Fig. 10.
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Constraints on the fraction of the DM density provided by PBHs from the OGLE microlensing survey (Mróz et al. 2024), accretion limits from CMB observations (Serpico et al. 2020), SNe lensing (Zumalacarregui & Seljak 2018), the population of X-ray sources (Inoue & Kusenko 2017), Lyman-α data (Murgia et al. 2019), survival of wide binaries (Monroy-Rodríguez & Allen 2014), the population of gravitational wave (GW) sources (Andrés-Carcasona et al. 2024), and GW lensing (Urrutia et al. 2023). The red line shows the upper limit derived in this work from measurements of the UV luminosity function.
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