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We report on new distances and proper motions to seven stars across theSerpens/Aquila complex. The observations were obtained as part of the Gould'sBelt Distances Survey (GOBELINS) project between September 2013 and April 2016with the Very Long Baseline Array (VLBA). One of our targets is theproto-Herbig AeBe object EC 95, which is a binary system embedded in theSerpens Core. For this system, we combined the GOBELINS observations withprevious VLBA data to cover a total period of ~8 years, and derive the orbitalelements and an updated source distance. The individual distances to sources inthe complex are fully consistent with each other, and the mean valuecorresponds to a distance of $436.0\pm9.2$~pc for the Serpens/W40 complex.Given this new evidence, we argue that Serpens Main, W40 and Serpens South arephysically associated and form a single cloud structure.

The Gould's Belt Distances Survey (GOBELINS) III. The distance to the Serpens/Aquila Molecular Complex