W-CDF-S, ELAIS-S1, and XMM-LSS will be three Deep-Drilling Fields (DDFs) of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), but their extensive multiwavelength data have not been fully utilized as done in the COSMOS field, another LSST DDF. To prepare for future science, we fit source spectral energy distributions (SEDs) from X-ray to far-infrared in these three fields mainly to derive galaxy stellar masses and star formation rates. We use CIGALE v2022.0, a code that has been regularly developed and evaluated, for the SED fitting. Our catalog includes 0.8 million sources covering 4.9deg^2^ in W-CDF-S, 0.8 million sources covering 3.4deg^2^ in ELAIS-S1, and 1.2 million sources covering 4.9deg^2^ in XMM-LSS. Besides fitting normal galaxies, we also select candidates that may host active galactic nuclei (AGNs) or are experiencing recent star formation variations and use models specifically designed for these sources to fit their SEDs; this increases the utility of our catalog for various projects in the future. We calibrate our measurements by comparison with those in well-studied smaller regions and briefly discuss the implications of our results. We also perform detailed tests of the completeness and purity of SED-selected AGNs. Our data can be retrieved from a public website.

Cone search capability for table J/ApJS/262/15/es1_v1 (*ELAIS-S1 SED-fitting results)

Cone search capability for table J/ApJS/262/15/wcdfs_v1 (*W-CDF-S SED-fitting results)

Cone search capability for table J/ApJS/262/15/xmmlss_v1 (*XMM-LSS SED-fitting results)