Some of the most luminous transient radio sources can be produced if a jet is launched as a star is ripped apart by a supermassive black hole (SMBH) creating a tidal disruption event (TDE). As the star approaches the SMBH, intense tidal forces overcome the gravity keeping the star together. Approximately half of the disrupted material is thought to be lost and the other half falls back and is accreted onto the SMBH. In some fraction of TDEs (five are known of so far), a relativistic jet is launched analogous to those launched from stellar mass black holes. I am interested in studying variance in the long term behaviour of jetted TDEs and searching for possible transient jet invariance across black hole mass.