New Q-wide vs. sky

As can be seen in the plot above, the short wavelength cut-off is
probably defined by the atmospheric transmission (becomes reasonable
> 17 μm?), and the long wavelength cut-off is likely to be set by the
combined effect of the KBr entrance window and the Si:As detector
quantum efficiency (both falling rapidly beyond ~26 μm?).
New Q-wide vs. old Q-short

As the new Q-wide filter is on average about 10%
more transparent than the old Q-short filter
(scanned thin black line), it is
expected that the sensitivity of the new QM mode would
perhaps be slightly more sensitive than the old
QM-short mode.