Template:Short description Template:Use dmy dates This article contains lists of quasars. More than a million quasars have been observed,<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> 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 quasarsEdit
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.<ref name="Toward the Edge of the Universe">Template:Cite magazine</ref> |
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. |
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List of named quasarsEdit
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. | |
Template:Nsl | 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. |
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List of multiply imaged quasarsEdit
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<ref>Template:Cite journal</ref> | Brightest known high-redshift source of CO emission<ref>Template:Cite journal</ref> | |
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 15Template:Pprime<ref name=Inada03>Template:Cite journal</ref><ref name=Oguri04>Template:Cite journal</ref><ref name=Inada05>Template:Cite journal</ref> |
SDSS J1029+2623 | 3 | Galaxy cluster at z = 0.6 | The current largest-separation quasar lens with 22.6Template:Pprime separation between furthest images<ref name=Inada06>Template:Cite journal</ref><ref name=Oguri08>Template:Cite journal</ref><ref name=Kratzer11>Template:Cite journal</ref> |
SDSS J2222+2745 | 6<ref name=ScienceDaily-2013-08-07/> | Galaxy cluster at z = 0.49<ref name=2013ApJ...773..146D/> | First sextuply-lensed galaxy<ref name=ScienceDaily-2013-08-07>ScienceDaily, "Quasar Observed in Six Separate Light Reflections", 7 August 2013</ref> Third quasar discovered to be lensed by a galaxy cluster.<ref name=2013ApJ...773..146D/> Quasar located at z = 2.82<ref name=2013ApJ...773..146D>Template:Cite journal</ref> |
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List of visual quasar associationsEdit
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 | Notes |
---|---|---|
QSO 1548+115
|
2 | <ref>SIMBAD, Object query : QSO 1548+115</ref><ref>Template:Cite book</ref> |
QSO 1146+111 | 8 | <ref>SIMBAD, Object query : QSO 1146+111</ref> |
z represents redshift, a measure of recessional velocity and inferred distance due to cosmological expansion |
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List of physical quasar groupsEdit
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.<ref>Space Daily, "Astronomers Baffled by Discovery of Rare Quasar Quartet", 18 May 2015</ref><ref name=2015arXiv150503786H>Template:Cite journal</ref> |
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.<ref>Template:Cite magazine</ref> |
QQ2345+007 (Q2345+007)
|
2 | Originally thought to be a doubly imaged quasar, but actually a quasar couplet.<ref>Template:Cite magazine</ref> |
QQQ J1519+0627 | 3 | <ref name=SpaceDaily-2013-03-14>SpaceDaily, "Extremely rare triple quasar found", 14 March 2013 (accessed 14 March 2013)</ref> |
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Large Quasar GroupsEdit
{{#invoke:Labelled list hatnote|labelledList|Main article|Main articles|Main page|Main pages}} 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.<ref name=Webster1982>Template:Cite journal</ref><ref name="2001ASPC..232..108C">Template:Cite book</ref> |
Huge-LQG (U1.27) |
73 | The largest structure known in the observable universe, as of 2013.<ref name="10.1093/mnras/sts497"> Template:Cite journal</ref><ref name=ScienceDaily-2013-01-13>ScienceDaily, "Biggest Structure in Universe: Large Quasar Group Is 4 Billion Light Years Across", Royal Astronomical Society, 11 January 2013 (accessed 13 January 2013)</ref> |
List of quasars with apparent superluminal jet motionEdit
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<ref name=xcrs /><ref name=startVLBI100m /><ref name=AIP /><ref>New Scientist, Quasar jets and cosmic engines: Some galaxies spew out vast amounts of material into space at velocities close to that of light. Astronomers still don't know why, 16 March 1991</ref><ref>The superluminal radio source in the gamma-ray blazar 3C 279</ref> |
3C 179 | 7.6c | Fifth discovered, first with double lobes<ref>Template:Cite journal</ref> |
3C 273 | This is also the first quasar ever identified<ref name=29-05-81>Daily Intelligencer, The May 29, 1981;</ref> | |
3C 216 | ||
3C 345 | <ref name=29-05-81 /><ref>Template:Cite news</ref> | |
3C 380 | ||
4C 69.21 (Q1642+690, QSO B1642+690) |
||
4C 39.25 | <ref>Template:Cite journal</ref> | |
8C 1928+738 (Q1928+738, QSO J1927+73, Quasar J192748.6+735802) |
||
PKS 0637-752 | ||
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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.<ref name=UoM23 /> Early attempts to explain superluminal quasars resulted in convoluted explanations with a limit of z = 2.326, or in the extreme z < 2.4.<ref name=QSRPSR8 /> The majority of quasars lie between z = 2 and z = 5.
