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LSST Strong Lensing Systems Dark Matter Sensitivity Analysis with Neural Ratio Estimators

  • Authors: Andreas Filipp, Yashar Hezaveh, Laurence Perreault-Levasseur, Daniel Gilman

Andreas Filipp et al 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure 1.

Range of possible DM HMFs with this parameterization with respect to the CDM parameterization, shown by the black solid line. The gray covers all the possibilities, with the minimal A being limited to A > 10−3 for illustration purposes. A = 0 corresponds to no subhalos for any power-law slope γ.

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