Correction to: Why the observed spin evolution of older-than-solar-like stars might not require a dynamo mode change.

This document is a correction to a previously published paper titled "Why the observed spin evolution of older-than-solar-like stars might not require a dynamo mode change." The correction addresses minor typographical errors that do not impact the results of the paper but could cause confusion in reproducing the calculations. Specifically, the correction involves changing the notation for stellar mass and radius in subsection 2.3. The corrected notation uses m⊙* and r⊙* to represent normalized values to solar mass and solar radius. The authors of the paper are Ketevan Kotorashvili, Eric G Blackman, and James E Owen. [Extracted from the article]