Galaxy Properties Derived with Spectral Energy Distribution Fitting in
  the Hawaii-Hubble Deep Field-North
  We compile multi-wavelength data from ultraviolet to infrared (IR) bands as
well as redshift and source-type information for a large sample of 178,341
sources in the Hawaii-Hubble Deep Field-North field. A total of 145,635 sources
among the full sample are classified/treated as galaxies and have redshift
information available. We derive physical properties for these sources
utilizing the spectral energy distribution fitting code CIGALE that is based on
Bayesian analysis. Through various consistency and robustness check, we find
that our stellar-mass and star-formation rate (SFR) estimates are reliable,
which is mainly due to two facts. First, we adopt the most updated and accurate
redshifts and point spread function-matched photometry; and second, we make
sensible parameter choices with the CIGALE code and take into account
influences of mid-IR/far-IR data, star-formation history models, and AGN
contribution. We release our catalog of galaxy properties publicly (including,
e.g., redshift, stellar mass, SFR, age, metallicity, dust attenuation), which
is the largest of its kind in this field and should facilitate future relevant
studies on formation and evolution of galaxies.
