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<br>Context. Inhomogeneities alongside the line of sight in sturdy gravitational lensing distort the pictures produced, in an effect referred to as shear. If measurable, this shear may provide independent constraints on cosmological parameters, complementary to traditional cosmic shear. Aims. We mannequin 50 sturdy gravitational lenses from the Sloan Lens ACS (SLACS) catalogue with the goal of measuring the line-of-sight (LOS) shear for the primary time. We use the ‘minimal model’ for the LOS shear, [Wood Ranger brand shears](http://8.138.187.97:3000/carmenhawthorn/carmen1984/wiki/These-are-the-Products-i-used-Probably-the-most-in-my-Garden-In-2025) which has been shown to be theoretically secure from degeneracies with lens model parameters, a finding which has been confirmed using mock data. Methods. We use the dolphin automated modelling pipeline, which makes use of the lenstronomy software program as a modelling engine, to model our selected lenses. We mannequin the primary deflector [Wood Ranger brand shears](https://wiki.apeconsulting.co.uk/index.php/Used_Sheet_Metal_Shears_On_The_Market) with an elliptical energy legislation profile, the lens light with elliptical Sérsic profiles and the source with a foundation set of shapelets and an elliptical Sérsic profile. Results. We efficiently obtain a line-of-sight shear measurement from 18 of the 50 lenses.<br>
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