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SWAG ("Survey of Water and Ammonia in the Galactic Center") is a multi-lineinterferometric survey toward the Center of the Milky Way conducted with theAustralia Telescope Compact Array. The survey region spans the entire ~400pcCentral Molecular Zone and comprises ~42 spectral lines at pc spatial andsub-km/s spectral resolution. In addition, we deeply map continuum intensity,spectral index, and polarization at the frequencies where synchrotron,free-free, and thermal dust sources emit. The observed spectral lines includemany transitions of ammonia, which we use to construct maps of molecular gastemperature, opacity and gas formation temperature (see poster by Nico Kriegeret al., this volume). Water masers pinpoint the sites of active star formationand other lines are good tracers for density, radiation field, shocks, andionization. This extremely rich survey forms a perfect basis to construct mapsof the physical parameters of the gas in this extreme environment.

SWAG: Survey of Water and Ammonia in the Galactic Center