HAWC's view of the very-high-energy gamma-ray sky

The HAWC (High-Altitude Water Cherenkov) Observatory is a wide-field very-high-energy (E>100 GeV) gamma-ray observatory located on Sierra Negra, Mexico. It has been taking data almost continuously for seveal years, and has detected gamma-ray emission from more than 50 sources, most of which are located within our own Galaxy. Recent improvements in the energy reconstruction have enabled the HAWC collaboration to present a large-scale gamma-ray survey above 100 TeV.  In this presentation, I will present recent results from the HAWC experiment, focusing in particular on Galactic objects: Supernova remnants, extended emission around pulsars, pevatron candidates, and the microquasar SS433. I will also present upgrades to the HAWC detector (currently in progress) as well as plans for future-generation
instrumentation.