LOFAR Low-Band Array (LBA) is capable of observing objects at frequencies between 10 and 80 MHz. At these frequencies, the main challenge is calibrating all antennas for effects from the ionosphere.
Although a lot of work has already been done between 40-70 MHz (for example, LoLSS), the lower frequency part (15-30 MHz) have yet to see extensive exploration. By pushing current calibration strategies to their limits, we can open up this new window to the universe.