ƒobs = òò sSN(r) p(x,y,t) dA dt / (SSNƒHI t)

• ƒobs = òò sSN(r) p(x,y,t) dA dt / (SSNƒHI t)

  • detection probability p = pGB ´ pTS
  • pGB(x,y,t): Galactic background contamination
    • pGB = 1 if vSNR ±|vs|> vl,max+50 km/s or < vl,min-50 km/s
    • 0 otherwise
  • pTS(x,y,t): telescope sensitivity
    • Flux unlimited: pGB = 1
    • Flux limited: pGB = 1 if d<dmax(DTA, Aeff ; Ms(t))
    • 0 otherwise
    • Ms(t), t: SNR dynamics

Notes: