摘要： We have calibrated the 6.5 m James Webb Space Telescope (JWST) mid-infrared (MIR) ?lters as star formation rate (SFR) indicators, using JWST photometry synthesized from Spitzer spectra of 49 low-redshift galaxies, which cover a wider luminosity range than most previous studies. We use Balmer-decrement-corrected Hα luminosity and synthesized MIR photometry to empirically calibrate the Spitzer, WISE, and JWST ?lters as SFR indicators. Our Spitzer and WISE calibrations are in good agreement with recent calibrations from the literature. While MIR luminosity may be directly proportional to SFR for high-luminosity galaxies, we ?nd a power-law relationship between MIR luminosity and SFR for low-luminosity galaxies (L ~ 1- ). We ?nd that for galaxies with an Hα luminosity of 10 erg s ), the corresponding JWST MIR ν Lν luminosity is between 1040.50 and 10. Power-law ?ts of JWST luminosity as a function of Hα luminosity have indices between 1.17 and 1.32. We ?nd that the scatter in the JWST ?lter calibrations decreases with increasing wavelength from 0.39 to 0.20 dex, although F1000W is an exception where the scatter is just 0.24 dex.