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Jogler","submitted_at":"2013-08-23T20:02:14Z","abstract_excerpt":"The very high energy (VHE; >100 GeV) source HESS J0632+057 has been recently confirmed as a \\gamma-ray binary, a subclass of the high mass X-ray binary (HMXB) population, through the detection of an orbital period of 321 days. We performed a deep search for the emission of HESS J0632+057 in the GeV energy range using data from the Fermi Large Area Telescope (LAT). The analysis was challenging due to the source being located in close proximity to the bright \\gamma-ray pulsar PSR J0633+0632 and lying in a crowded region of the Galactic plane where there is prominent diffuse emission. 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