1. Introduction
2. Scientific Goals
2.1. The dust properties of dwarf galaxies
2.2. FIR Fine-Structure lines as gas coolants in the interstellar medium
2.3. Possible Warm Gas Reservoir in Dwarf Galaxies?
2.4. Dust to Gas Mass ratios (D/G)
3. Source Selection
4. Observation strategy and data reduction
4.1. PACS imaging
4.2. PACS spectroscopic observations
4.3. SPIRE imaging
4.4. SPIRE FTS observations
4.5. Ancillary data - for a multiphase, multiwavelength approach
5. A taste of science results
5.1. Distribution of the ISM components in NGC 4214
5.2. FIR dust and gas properties within NGC 4214
5.3. Submillimetre excess
6. DGS Products
7. Summary