# 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 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.

## 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 declared that this quasar was sending coded messages 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. |
| RT679 BLZ-1 | RT679 BLZ-1 is a Bright Spiral SBa Galaxy is a Quasar/Blazar Discovered from ESO and NASA Close to Twin Quasar |

## 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. | |
| Triple Quasar | 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. |

## 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 (PG 1115+080) | 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 |

## 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.
| Quasars | Count |
| QSO 1548+115 4C 11.50 (z = 0.436) QSO B1548+115B (z = 1.901) | 2 |
| QSO 1146+111 | 8 |
| z represents redshift, a measure of recessional velocity and inferred distance due to cosmological expansion |||

## 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 (QQQ 1432-0106) | 3 | First quasar triplet discovered. It was first discovered as a binary quasar, before the third quasar was found. |
| QQ2345+007 (Q2345+007) Q2345+007A Q2345+007B | 2 | Originally thought to be a doubly imaged quasar, but actually a quasar couplet. |
| QQQ J1519+0627 | 3 | |

### Large Quasar Groups

Large quasar groups (LQGs) are bound to a filament of mass, and not directly bound to each other.
| LQG | Count | Notes |
| Webster LQG (LQG 1) | 5 | First LQG discovered. At the time of its discovery, it was the largest structure known. |
| Huge-LQG (U1.27) | 73 | The largest structure known in the observable universe, as of 2013. |

## List of quasars with apparent superluminal jet motion

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.
| Quasar | Superluminality | Notes |
| 3C 279 | 4c | First quasar discovered with superluminal jets |
| 3C 179 | 7.6c | Fifth discovered, first with double lobes |
| 3C 273 | | This is also the first quasar ever identified |
| 3C 216 | | |
| 3C 345 | | |
| 3C 380 | | |
| 4C 69.21 (Q1642+690, QSO B1642+690) | | |
| 8C 1928+738 (Q1928+738, QSO J1927+73, Quasar J192748.6+735802) | | |
| PKS 0637-752 | | |
| QSO B1642+690 | | |
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 < 2.4. The majority of quasars lie between z = 2 and z = 5.

## Firsts

| Title | Quasar | Year | Data | Notes |
| First quasar discovered | 3C 48 | 1960 | | first radio source for which optical identification was found, that was a star-like looking object |
| First "star" discovered later found to be a quasar | 3C 48 | 1960 | | first radio source for which optical identification was found, that was a star-like looking object |
| First radio source discovered later found to be a quasar | 3C 48 | 1960 | | first radio source for which optical identification was found, that was a star-like looking object |
| First quasar identified | 3C 273 | 1962 | | first radio-"star" found to be at a high redshift with a non-stellar spectrum. |
| First radio-quiet quasar | QSO B1246+377 (BSO 1) | 1965 | | The first radio-quiet quasi-stellar objects (QSO) were called Blue Stellar Objects or BSO, because they appeared like stars and were blue in color. They also had spectra and redshifts like radio-loud quasi-stellar radio-sources (QSR), so became quasars. |
| First host galaxy of a quasar discovered | 3C 48 | 1982 | | |
| First quasar found to seemingly not have a host galaxy | HE0450-2958 (Naked Quasar) | 2005 | | Some disputed observations suggest a host galaxy, others do not. |
| First multi-core quasar | PG 1302-102 | 2014 | Binary supermassive black holes within the quasar | |
| First quasar containing a recoiling supermassive black hole | SDSS J0927+2943 | 2008 | | Two optical emission line systems separated by 2650 km/s |
| First gravitationally lensed quasar identified | Twin Quasar | 1979 | Lensed into 2 images | The lens is a galaxy known as YGKOW G1 |
| First quasar found with a jet with apparent superluminal motion | 3C 279 | 1971 | | |
| First quasar found with the classic double radio-lobe structure | 3C 47 | 1964 | | |
| First quasar found to be an X-ray source | 3C 273 | 1967 | | |
| First "dustless" quasar found | QSO J0303-0019 and QSO J0005-0006 | 2010 | | |
| First Large Quasar Group discovered | Webster LQG (LQG 1) | 1982 | | |

