Table 2: Lower lifetime limits $T_{\rm {min}}$ at different significance levels for 1612 MHz OH masers based on observations in this paper. Pnm is the probability for finding exactly m extinguished maser among n stars reobserved after $\Delta t$ years.
n m $\Delta t$ $T_{\rm {min}}$ Pnm Comments
    [yr] [yr] [%]    
114 0 28 550 0.2 3$\sigma $ This paper
114 0 28 1050 4.6 2$\sigma $  
114 0 28 2800 31.8 1$\sigma $  

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