The Great Observatories All-Sky LIRG Survey: Herschel Image Atlas and
  Aperture Photometry
  Far-infrared (FIR) images and photometry are presented for 201 Luminous and
Ultraluminous Infrared Galaxies [LIRGs: log$(L_{\rm IR}/L_\odot) = 11.00 -
11.99$, ULIRGs: log$(L_{\rm IR}/L_\odot) = 12.00 - 12.99$], in the Great
Observatories All-Sky LIRG Survey (GOALS) based on observations with the
$Herschel$ $Space$ $Observatory$ Photodetector Array Camera and Spectrometer
(PACS) and the Spectral and Photometric Imaging Receiver (SPIRE) instruments.
The image atlas displays each GOALS target in the three PACS bands (70, 100,
and 160 $\mu$m) and the three SPIRE bands (250, 350, and 500 $\mu$m), optimized
to reveal structures at both high and low surface brightness levels, with
images scaled to simplify comparison of structures in the same physical areas
of $\sim$$100\times100$ kpc$^2$. Flux densities of companion galaxies in
merging systems are provided where possible, depending on their angular
separation and the spatial resolution in each passband, along with integrated
system fluxes (sum of components). This dataset constitutes the imaging and
photometric component of the GOALS Herschel OT1 observing program, and is
complementary to atlases presented for the Hubble Space Telescope (Evans et al.
2017, in prep.), Spitzer Space Telescope (Mazzarella et al. 2017, in prep.),
and Chandra X-ray Observatory (Iwasawa et al. 2011, 2017, in prep.).
Collectively these data will enable a wide range of detailed studies of AGN and
starburst activity within the most luminous infrared galaxies in the local
Universe.
