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The rich information on (sub)millimeter dust continuum emission from distantgalaxies in the public Atacama Large Millimeter/submillimeter Array (ALMA)archive is contained in thousands of inhomogeneous observations from individualPI-led programs. To increase the usability of these data for studies deepeningour understanding of galaxy evolution, we have developed automated miningpipelines for the ALMA archive in the COSMOS field (A3COSMOS) that efficientlyexploit the available information for large numbers of galaxies across cosmictime and keep the data products in sync with the increasing public ALMAarchive: (a) a dedicated ALMA continuum imaging pipeline, (b) two complementaryphotometry pipelines for both blind source extraction and prior source fitting,(c) a counterpart association pipeline utilizing the multiwavelength dataavailable (including quality assessment based on machine-learning techniques),(d) an assessment of potential (sub)millimeter line contribution to themeasured ALMA continuum, and (e) extensive simulations to provide statisticalcorrections to biases and uncertainties in the ALMA continuum measurements.Application of these tools yields photometry catalogs with ~1000(sub)millimeter detections (spurious fraction ~8%-12%) from over 1500individual ALMA continuum images. Combined with ancillary photometric andredshift catalogs and the above quality assessments, we provide robustinformation on redshift, stellar mass, and star formation rate for ~700galaxies at redshifts 0.5-6 in the COSMOS field (with undetermined selectionfunction). The ALMA photometric measurements and galaxy properties are releasedpublicly within our blind extraction, prior fitting, and galaxy propertycatalogs, plus the images. These products will be updated on a regular basis inthe future.

the astrophysical journal. supplement series/astrophysical journal. supplement series

Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): I.  Robust ALMA Continuum Photometry Catalogs and Stellar Mass and Star Formation  Properties for ~700 Galaxies at z=0.5-6