  Ellerman bombs (EBs) are small-scale intense brightenings in H$\alpha$ wing
images, which are generally believed to be signatures of magnetic reconnection
events around the temperature minimum region of the solar atmosphere. They have
a flame-like morphology when observed near the solar limb. Recent observations
from the Interface Region Imaging Spectrograph (IRIS) reveal another type of
small-scale reconnection events, termed UV bursts, in the lower atmosphere.
Though previous observations have shown a clear coincidence of some UV bursts
and EBs, the exact relationship between these two phenomena is still under
debate. We investigate the spatial and temporal relationship between flame-like
EBs and UV bursts using joint near-limb observations between the 1.6--meter
Goode Solar Telescope (GST) and IRIS. In total 161 EBs have been identified
from the GST observations, and 20 of them reveal signatures of UV bursts in the
IRIS images. Interestingly, we find that these UV bursts have a tendency to
appear at the upper parts of their associated flame-like EBs. The intensity
variations of most EB-related UV bursts and their corresponding EBs match well.
Our results suggest that these UV bursts and EBs are likely formed at different
heights during a common reconnection process.
