An introduction to Bayesian inference in gravitational-wave astronomy: parameter estimation, model selection, and hierarchical models—Corrigendum
An introduction to Bayesian inference in gravitational-wave astronomy: parameter estimation, model selection, and hierarchical models—Corrigendum
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DOI:
10.1017/pasa.2020.23
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发表时间:
2020-09
影响因子:
6.3
通讯作者:
E. Thrane;C. Talbot
中科院分区:
文献类型:
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作者:
E. Thrane;C. Talbot
1. In the original version of this article, we included a subsection in Appendix E, “Selection effects with a single event.” This section included formulas with errors including Eq. 89 and Eq. 95 of the arxiv version (Eq. E2 and Eq. E8 in the version published in PASA). Moreover, the section included a conceptual error since the idea of selection effects for single events does not make sense. Selection effects are intrinsically related to population studies, so they simply do not affect the analysis of single detections. It is interesting to consider how this comes about mathematically. While the single-event det likelihood gains a factor of p−1 det (as correctly noted in the original article), the single-event det prior picks up a compensating factor of pdet, because the prior for detected events is not the same as the original (no det) prior. Since the det posterior is proportional to the product of the likelihood and the prior, these two factors cancel, giving the original (no det) likelihood. A revised version of the appendix is presented below. 2. In eight places we referred to “the odds ratio.” However, we should have referred simply to “the odds.” In statistics, the odds refers to a ratio of probabilities. When we multiply the Bayes factor by the prior odds, we obtain the posterior odds. The odds ratio, which is also a statistical term, refers to a ratio of ratios.