Absolute integrated line fluxes of H II regions have been measured using a
Fabry-Perot spectrophotometer. We describe the observations and calibration
procedures. Fluxes are given for 36 H II regions with Galactocentric dista
nces ranging from 6.6 to 17.7 kpc. Several emission lines have been measure
d, mainly [O II] lambda lambda 3726 and 3629, H beta, [O III] lambda 5007,
He I lambda 5876 and H alpha. The very faint [O III] lambda 4363 line has b
een measured in six regions, allowing a direct determination of the electro
n temperature. New photometric distances have been derived based on data fr
om the literature. A discussion of these results in terms of extinction, el
ectron density and temperature, and oxygen and helium abundances is given i
n Paper II.