GAMA_quasarhosts_starformation analyzes galaxy- and quasar-host photometric data from the GAMA Survey to estimate star-formation rates (SFRs) for quasar host galaxies. The code compiles host-galaxy photometry and performs SED-based fitting to derive SFRs for a sample of quasar-hosts in the GAMA fields. It also applies quality cuts and selection criteria defined in the repository to separate reliable host SFR estimates from less certain ones. The pipeline outputs tables of galaxy properties and plots that can be used for analysis and publication.