We present 850 \mu m and 450 \mu m data from the JCMT Gould Belt Survey obtained with SCUBA-2 and characterise the dust attributes of Class I , Class II and Class III disk sources in L 1495 .
We detect 23 % of the sample at both wavelengths , with the detection rate decreasing through the Classes from I–III .
The median disk mask is 1.6 \times 10 ^ { -3 } M _ { \odot } , and only 7 % of Class II sources have disk masses larger than 20 Jupiter masses .
We detect a higher proportion of disks towards sources with stellar hosts of spectral type K than spectral type M. Class II disks with single stellar hosts of spectral type K have higher masses than those of spectral type M , supporting the hypothesis that higher mass stars have more massive disks .
Variations in disk masses calculated at the two wavelengths suggests there may be differences in dust opacity and/or dust temperature between disks with hosts of spectral types K to those with spectral type M .