Abstract
Short gamma-ray bursts (sGRB) are among the most energetic phenomena in the Universe. sGRBs go through two important stages during their lifetime, which are referred to as the "prompt emission" and "afterglow." Prompt emissions last in the order of seconds, afterglows can last for months, which allows us to follow sGRB’s extensively and use them to infer physical parameters of the explosion and its environment. However, given that most sGRBs are not directed straight toward us, we study the properties of sGRBs afterglows at various observer angles. It is imperative that we consider how the jet properties change as a function of the angle between the burst axis and the observer in order to garner relevant information on the nature of short gamma-ray bursts as a whole.