## Extremes

| Title | Quasar | Data | Notes |
| Brightest | 3C 273 | Apparent magnitude of ~12.9 | Absolute magnitude: −26.7 |
| Seemingly optically brightest | APM 08279+5255 | Seeming absolute magnitude of −32.2 | This quasar is gravitationally lensed; its actual absolute magnitude is estimated to be −30.5 |
| Most luminous | SMSS J215728.21-360215.1 | Absolute magnitude of −32.36 | Highest absolute magnitude discovered thus far. |
| Most powerful quasar radio source | 3C 273 | | Also the most powerful radio source in the sky |
| Most powerful | SMSS J215728.21-360215.1 | | |
| Most variable quasar radio source | QSO J1819+3845 (Q1817+387) | | Also the most variable extrasolar radio source |
| Least variable quasar radio source | | | |
| Most variable quasar optical source | | | |
| Least variable quasar optical source | | | |
| Most distant | UHZ1 | z = 10.1 | Most distant quasar known as of 2023 |
| Most distant radio-quiet quasar | | | |
| Most distant radio-loud quasar | QSO J1427+3312 | z = 6.12 | Found June 2008 |
| Most distant blazar quasar | PSO J0309+27 | z > 6 | |
| Least distant | Markarian 231 | 600 Mly | inactive: IC 2497 |
| Largest Large Quasar Group | Huge-LQG (U1.27) | 73 quasars | |
| Fastest Growing Quasar | SMSS J052915.80–435152.0 (QSO J0529-4351) | ~ 413 solar masses per year (using standard radiative efficiency); ~ 370 solar masses per year (using best-fit slim disc model) | |

## First quasars found

First 10 Quasars Identified :
| Rank | Quasar | Date of discovery |
| 1 | 3C 273 | 1963 |
| 2 | 3C 48 | 1963 |
| 3 | 3C 47 | 1964 |
| 3 | 3C 147 | 1964 |
| 5 | CTA 102 | 1965 |
| 5 | 3C 287 | 1965 |
| 5 | 3C 254 | 1965 |
| 5 | 3C 245 | 1965 |
| 5 | 3C 9 | 1965 |
| These are the first quasars which were found and had their redshifts determined. ||||

