“…The gray shaded regions are the leading existing constraints from PIENU [78,79], PS191 [13, (although these constraints have recently been reanalyzed and found to be weaker; see [80] for more details), NA62 [81], CHARM [82], BEBC [83,84], Belle [43], DEL-PHI [85], and ATLAS [86] for electron-mixed HNLs; E949 [87], PS191 [13,14], T2K [16,17], NuTeV [88], CHARM [89], Belle [43], DELPHI [85], and ATLAS [86] for muon-mixed HNLS; and NOMAD [15], CHARM [12,15,90], BEBC [84], ArgoNeuT [20], and DELPHI [85] for τ -mixed HNLs. The shaded blue regions at small mixing angles are additional constraints from Big Bang nucleosynthesis (BBN) studies [91,92].…”