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Using data from the Two Micron All Sky Survey, we identify a population of infrared carbon stars with J-KS ≥ 2 in the Milky Way. These stars are shown to trace the stellar bar previously identified in...
Implementation of upper limit calculation for a Poisson variable by Bayesian approach
upper limit systematic uncertainties Poisson distribution Bayesian statistics
2009/7/31
The calculation of Bayesian confidence upper limit for a Poisson variable including both signal and background with and without
systematic uncertainties has been formulated. A Fortran 77 routine, BPU...