Radio emissions under 5 GHz provide a unique look at stellar and exoplanetary
physical mechanisms, as they are often associated with flares and magnetic
phenomena in our Solar System. However, there are still few such low-frequency
detections throughout the galaxy. In order to add new discoveries and to
test different physical situations, we utilized publicly available
low-frequency radio sky surveys to cross match the positions of exoplanets,
young stars, and nearby mature stars. We have found 11 candidate detections,
some of which are redetections of known radio stars, while others
are brand new low-frequency radio detections. These candidates will
be discussed, along with analyses of the samples as a whole.