Gamma-ray Transients Monitor(GTM) is the first space astronomical telescope of Taiwan.

[1] The goal of GTM is to track Gamma Ray Bursts (GRBs) and other bright gamma-ray transients with energies ranging from 50 keV to 2 MeV.

[1] The repository that stores the code for Science Data Center (SDC) of Gamma-ray Transients Monitor is on GitHub.

However, there is significant overlap in the duration comparison of SGRBs and LGRBs, complicating a clear distinction between the two types of GRBs.

Actually, many other classification methods, such as hardness ratio, time and lag, encounter overlapping issues.