Dust mass compared to stellar mass for the Taurus disks. We note that M_d was computed using distances inferred from Gaia DR2, assuming a 20K disk temperature and using the most updated value of F_0.87mm from Andrews et al. (2013), Tripathi et al. (2017), and Ward-Duong et al. (2018). Sources where F_0.87mm was extrapolated from a F_1.3mm measurement are plotted in faded colors (see Table 2 in Andrews et al. 2013), while direct measurements from SMA or ALMA are plotted in darker colors. Green triangles denotes upper limits, and the VLMS studied in this work are plotted as orange stars.