  The physics program of ultra-relativistic heavy-ion collisions at the Large
Hadron Collider (LHC) and Relativistic Heavy-Ion Collider (RHIC) has brought a
unique insight into the hot and dense QCD matter created in such collisions,
the Quark-Gluon Plasma (QGP). Jet quenching, a collection of medium-induced
modifications of the jets' internal structure that occur through their
development in dense QCD matter, has a unique potential to assess the time
structure of the produced medium. In this work, we perform an exploratory study
to identify jet reclustering tools that can potentiate future QGP tomographic
measurements with jets at current energies. Our results show that by using the
inverse of formation time to obtain the jet clustering history, one can
identify more accurately the time structure of QCD emissions inside jets, even
in the presence of jet quenching.
