Photometric Redshifts in the W-CDF-S and ELAIS-S1 Fields Based on Forced
  Photometry from 0.36 -- 4.5 Microns
  The W-CDF-S and ELAIS-S1 fields will be two of the LSST Deep Drilling fields,
but the availability of spectroscopic redshifts within these two fields is
still limited on deg^2 scales. To prepare for future science, we use EAZY to
estimate photometric redshifts (photo-zs) in these two fields based on
forced-photometry catalogs. Our photo-z catalog consists of ~0.8 million
sources covering 4.9 deg^2 in W-CDF-S and ~0.8 million sources covering 3.4
deg^2 in ELAIS-S1, among which there are ~0.6 (W-CDF-S) and ~0.4 (ELAIS-S1)
million sources having signal-to-noise-ratio (SNR) > 5 detections in more than
5 bands. By comparing photo-zs and available spectroscopic redshifts, we
demonstrate the general reliability of our photo-z measurements. Our photo-z
catalog is publicly available at \doi{10.5281/zenodo.4603178}.
