This is a view of the dust maps in the five orders, generated by
splitting the larger pixels from the higher orders into HEALPixes of
order 10. This means, in particular, that the spatial resolution for
all pixels with original_order!=10. Use this for convenient joins to
other tables.
A catalogue of E(V-I) extinction values is presented for 3174 (LMC)
and 693 (SMC) fields within the Magellanic Clouds. The extinction
values were computed by determining the (V-I) colour difference of the
red clump from Optical Gravitational Microlensing Experiment (OGLE
III) observations in the V and I bands and theoretical values for
unreddend red clump colours.
TEUV corrects synthetic stellar fluxes for interstellar absorption
for wavelengths smaller than 91.1 nm. It simulates radiative
bound-free absorption of the ground states of H, He, C, N, and O using
Opacity Project data. Two interstellar components with different
radial and turbulent velocities, temperatures, and column densities
are considered.
