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We present and describe the astro-photometric catalog of more than 800,000sources found in the Hubble Tarantula Treasury Project (HTTP). HTTP is a HubbleSpace Telescope (HST) Treasury program designed to image the entire 30 Doradusregion down to the sub-solar (~0.5 solar masses) mass regime using the WideField Camera 3 (WFC3) and the Advanced Camera for Surveys (ACS). We observed 30Doradus in the near ultraviolet (F275W, F336W), optical (F555W, F658N, F775W),and near infrared (F110W, F160W) wavelengths. The stellar photometry wasmeasured using point-spread function (PSF) fitting across all the bandssimultaneously. The relative astrometric accuracy of the catalog is 0.4 mas.The astro-photometric catalog, results from artificial star experiments and themosaics for all the filters are available for download. Color-magnitudediagrams are presented showing the spatial distributions and ages of starswithin 30 Dor as well as in the surrounding fields. HTTP provides the firstrich and statistically significant sample of intermediate and low mass pre-mainsequence candidates and allows us to trace how star formation has beendeveloping through the region. The depth and high spatial resolution of ouranalysis highlight the dual role of stellar feedback in quenching andtriggering star formation on the giant HII region scale. Our results areconsistent with stellar sub-clustering in a partially filled gaseous nebulathat is offset towards our side of the Large Magellanic Cloud.

Hubble Tarantula Treasury Project. III. Photometric Catalog and Resulting Constraints on the Progression of Star Formation in the 30 Doradus Region