The JCMT Gould Belt Survey: SCUBA-2 observations of circumstellar disks
  in L 1495
  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 L1495. 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.
