“…For the shot-noise contributions, we consider typical values of M PBH / f PBH = 10 −12 M , 10 −3 M , 10 4.5 M , and 10 10 M . These values correspond to the cases of all the dark matter ("DM": light green, M PBH = 10 −12 M , f PBH = 1) [74], excess events of OGLE observations ("OGLE": dark yellow, M PBH = 10 −5 M , f PBH = 10 −2 ) [11,75,76], the origin of binary black holes leading to the gravitational-wave events of LIGO/Virgo ("LIGO/Virgo": orange, M PBH = 10 1.5 M , f PBH = 10 −3 ) [2,4,5], and the seeds of supermassive black holes ("SMBH": red, M PBH = 10 3.5 M , f PBH = 10 −6.5 ) [12][13][14], respectively. These are just benchmark points, and the actual allowed region of M PBH is not a point but a band.…”