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The Milky Way contains hundreds of binary systems which are known to emit inradio and X-rays, but only a handful of binaries have been observed to producevery high-energy gamma rays. In addition, the emission mechanisms which producethe gamma rays in the few known sources are not well understood. To improve thestatistics of binary sources in the TeV band, the High-Altitude Water CherenkovGamma-ray Observatory, or HAWC, has begun to carry out a simultaneous survey ofTeV binary candidates in the Northern Hemisphere between 100 GeV and 100 TeV.HAWC is a surface array that records air showers from cosmic rays and gammarays with a high uptime and wide field of view, making it well-suited toobserve time-dependent emission from objects such as TeV binaries. We describethe sensitivity of HAWC to periodic emission from Galactic sources of gammarays and present data from the first year of observations with the partiallyconstructed observatory.

Looking for Gamma-ray Emission from TeV Binary Candidates with HAWC