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==> In this proposal, more time is being requested for RTUFFS.SNR
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We propose observations to follow up the detections of dust and line emission
from SN ejecta in Cas A. We further request more time to replace observations
which had to be removed from RTUFFS.SNR due to time constraints. In particular,
we request a combination of SWS full resolution spectra and deep PHT-S spectra
at the position detected in Cas A with ejected dust to measure the dust
composition. Also for Cas A we need mapping at more FIR wavelengths to counter
Cirrus confusion  and place deep limits on the overall grain yield in the SNR.
We further propose a deep PHT-S map of the whole remnant to delineate the
space and velocity distribution of the bright MIR emission lines.
We put spring launch Crab targets into the autumn list and in addition
propose spectrophotometry towards a prominent patch of optical obscuration in
the ejecta with PHT-S and SWS.