## Most distant quasars

In 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 (galaxies CL 1358+62 G1 & CL 1358+62 G2 lensed by galaxy cluster CL 1358+62).
In cosmic scales distance is usually indicated by redshift (denoted by z) which is a measure of recessional velocity and inferred distance due to cosmological expansion.
Quasars with z > 6 :
| Quasar | Distance | Notes |
| UHZ1 | z = 10.1 | Most distant quasar known as of 2023 |
| QSO J0313–1806 | z = 7.64 | Former most distant quasar. |
| ULAS J1342+0928 | z = 7.54 | Former most distant quasar. |
| J1007+2115 (Pōniuāʻena) | z = 7.52 | |
| ULAS J1120+0641 (ULAS J112001.48+064124.3) | z = 7.085 | Former most distant quasar. First quasar with z > 7. |
| CHFQS J2348-3054 (CHFQS J234833.34-305410.0) | z = 6.90 | |
| PSO J172.3556+18.7734 | z = 6.82 | Currently the most distant radio-loud known quasar |
| CFHQS J2329-0301 (CFHQS J232908-030158) | z = 6.43 | Former most distant quasar. |
| SDSS J114816.64+525150.3 (SDSS J1148+5251) | z = 6.419 | Former most distant quasar. |
| SDSS J1030+0524 (SDSSp J103027.10+052455.0) | z = 6.28 | Former most distant quasar. First quasar with z > 6. |
| SDSS J104845.05+463718.3 (QSO J1048+4637) | z = 6.23 | |
| SDSS J162331.81+311200.5 (QSO J1623+3112) | z = 6.22 | |
| CFHQS J0033-0125 (CFHQS J003311-012524) | z = 6.13 | |
| SDSS J125051.93+313021.9 (QSO J1250+3130) | z = 6.13 | |
| CFHQS J1509-1749 (CFHQS J150941-174926) | z = 6.12 | |
| QSO B1425+3326 / QSO J1427+3312 | z = 6.12 | Most distant radio-quasar. |
| SDSS J160253.98+422824.9 (QSO J1602+4228) | z = 6.07 | |
| SDSS J163033.90+401209.6 (QSO J1630+4012) | z = 6.05 | |
| CFHQS J1641+3755 (CFHQS J164121+375520) | z = 6.04 | |
| SDSS J113717.73+354956.9 (QSO J1137+3549) | z = 6.01 | |
| SDSS J081827.40+172251.8 (QSO J0818+1722) | z = 6.00 | |
| SDSSp J130608.26+035626.3 (QSO J1306+0356) | z = 5.99 | |
| z > 6 quasars are used to explore the reionization era |||
Most Distant Quasar by Type :
| Type | Quasar | Date | Distance |
| Most distant | UHZ1 | 2023 | z = 10.2 |
| Most distant radio loud quasar | QSO B1425+3326 / QSO J1427+3312 | 2008 | z = 6.12 |
| Most distant radio quiet quasar | | | |
| Most distant OVV quasar | | | |
Most Distant Quasar Titleholders :
| Quasar | Date | Distance | Notes |
| UHZ1 | 2023– | z = 10.2 | Current distance record holder |
| QSO J0313−1806 | 2021–2023 | z = 7.64 | |
| ULAS J1342+0928 | 2017–2021 | z = 7.54 | |
| ULAS J1120+0641 | 2011–2017 | z = 7.085 | Not the most distant object when discovered. First quasar with z > 7. |
| CFHQS J2329-0301 (CFHQS J232908-030158) | 2007–2011 | z = 6.43 | Not the most distant object when discovered. It did not exceed IOK-1 (z = 6.96), which was discovered in 2006. |
| SDSS J114816.64+525150.3 (SDSS J1148+5251) | 2003–2007 | z = 6.419 | Not the most distant object when discovered. It did not exceed HCM 6A galaxy lensed by Abell 370 at z = 6.56, discovered in 2002. Also discovered around the time of discovery was a new most distant galaxy, SDF J132418.3+271455 at z = 6.58. |
| SDSS J1030+0524 (SDSSp J103027.10+052455.0) | 2001–2003 | z = 6.28 | Most distant object when discovered. First object with z > 6. |
| SDSS 1044-0125 (SDSSp J104433.04-012502.2) | 2000–2001 | z = 5.82 | Most distant object when discovered. It exceeded galaxy SSA22-HCM1 (z = 5.74; discovered in 1999) as the most distant object. |
| RD300 (RD J030117+002025) | 2000 | z = 5.50 | Not the most distant object when discovered. It did not surpass galaxy SSA22-HCM1 (z = 5.74; discovered in 1999). |
| SDSSp J120441.73−002149.6 (SDSS J1204-0021) | 2000 | z = 5.03 | Not the most distant object when discovered. It did not surpass galaxy SSA22-HCM1 (z = 5.74; discovered in 1999). |
| SDSSp J033829.31+002156.3 (QSO J0338+0021) | 1998–2000 | z = 5.00 | First quasar discovered with z > 5. Not the most distant object when discovered. It did not surpass galaxy BR1202-0725 LAE (z = 5.64; discovered earlier in 1998). |
| PC 1247+3406 | 1991–1998 | z = 4.897 | Most distant object when discovered. |
| PC 1158+4635 | 1989–1991 | z = 4.73 | Most distant object when discovered. |
| Q0051-279 | 1987–1989 | z = 4.43 | Most distant object when discovered. |
| Q0000-26 (QSO B0000-26) | 1987 | z = 4.11 | Most distant object when discovered. |
| PC 0910+5625 (QSO B0910+5625) | 1987 | z = 4.04 | Most distant object when discovered; second quasar with z > 4. |
| Q0046–293 (QSO J0048-2903) | 1987 | z = 4.01 | Most distant object when discovered; first quasar with z > 4. |
| Q1208+1011 (QSO B1208+1011) | 1986–1987 | z = 3.80 | Most distant object when discovered and a gravitationally-lensed double-image quasar. From the time of discovery to 1991, had the least angular separation between images, 0.45″. |
| PKS 2000-330 (QSO J2003-3251, Q2000-330) | 1982–1986 | z = 3.78 | Most distant object when discovered. |
| OQ172 (QSO B1442+101) | 1974–1982 | z = 3.53 | Most distant object when discovered. |
| OH471 (QSO B0642+449) | 1973–1974 | z = 3.408 | Most distant object when discovered; first quasar with z > 3. Nicknamed "the blaze marking the edge of the universe". |
| 4C 05.34 | 1970–1973 | z = 2.877 | Most distant object when discovered. The redshift was so much greater than the previous record that it was believed to be erroneous, or spurious. |
| 5C 02.56 (7C 105517.75+495540.95) | 1968–1970 | z = 2.399 | Most distant object when discovered. |
| 4C 25.05 (4C 25.5) | 1968 | z = 2.358 | Most distant object when discovered. |
| PKS 0237-23 (QSO B0237-2321) | 1967–1968 | z = 2.225 | Most distant object when discovered. |
| 4C 12.39 (Q1116+12, PKS 1116+12) | 1966–1967 | z = 2.1291 | Most distant object when discovered. |
| 4C 01.02 (Q0106+01, PKS 0106+1) | 1965–1966 | z = 2.0990 | Most distant object when discovered. |
| 3C 9 | 1965 | z = 2.018 | Most distant object when discovered; first quasar with z > 2. |
| 3C 147 | 1964–1965 | z = 0.545 | First quasar to become the most distant object in the universe, beating radio galaxy 3C 295. |
| 3C 48 | 1963–1964 | z = 0.367 | Second quasar redshift measured. Redshift was discovered after publication of 3C273's results prompted researchers to re-examine spectroscopic data. Not the most distant object when discovered. The radio galaxy 3C 295 was found in 1960 with z = 0.461. |
| 3C 273 | 1963 | z = 0.158 | First quasar redshift measured. Not the most distant object when discovered. The radio galaxy 3C 295 was found in 1960 with z = 0.461. |

