AMPM survey detects one microlensing candidate in LMC data and constrains up to 30% of Galactic primordial black hole dark matter at 95% C.L. in the asteroid-to-planetary mass range, with peak sensitivity shifted to lunar masses by second-order effects.
Salucci, The distribution of dark matter in galaxies
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The universal rotation curve remains universal out to 2R_opt when constructed from SPARC extended HI rotation curves.
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AMPM I. A Targeted Search for Asteroid Mass Primordial Black Hole Microlenses
AMPM survey detects one microlensing candidate in LMC data and constrains up to 30% of Galactic primordial black hole dark matter at 95% C.L. in the asteroid-to-planetary mass range, with peak sensitivity shifted to lunar masses by second-order effects.
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Extended Universal Rotational Curve of Spiral Galaxies
The universal rotation curve remains universal out to 2R_opt when constructed from SPARC extended HI rotation curves.