A preprint study on arXiv (https://arxiv.org/abs/2603.24673), not yet peer-reviewed, reports results from a multi-cycle Chandra X-ray Observatory program that systematically monitored 10 weak-line quasars (WLQs). These are unusual quasars with very weak ultraviolet emission lines. Researchers obtained three new Chandra observations for each object, with exposure times ranging from 2.8 to 8.2 kiloseconds, substantially improving the available multi-epoch X-ray data. They observed recurrent extreme variability in one quasar that brightened by a factor of at least 6 between 2023 and 2024, and another that varied by a factor of at least 14 between 2019 and 2023. With a small sample size of only 10 WLQs, the fraction showing such extreme variability is estimated at 0.20 with sizable uncertainty. Limitations include the modest sample, which restricts how broadly the findings can be applied. The study also found WLQs have roughly 6.8 times higher odds of extreme X-ray variability events than typical radio-quiet quasars.