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Each Rocky Worlds target will require multiple eclipse observations with JWST to search for evidence of atmospheres; a subset of host stars will be targeted for UV observations with HST. Those observations will be interspersed with other GO and DD programs throughout each cycle. For each target, the eclipse data will be combined by STScI and the combined final data product, together with the raw data files, will be made public through MAST, likely after all observations of that particular target are taken. This follows the recommendation of the Working Group to provide open access (see below for restrictions for CIT and SAC members). HST observations of the host stars will be non-proprietary and will likely be available immediately. The SAC will determine the final release schedule. 

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