This is an MCMC Bayesian Spectral Energy Distribution fitting for HST photometry. The current release has been tested with ACS and WFC3-IR data.

Maintenance and current development of this MCMC Bayesian SED fitting tool is led by Giovanni M. Strampelli (STScI). A special thanks to Dr. Massimo Robberto (STScI), Dr. Laurant Pueyo (STScI), Dr. Jonathan Aguilar (STScI) and Professor Antonio Aparicio (ULL) for their guidance during the development of the pipeline.

Citation: If this tool is useful for your research, please cite Strampelli, G. M. et al. 2024, apj, 967, 52S