Hinkley, SashaKraus, A LCheetham, AnthonyCarpenter, J MTuthill, Peter GLacour, SylvestreEvans, Thomas MHaubois, XIreland, Michael2016-06-142041-8205http://hdl.handle.net/1885/103215We report the detection of seven low-mass companions to intermediate-mass stars (SpT B/A/F; 1.5-4.5 M<inf>o</inf>) in the Scorpius-Centaurus (Sco-Cen) Association using nonredundant aperture masking interferometry. Our newly detected objects have contrasts 4-6, corresponding to masses as low as ∼20 M<inf>Jup</inf> and mass ratios of 0.01-0.08, depending on the assumed age of the target stars. With projected separations ρ ≈ 10-30 AU, our aperture masking detections sample an orbital region previously unprobed by conventional adaptive optics imaging of intermediate-mass Sco-Cen stars covering much larger orbital radii (∼30-3000 AU). At such orbital separations, these objects resemble higher-mass versions of the directly imaged planetary mass companions to the 10-30 Myr, intermediate-mass stars HR 8799, β Pictoris, and HD 95086. These newly discovered companions span the brown dwarf desert, and their masses and orbital radii provide a new constraint on models of the formation of low-mass stellar and substellar companions to intermediate-mass stars.Author/s retain copyright201510.1088/2041-8205/806/1/L92016-06-14