Determining dust temperatures and masses in the Herschel era: the importance of observations longward of 200 micron

K. D. Gordon, F. Galliano, S. Hony +21

The properties of the dust grains (e.g., temperature and mass) can be derived from fitting far-IR SEDs (>100 micron). Only with SPIRE on Herschel has it been possible to get high s…