  We have performed a molecular line search toward the flaring 6.7-GHz masers
G24.33+0.13 and G359.62-0.24 using the Australia Telescope Compact Array. We
present spectra of the 6.7-GHz class~II methanol and 22.2-GHz water masers
toward these sources and provide comparison with other recent flaring events
these sources have experienced. We also detect the fourth example of a 23.4-GHz
class~I methanol maser, and the eleventh example of a 4.8-GHz formaldehyde
maser toward G24.33+0.13. Alongside these results, we observe the previously
detected ammonia (3,3) emission and report upper limits on the presence of
various other cm-wavelength methanol, ammonia and OH transitions. Our results
are consistent with the flaring of G24.33+0.13 being driven by a variable
accretion rate in the host high-mass young stellar object.
