  We present Hubble multi-wavelength photometric catalogs, including (up to) 17
filters with the Advanced Camera for Surveys and Wide Field Camera 3 from the
ultra-violet to near-infrared for the Hubble Frontier Fields and associated
parallels. We have constructed homogeneous photometric catalogs for all six
clusters and their parallels. To further expand these data catalogs, we have
added ultra-deep $K_{S}$-band imaging at 2.2~\micron\ from the Very Large
Telescope HAWK-I and Keck-I MOSFIRE instruments. We also add post-cryogenic
\spitzer\ imaging at 3.6~\micron\ and 4.5~\micron\ with the Infrared Array
Camera (IRAC), as well as archival IRAC 5.8~\micron\ and 8.0~\micron\ imaging
when available. We introduce the public release of the multi-wavelength
(0.2--8~\micron) photometric catalogs, and we describe the unique steps applied
for the construction of these catalogs. Particular emphasis is given to the
source detection band, the contamination of light from the bright cluster
galaxies and intra-cluster light. In addition to the photometric catalogs, we
provide catalogs of photometric redshifts and stellar population properties.
Furthermore, this includes all the images used in the construction of the
catalogs, including the combined models of bright cluster galaxies and
intra-cluster light, the residual images, segmentation maps and more. These
catalogs are a robust data set of the Hubble Frontier Fields and will be an
important aide in designing future surveys, as well as planning follow-up
programs with current and future observatories to answer key questions
remaining about first light, reionization, the assembly of galaxies and many
more topics, most notably, by identifying high-redshift sources to target.