## Most powerful quasars

10 Most luminous Quasars :
| Rank | Quasar | Data |
| 1 | SMSS J215728.21-360215.1 | It has an intrinsic bolometric luminosity of ~ 6.9 × 10$^{14}$ Suns or ~ 2.6 × 10$^{41}$ watts |
| 2 | HS 1946+7658 | It has an intrinsic bolometric luminosity in excess of 10$^{14}$ Suns or 10$^{41}$ watts |
| 3 | SDSS J155152.46+191104.0 | Has over 10$^{41}$ watts luminosity |
| 4 | HS 1700+6416 | Has a luminosity of over 10$^{41}$ watts |
| 5 | SDSS J010013.02+280225.8 | Has a luminosity of around 1.62 × 10$^{41}$ watts |
| 6 | SBS 1425+606 | Has a luminosity of over 10$^{41}$ watts – optically brightest for z>3 |
| | J1144-4308 | Has a luminosity of 4.7 x 10$^{40}$ watts or M_i(z=2) = -29.74 mag, optically brightest in last 9 Gyr |
| | SDSS J074521.78+473436.2 | |
| | S5 0014+813 | |
| | SDSS J160455.39+381201.6 | z = 2.51, M(i) = 15.84 |
| | SDSS J085543.40-001517.7 | |