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This paper gives an overview of TEMPLATES, a JWST Early Release Scienceprogram that targeted four extremely bright, gravitationally lensed galaxies:two extremely dusty, two with low attenuation, as templates for galaxyevolution studies with JWST. TEMPLATES obtains a common set of spectraldiagnostics for these 1.3 < z < 4.2 galaxies, in particular H alpha, Paschenalpha, and the rest-frame optical and near-infrared continua. In addition, twoof the four targets have JWST coverage of [O III] 5007 Angstrom and H beta; theother two targets have have JWST coverage of PAH 3.3 micron and complementaryALMA data covering the [C II] 158 micron emission line. The science goals ofTEMPLATES are to demonstrate attenuation-robust diagnostics of star formation,map the distribution of star formation, compare the young and old stellarpopulations, and measure the physical conditions of star formation and theirspatial variation across the galaxies. In addition, TEMPLATES has technicalgoals to establish best practices for the Integral Field Units (IFU) within theNIRSpec and MIRI instruments, both in terms of observing strategy and in termsof data reduction. The paper describes TEMPLATES's observing program,scientific and technical goals, data reduction methods, and deliverables,including high-level data products and data reduction cookbooks.

JWST Early Release Science Program TEMPLATES: Targeting Extremely Magnified Panchromatic Lensed Arcs and their Extended Star formation