This article contains lists of quasars. More than a million quasars have been observed, so any list on Wikipedia is necessarily a selection of them.
Proper naming of quasars are by Catalogue Entry, Qxxxx±yy using B1950 coordinates, or QSO Jxxxx±yyyy using J2000 coordinates. They may also use the prefix QSR. There are currently no quasars that are visible to the naked eye.
This is a list of exceptional quasars for characteristics otherwise not separately listed
This is a list of quasars, with a common name, instead of a designation from a survey, catalogue or list.
This is a list of quasars that as a result of gravitational lensing appear as multiple images on Earth.
This is a list of double quasars, triple quasars, and the like, where quasars are close together in line-of-sight, but not physically related.
This is a list of binary quasars, trinary quasars, and the like, where quasars are physically close to each other.
Large quasar groups (LQGs) are bound to a filament of mass, and not directly bound to each other.
This is a list of quasars with jets that appear to be superluminal due to relativistic effects and line-of-sight orientation. Such quasars are sometimes referred to as superluminal quasars.
Quasars that have a recessional velocity greater than the speed of light (c) are very common. Any quasar with z > 1 is receding faster than c, while z exactly equal to 1 indicates recession at the speed of light. Early attempts to explain superluminal quasars resulted in convoluted explanations with a limit of z = 2.326, or in the extreme z