This is a list of quasars. 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.
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 gravitationally lensed quasar is produced.
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.
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
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-separatioon 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.
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
8C 1928+738
PKS 0637-752
QSO B1642+690
Quasars that have a recessional velocitygreater thanthe speed of light are very common. Any quasar with z>1 is going away from us in excess of c. Early attempts to explain superlumic quasars resulted in convoluted explanations with a limit of z = 2.326, or in the extreme z<2.4. z = 1 means a redshift indicating travel away from us at the speed of light. The majority of quasars lie between z = 2 and z = 5.
Firsts
Extremes
First quasars found
Most distant quasars
The first time that quasars became the most distant object in the universe was in 1964. Quasars would remain the most distant objects in the universe until 1997, when a pair of non-quasar galaxies would take the title.
Most powerful quasars
Rank
Quasar
Data
Notes
1
SMSS J215728.21-360215.1
It has an intrinsic bolometric luminosity of ~ 6.9 × 1014 Suns or ~ 2.6 × 1041 watts
2
HS 1946+7658
It has an intrinsic bolometric luminosity in excess of 1014 Suns or 1041 watts
3
SDSS J155152.46+191104.0
Has over 1041 watts luminosity
4
HS 1700+6416
Has a luminosity of over 1041 watts
5
SDSS J010013.02+280225.8
Has a luminosity of around 1.62 × 1041 watts
6
SBS 1425+606
Has a luminosity of over 1041 watts – optically brightest for z>3