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Galactic diffuse emission has provided us with evidence for cosmic rayacceleration throughout the Galaxy and the background for searches for physicsbeyond the Standard Model. However, only the very limited measurements of thediffuse flux are available in TeV $\gamma$ rays. The High Altitude WaterCherenkov (HAWC) Observatory is well-suited for observing the diffuse emissionof very high energy with its unbiased, wide field of view (2 sr). Using datafrom HAWC, we present techniques for measuring the diffuse flux and showpreliminary results.

Techniques for Measuring Galactic Diffuse Emission Flux and their Preliminary Results in Confused Regions