List of quasars
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 is 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.
List of quasars
This is a list of exceptional quasars for characteristics otherwise not separately listed| Quasar | Notes |
| Twin Quasar | Associated with a possible planet microlensing event in the gravitational lens galaxy that is doubling the Twin Quasar's image. |
| QSR J1819+3845 | Proved interstellar scintillation due to the interstellar medium. |
| CTA-102 | In 1965, Soviet astronomer Nikolai S. Kardashev posited that this quasar could be the source of signals from an alien civilization. |
| CID-42 | Its supermassive black hole is being ejected and will one day become a displaced quasar. |
| TON 618 | TON 618 is a very distant and extremely luminous quasar—technically, a hyperluminous, broad-absorption line, radio-loud quasar—located near the North Galactic Pole in the constellation Canes Venatici. |
List of named quasars
This is a list of quasars, with a common name, instead of a designation from a survey, catalogue or list.| Quasar | Origin of name | Notes |
| Twin Quasar | From the fact that two images of the same quasar are produced by gravitational lensing. | |
| Einstein Cross | From the fact that gravitational lensing of the quasar forms a near perfect Einstein cross, a concept in gravitational lensing. | |
| From the fact that there are three bright images of the same gravitationally lensed quasar. | There are actually four images; the fourth is faint. | |
| Cloverleaf | From its appearance having similarity to the leaf of a clover. It has been gravitationally lensed into four images, of roughly similar appearance. | |
| Teacup Galaxy | The name comes from the shape of the extended emission, which is shaped like the handle of a teacup. The handle is a bubble shaped by quasar winds or small-scale radio jets. | Low redshift, highly obscured type 2 quasar. |
| Pōniuāʻena | The third most distant quasar known as of 2025, named for its early formation at most 100 million years after the Big Bang. | Named as part of the A Hua He Inoa program by the ʻImiloa Astronomy Center. |
List of multiply imaged quasars
This is a list of quasars that as a result of gravitational lensing appear as multiple images on Earth.| Quasar | Images | Lens | Notes |
| Twin Quasar | 2 | YGKOW G1 | First gravitationally lensed object discovered |
| Triple Quasar | 4 | Originally discovered as 3 lensed images, the fourth image is faint. It was the second gravitationally lensed quasar discovered. | |
| Einstein Cross | 4 | Huchra's Lens | First Einstein Cross discovered |
| RX J1131-1231's quasar | 4 | RX J1131-1231's elliptical galaxy | RX J1131-1231 is the name of the complex, quasar, host galaxy and lensing galaxy, together. The quasar's host galaxy is also lensed into a Chwolson ring about the lensing galaxy. The four images of the quasar are embedded in the ring image. |
| Cloverleaf | 4 | Brightest known high-redshift source of CO emission | |
| QSO B1359+154 | 6 | CLASS B1359+154 and three more galaxies | First sextuply-imaged galaxy |
| SDSS J1004+4112 | 5 | Galaxy cluster at z = 0.68 | First quasar discovered to be multiply image-lensed by a galaxy cluster and currently the third largest quasar lens with the separation between images of 15 |
| SDSS J1029+2623 | 3 | Galaxy cluster at z = 0.6 | The current largest-separation quasar lens with 22.6 separation between furthest images |
| SDSS J2222+2745 | 6 | Galaxy cluster at z = 0.49 | First sextuply-lensed galaxy Third quasar discovered to be lensed by a galaxy cluster. Quasar located at z = 2.82 |
| RX J0911.4+0551 | 4 | Galaxy located at z = 0.76 | Gravitationally lensed object discovered by the ROSAT All-Sky survey in 1997. Quasar located at z = 2.800. |
| CLASS B1152+199 | 2 | Galaxy located at z = 0.43 | |
| HE 1104-1805 | 2 | Galaxy located at z = 0.72 | Also known as Double Hamburger. |
| HE 2149-2745 | 2 | Galaxy at z = 0.60 | Gravitationally lensed broad absorption object at z = 2.033 |
| FBQ 0951+2635 | 2 | Galaxy located at z = 0.26 | |
| HE0435-1223 | 4 | Elliptical galaxy of HE0435-1223 at z = 0.45 | Quasar located at z = 1.689. Components arranged in cross figuration. |
| SBS 0909+532 | 2 | Lens galaxy of SBS 0909+532 at z = 0.83 | Originally interpreted as a binary quasar but later revealed as a gravitationally lensed object. |
| UM 673 | 2 | Lens galaxy at z = 0.49 | Quasar located at at z = 2.71, first discovered by J. Surdej |
| CTQ 327 | 2 | Lens galaxy between z = 0.4 and z= 0.6 | |
| CTQ 414 | 2 | Discovered in 1999. Quasar located at z = 1.29. | |
| HE 0230-2130 | 5 | Complex lensed system. Quasar located at z = 2.130. | |
| SDSS J1001+5027 | 2 | Lens galaxy at z = 0.3 | |
| SDSS J1206+4332 | 2 | Lens galaxy at z = 0.74 | |
| SDSS J0246-0825 | 2 | Lens galaxy at z = 0.724 | Discovered by Scott Burles. |
| SDSS J0904+1512 | 2 | Discovered in the SDSS Quasar Lens Search | |
| SDSS J1054+2733 | 2 | Discovered in the SDSS Quasar Lens Search | |
| SDSS J1620+1203 | 2 | Lens galaxy at z = 0.39 | Discovered in the SDSS Quasar Lens Search. Quasar located at z = 1.158 |
| SDSS J0746+4403 | 2 | Lens galaxy at z = 0.513 | Discovered in 2007. Quasar located at z = 2.00 |
List of visual quasar associations
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.List of physical quasar groups
This is a list of binary quasars, trinary quasars, and the like, where quasars are physically close to each other.| Quasars | Count | Notes | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| quasars of SDSS J0841+3921 protocluster | 4 | First quasar quartet discovered. | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| LBQS 1429-008 | 3 | First quasar triplet discovered. It was first discovered as a binary quasar, before the third quasar was found. | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
QQ2345+007Large Quasar GroupsLarge quasar groups are bound to a filament of mass, and not directly bound to each other.
List of quasars with apparent superluminal jet motionThis 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 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 < 2.4. The majority of quasars lie between z = 2 and z = 5. Most distant quasarsIn 1964 a quasar became the most distant object in the universe for the first time. Quasars would remain the most distant objects in the universe until 1997, when a pair of non-quasar galaxies would take the title.In cosmic scales distance is usually indicated by redshift which is a measure of recessional velocity and inferred distance due to cosmological expansion.
Most powerful quasars
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