
DN Tau $147\pm 469$ $\rm 100^{+300}_{-25}$ 125 125-225
DO Tau $98\pm 52$ ... ... 100-200
DR Tau $193\pm 141$ $\rm 100^{+175}_{-25}$ 90 90-190
DS Tau ... ... ... 100-300
FM Tau ... ... ... 100-300
FZ Tau ... ... ... 100-300
GM Aur $\rm 151^{+63}_{-29}$ $150\pm 25$ 270 270-370
GO Tau ... $\rm 350^{+650}_{-175}$ 160 160-260
HO Tau ... ... ... 100-300
IQ Tau $\rm 329^{+403}_{-70}$ ... ... 250-400
RY Tau $81\pm 128$ $150\pm 25$ 115 115-215
SU Aur ... ... ... 100-300
UZ Tau E ... ... 160 160-260

Notes. (a)  $R_{\rm {out}}$ listed here results from image fitting using a truncated power-law for the surface density profile. K02: Kitamura et al. (2002); AW07: Andrews & Williams (2007). (b)  $R_{\rm {g}}$ is the radius within which the 95% of the flux is observed, after fitting the visibility of the source with a Gaussian; we used this value, when available, as a lower limit for our adopted $R_{\rm {out}}$-interval. I09: Isella et al. (2009).


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