The apparent excess of hot Jupiters in phase-space overdensities is driven by younger, more massive, more metal-rich host stars, not by an intrinsic environmental formation channel.
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On Hot Jupiters and Stellar Clustering: The Role of Host Star Demographics
The apparent excess of hot Jupiters in phase-space overdensities is driven by younger, more massive, more metal-rich host stars, not by an intrinsic environmental formation channel.