1) In section 4, the uncertainties for MIPS 70um should be 5%, not 7%
(the 7% is an old number, the final version of the paper found 5%).

--thanks

2) While the pile-on may not be useful, I wouldn't mind having a
reference to Gordon et al. (2008, ApJ, 682, 336) added to the list
discussing cause of depressed aromatic emission at low
metallicities/hard radiation fields (section 5.4, page 14).  I think
this paper does add something new to the discussion.

--done

3) The discussion of the tight correlation between 70/TIR and 160/TIR
versus 70/160 should probably include some acknowledgement that TIR is
based strongly on 70 & 160.  The tightness of the correlation is to be
expected, right?

--yes, and i've tweaked the text accordingly.

4) I would argue in section 5.5, that the IR-to-UV ratio is an excellent
measure of dust extinction for star forming systems.  The fact that it
does not correlation with dust reddening (as defined by beta or
1500/2500) is not surprising given that this reddening is the poor
indicator.  This was shown (fairly convincingly I think) in Witt &
Gordon (2000, ApJ, 528, 799) and, in more detail, Gordon et al. (2000,
ApJ, 533, 236).

--I've updated the text accordingly.  One of the issues here is the qualification for 'star-forming' galaxies that I added to the sentence -- some of the LVL targets are not star-forming, so we need to be a bit careful with the wording.

5) Today was my paper writing day at home and I worked on the SAGE-SMC
Overview paper (Gordon et al. 2009, in prep - I expect it will be
submitted in the next few months).  Part of this work was to measure the
IRAC and MIPS global fluxes of the SMC.  They are below.  These
supercede previous work as we now have the full SMC covered and can do
accurate background subtraction.  There still are some issues with
mosaicking the full set of IRAC 5.8um data and so I don't have a
measurement there yet.  I should have one soon.

wavelength, flux [Jy], unc [Jy], band
3.550   300.   20.  IRAC1
4.493   220.   10.  IRAC2
7.872   200.   10.  IRAC4
 23.7   350.   10.  MIPS24
 71.0 11200   500.  MIPS70
156.0 21700  2600.  MIPS160

--Thanks!