Choose the potential right-censoring times to include every observed right censoring time up to , and also the endpoints 0 and . Then no individual is censored strictly inside . Use an explicit endpoint convention: let count individuals still event-free after any events at , but before censoring at . If events occur in , the number at the beginning of that interval, after censoring at its left endpoint, is .
The no-censoring interval estimate from the preceding parts is therefore . The possible event mass at zero contributes . Multiplying yields
For a continuous event-time distribution, normally . Within interval , put and let its successive event counts be . Its Kaplan–Meier estimator factors telescope:
The same calculation at zero proves
The paper's phrase “at risk at ” does not specify its side of an event at that endpoint. If it denotes the conventional pre-event risk set size instead, and events occur exactly at , substitute . The interval factor is then ; at zero it is . This keeps the events-before-censoring convention consistent. After an empty risk set, stop the product; if the fitted survival has reached zero, retain zero rather than creating a factor.