Publications by authors named "S C Vermeulen"

The bacterial microbiome of the ant has been well characterized across body regions and maturation levels. However, potential effects of entomopathogens on the gut microbiome, and the fungal communities therein, are yet to be assessed. Additionally, the mycobiome remains often overlooked despite playing a vital role in gut ecology with potential implications for health and infection outcomes.

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Taxanes, such as paclitaxel (PTX), stabilize microtubules and are used as a first-line therapy in multiple cancer types. Disruption of microtubule equilibrium, which plays an essential role in mitosis and cell homeostasis, ultimately results in cell death. Even though PTX is a very potent chemotherapy, its use is associated with major side effects and therapy resistance.

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Article Synopsis
  • The study focuses on improving the quantification of phages for personalized therapy and industrial use, highlighting that the traditional culture-based method is accurate but time-consuming.
  • A DNase treatment before using quantitative polymerase chain reaction (qPCR) is proposed to enhance the accuracy of phage quantification, though qPCR still tends to overestimate compared to the gold standard method.
  • Findings indicate that the differences in phage quantification methods vary based on the age of the phage stocks, and electron microscopy confirmed the presence of free DNA influencing the results.
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De Bleecker, C, Vermeulen, S, Willems, T, Segers, V, Spanhove, V, Leys, R, Vanrenterghem, J, and De Ridder, R. Validation of impact forces estimated by wearable device VERT in volleyball validation impact forces VERT. J Strength Cond Res XX(X): 000-000, 2024-As volleyball players are exposed to high volumes of forceful jump-landing actions, the risk of injuries is increased.

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The most massive black holes in our Universe form binaries at the centre of merging galaxies. The recent evidence for a gravitational-wave (GW) background from pulsar timing may constitute the first observation that these supermassive black-hole binaries (SMBHBs) merge. Yet, the most massive SMBHBs are out of reach of interferometric GW detectors and are exceedingly difficult to resolve individually with pulsar timing.

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