1. INTRODUCTION

1.2. Forward Modelling and Direct Inference of Semi-Resolved Stellar Populations

1.3. Simulation Based Inference

2. THE SILKSCREEN FRAMEWORK

2.1. Simulating Images of Dwarf Galaxies

2.2. Network Architecture

2.3. Current Pipeline: Bespoke Simulations and Training

3. INFERENCE ON MOCK GALAXIES

4. APPLICATION TO A SAMPLE OF REAL GALAXIES

5. CURRENT LIMITATIONS

6. SUMMARY AND FUTURE OUTLOOK