The 1.4 GHz NRAO VLA Sky Survey (NVSS) images and source catalog were
used to detect radio emission from the 885 planetary nebulae north of
J2000 declination delta = -40 degrees in the Strasbourg-ESO Catalogue
of Galactic Planetary Nebulae. We identified 680 radio sources brighte
r than about S = 2.5 mJy beam(-1) (equivalent to T approximate to 0.8
K in the 45 '' FWHM NVSS beam) with planetary nebulae by coincidence w
ith accurate optical positions measured from Digitized Sky Survey (DSS
) images. Total extinction coefficients c at lambda = 4861 Angstrom we
re calculated for the 429 planetary nebulae with available HP fluxes a
nd low free-free optical depths at 1.4 GHz. The variation of c with Ga
lactic latitude and longitude is consistent with the extinction being
primarily interstellar and not intrinsic.