672
JOHN ALROY Höhle and Held (2006) went on from
Goodman’s equation to present a formula that yields each interval’s posterior extinction prob- ability given that the species is extinct, period (because they envisioned examining an infinite series of observations). Equation (3) (Alroy 2015) additionally incorporates a term that captures the hypothesis of survival up to the end of the observation period, that is, the product P(A)P(D|A) that includes the 0.5 prior. So, it builds in complete uncertainty about whether extinction has happened in the first place. I therefore suggest calling it an agnostic extinction equation. The method as described to this point
assumes a uniform distribution of extinction probabilities through time, which is simply not realistic. Instead, if all other things are equal, then it makes sense to assume that extinction is an exponential process (as also assumed by Alroy [2014]). For example, if half of the population dies each year, then we expect one-quarter to survive 2 years and therefore one-quarter to have died in the second year; one-eighth to survive 3 years and therefore one-eighth to die in the third year; and so on. Switching to an exponential model only requires treating the P(Ei) term in equation (3) as a changing variable that depends on the time interval number i. Specifically, the function is:
PðEiÞ=exp½μði1ÞμexpðμiÞ (6)
where μ=the per-interval instantaneous extinction rate, which is log(0.5)/N on the aforementioned assumption that there is a 50% chance of surviving to the end of the observa- tion period. Note that if some other prior is used, then μ=log[P(A)]/N, not log(0.5)/N. Another concern is the fact that when real
extinction rates are minuscule, employing a 0.5 value for the overall prior P(E) creates a strong upward bias in the P(E|D) posteriors. There is no real solution to this problem if a single species is being analyzed. However, if the data set consists of a substantial popula- tion, then one possibility would be to compute a mean posterior for the population and then recycle the mean as a new prior and recompute all the individual posteriors using it
(Alroy 2015). As shown later, when the rate is very close to zero, recycling produces much better results than using a 0.5 prior. There is also a noticeable improvement when extinction rates are moderate, which is the case inmost of the simulations. Solow (2016) also developed an equation
that eliminates sampling probabilities by conditioning on the number of sightings. His method and mine (Alroy 2015), which were developed independently, both stem from the work of Goodman (1952) and Höhle and Held (2006). However, Solow’s method is biased and unrealistic because of the way its prior is formulated (Alroy 2016), and so it does not merit detailed discussion. Because the agnostic method and CSD are
both Bayesian and both simple, there is some chance of assuming that they are somehow related on a mathematical level. It must be emphasized that they are not. First, obviously, the new equation involves combinatorics instead of sampling probabilities. Second, the computa- tion is not iterative: equation (3) is applied separately to each interval, and no attention is paid to the values for the other intervals. Third and last, the extinction prior is 0.5 for the entire time series of N intervals, instead of being 0.5 at interval L. In practice, because intervals before L have zero priors, the actual overall prior is (N − L)/2N. For example, if L=10 and N=10, then the overall prior is zero for every interval based on this newmethod, but 0.5 based onCSD (despite the fact that the posterior is zero according to both methods). Calculations for cases where N > L are highly complicated, but regardless, the values produced by the two methods still come out differently. In sum, there is no connection whatsoever
between the agnostic and CSD methods except that they are Bayesian and highly accurate. The method of Solow (2016) is actually more related on a conceptual level. That said, CSD has a number of advantages over all other methods with respect to the way it handles complexities in the data (Alroy 2014). Most of these advantages are also shared by the new method.
1. When CSD is used, the prior extinction rate depends on whether the entire
Page 1 |
Page 2 |
Page 3 |
Page 4 |
Page 5 |
Page 6 |
Page 7 |
Page 8 |
Page 9 |
Page 10 |
Page 11 |
Page 12 |
Page 13 |
Page 14 |
Page 15 |
Page 16 |
Page 17 |
Page 18 |
Page 19 |
Page 20 |
Page 21 |
Page 22 |
Page 23 |
Page 24 |
Page 25 |
Page 26 |
Page 27 |
Page 28 |
Page 29 |
Page 30 |
Page 31 |
Page 32 |
Page 33 |
Page 34 |
Page 35 |
Page 36 |
Page 37 |
Page 38 |
Page 39 |
Page 40 |
Page 41 |
Page 42 |
Page 43 |
Page 44 |
Page 45 |
Page 46 |
Page 47 |
Page 48 |
Page 49 |
Page 50 |
Page 51 |
Page 52 |
Page 53 |
Page 54 |
Page 55 |
Page 56 |
Page 57 |
Page 58 |
Page 59 |
Page 60 |
Page 61 |
Page 62 |
Page 63 |
Page 64 |
Page 65 |
Page 66 |
Page 67 |
Page 68 |
Page 69 |
Page 70 |
Page 71 |
Page 72 |
Page 73 |
Page 74 |
Page 75 |
Page 76 |
Page 77 |
Page 78 |
Page 79 |
Page 80 |
Page 81 |
Page 82 |
Page 83 |
Page 84 |
Page 85 |
Page 86 |
Page 87 |
Page 88 |
Page 89 |
Page 90 |
Page 91 |
Page 92 |
Page 93 |
Page 94 |
Page 95 |
Page 96 |
Page 97 |
Page 98 |
Page 99 |
Page 100 |
Page 101 |
Page 102 |
Page 103 |
Page 104 |
Page 105 |
Page 106 |
Page 107 |
Page 108 |
Page 109 |
Page 110 |
Page 111 |
Page 112 |
Page 113 |
Page 114 |
Page 115 |
Page 116 |
Page 117 |
Page 118 |
Page 119 |
Page 120 |
Page 121 |
Page 122 |
Page 123 |
Page 124 |
Page 125 |
Page 126 |
Page 127 |
Page 128 |
Page 129 |
Page 130 |
Page 131 |
Page 132 |
Page 133 |
Page 134 |
Page 135 |
Page 136 |
Page 137 |
Page 138 |
Page 139 |
Page 140 |
Page 141 |
Page 142 |
Page 143 |
Page 144 |
Page 145 |
Page 146 |
Page 147 |
Page 148 |
Page 149 |
Page 150 |
Page 151 |
Page 152 |
Page 153 |
Page 154 |
Page 155 |
Page 156 |
Page 157 |
Page 158 |
Page 159 |
Page 160 |
Page 161 |
Page 162 |
Page 163 |
Page 164 |
Page 165 |
Page 166 |
Page 167 |
Page 168 |
Page 169 |
Page 170 |
Page 171 |
Page 172 |
Page 173 |
Page 174 |
Page 175 |
Page 176 |
Page 177 |
Page 178 |
Page 179 |
Page 180 |
Page 181 |
Page 182 |
Page 183 |
Page 184 |
Page 185 |
Page 186 |
Page 187 |
Page 188 |
Page 189 |
Page 190 |
Page 191 |
Page 192