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Hatchell, J.M. Kirk, J. Rawlings, J. S. Richer, J. V. Buckle, J. Wouterloot, J. Yates, K. Marsh, K. Pattle, L.B.G. Knee, M. Chen, M. Fich, M.J. Currie, M.R. Hogerheijde, M. Zhu, N. Tothill, P. Bastien, P. Friberg, R. Friesen, S. Coude, S.F. Beaulieu, S. Graves, S. Mairs, S. Sadavoy, S. Tisi, S. Viti, T. Jenness, W. Holland","submitted_at":"2015-02-27T16:06:33Z","abstract_excerpt":"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. 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