  We present a multi-band analysis of the six Hubble Frontier Field clusters
and their parallel fields, producing catalogs with measurements of source
photometry and photometric redshifts. We release these catalogs to the public
along with maps of intracluster light and models for the brightest galaxies in
each field. This rich data set covers a wavelength range from 0.2 to 8 $\mu m$,
utilizing data from the Hubble Space Telescope, Keck Observatories, Very Large
Telescope array, and Spitzer Space Telescope. We validate our products by
injecting into our fields and recovering a population of synthetic objects with
similar characteristics as in real extragalactic surveys. The photometric
catalogs contain a total of over 32,000 entries with 50\% completeness at a
threshold of $\mathrm{mag_{AB}}\sim 29.1$ for unblended sources, and
$\mathrm{mag_{AB}}\sim 29$ for blended ones, in the IR-Weighted detection band.
Photometric redshifts were obtained by means of template fitting and have an
average outlier fraction of 10.3\% and scatter $\sigma = 0.067$ when compared
to spectroscopic estimates. The software we devised, after being tested in the
present work, will be applied to new data sets from ongoing and future surveys.
