Context. Images of spatially resolved astrophysical objects contain a wealth of morphological and dynamical information, and effectively extracting this information is of paramount importance for understanding the physics and evolution of these objects. The algorithms and methods currently employed for this purpose (such as Gaussian model fitting) often use simplified approaches to describe the structure of resolved objects.
No takes yet. Share an insight, caveat, or question.
A 2014 study studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: