Abstract Phosphorus is a necessary element for life on Earth, but at present, we have limited constraints on its chemistry in star- and planet-forming regions; to date, phosphorus carriers have only been detected toward a few low-mass protostars. Motivated by an apparent association between phosphorus molecule emission and outflow shocking, we used the IRAM 30 m telescope to target PN and PO lines toward seven solar-type protostars with well-characterized outflows and firmly detected phosphorus molecules in three new sources. This sample, combined with archival observations of three additional sources, enables the first exploration of the demographics of phosphorus chemistry in low-mass protostars. The sources with PN detections show evidence for strong outflow shocks based on their H₂O 1₁₀–1₀₁ fluxes. On the other hand, no protostellar properties or bulk outflow mechanical properties are found to correlate with the detection of PN. This implies that gas-phase phosphorus is specifically linked to shocked gas within the outflows. Still, the PN and PO line kinematics suggest an emission origin in postshocked gas rather than directly shocked material. Despite sampling a wide range of protostellar properties and outflow characteristics, we find a fairly narrow range of source-averaged PO/PN ratios (0.6–2.2) and volatile P abundances as traced by (PN+PO)/CH₃OH (∼1%–3%). Spatially resolved observations are needed to further constrain the emission origins and environmental drivers of the phosphorus chemistry in these sources.