Optical templates used in Rowan-Robinson et al (2008) are given in files new**.dat, 
with pairs of numbers in Angstrom and arbitrary f_lambda units.

Individual infrared templates are given in cirrus.dat, M82.dat, A220.dat, 
as pairs of numbers log10 lambda(mu), log vu S(nu),
and in dusttor.dat, as pairs of numbers log10 lambda(mu), vu S(nu) [first two columns
only].

Infrared templates, smoothed with a 0.1 dex boxcar filter,are collected in irtemplates2
There are 4 blocks of 147 numbers, 
first is log10(wavelngth in microns), second is log10 (nu S(nu)) for cirrus, third is for M82, 
fourth is A220 template.
Fifth block of numbers is log10( nu S(nu)) for AGN dust torus template at wavelengths given by
log10(lambda(microns)) = 3.1 (-0.1) -1.4

Cool cirrus templates used in Rowan-Robinson et al (2010) are cirrus1.dat (psi=1) and cirrus01.dat
(psi = 0.1).  Young starburst in same paper is youngsb.150.0.dat (Av=150, t=0).
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