FirstsEdit
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 | ||||
First radio source discovered later found to be a quasar | ||||
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.<ref name=AIP>Template:Cite journal</ref><ref name=Quasi-Quasars>Template:Cite magazine</ref><ref>SIMBAD, Object query : BSO 1, QSO B1246+377 -- Quasar</ref> | |
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 | <ref name=Ars-2015-01-08>Template:Cite news</ref><ref name="10.1038/nature14143" > Template:Cite journal</ref> |
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 | <ref name=xcrs>Template:Cite book</ref><ref name=startVLBI100m>Template:Cite book</ref><ref name=AIP /> | |
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 | <ref>Template:Cite magazine</ref> | |
First "dustless" quasar found | QSO J0303-0019 and QSO J0005-0006 | 2010 | <ref>Discovery News, "Primordial 'Dust Free' Monsters Lurk at the Edge of the Universe", Ian O'Neill, 18 March 2010 (accessed 6 April 2010)</ref><ref>DNA India, "Astronomers discover most primitive supermassive black holes known", ANI, 19 March 2010 (accessed 6 April 2010)</ref><ref>Template:Cite news</ref><ref>Template:Cite journal</ref><ref>Scientific Computing, "Fast-growing Primitive Black Holes found in Distant Quasars " Template:Webarchive (accessed 4 April 2010)</ref><ref>SIMBAD, "QSO J0303-0019" (accessed 4 April 2010)</ref><ref>SIMBAD, "QSO J0005-0006" (accessed 4 April 2010)</ref> | |
First Large Quasar Group discovered | Webster LQG (LQG 1) |
1982 | <ref name=Webster1982/><ref name="2001ASPC..232..108C"/> |
ExtremesEdit
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<ref name=APOD-20231110/> | ||
Most distant radio-quiet quasar | |||||
Most distant radio-loud quasar | QSO J1427+3312 | z = 6.12 | Found June 2008<ref name=bbqsr>Radio astronomers detect 'baby quasar' near the edge of the visible Universe, 13:50 EST, 6 June 2008</ref><ref>SIMBAD, Object query : QSO J1427+3312, QSO J1427+3312 -- Quasar</ref> | ||
Most distant blazar quasar | PSO J0309+27 | z > 6 | |||
Least distant | Markarian 231 | 600 Mly | citation | CitationClass=web
}}</ref> inactive: IC 2497 | |
Largest Large Quasar Group | Huge-LQG (U1.27) | 73 quasars | <ref name="10.1093/mnras/sts497"/><ref name=ScienceDaily-2013-01-13/> | ||
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) |
citation | CitationClass=web
}}</ref><ref>{{#invoke:citation/CS1|citation |
CitationClass=web
}}</ref> |
First quasars foundEdit
Rank | Quasar | Date of discovery | Notes | |
---|---|---|---|---|
1 | 3C 273 | 1963 | <ref name=Maaarten /> | |
2 | 3C 48 | 1963 | <ref name=Maaarten /> | |
3 | 3C 47 | 1964 | <ref name=Maaarten /> | |
3 | 3C 147 | 1964 | <ref name=Maaarten /> | |
5 | CTA 102 | 1965 | <ref name=Shields1999>Template:Cite journal; {{#invoke:citation/CS1|citation | CitationClass=web
}}</ref> |
5 | 3C 287 | 1965 | <ref name=Shields1999 /> | |
5 | 3C 254 | 1965 | <ref name=Shields1999 /> | |
5 | 3C 245 | 1965 | <ref name=Shields1999 /> | |
5 | 3C 9 | 1965 | <ref name=Shields1999 /> | |
These are the first quasars which were found and had their redshifts determined. |
Most distant quasarsEdit
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).<ref name=Illingworth>Template:Cite journal; {{#invoke:citation/CS1|citation |CitationClass=web }}</ref>
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.
Quasar | Distance | Notes | |
---|---|---|---|
UHZ1 | z = 10.1 | Most distant quasar known Template:As of<ref name=APOD-20231110/><ref name="2023arXiv231213837I"/> | |
QSO J0313–1806 | z = 7.64 | Former most distant quasar.<ref name=Temming2021>Template:Citation</ref><ref name="2023arXiv231213837I"/> | |
ULAS J1342+0928 | z = 7.54 | Former most distant quasar. <ref name="2019ApJ...881L..23B"> Template:Cite journal </ref><ref name="2023arXiv231213837I"/> | |
Pōniuāʻena (Q J1007+2115) | z = 7.52 | <ref name="2020ApJ...897L..14Y"> Template:Cite journal </ref><ref name="2023arXiv231213837I"> Template:Citation </ref> | |
ULAS J1120+0641 (ULAS J112001.48+064124.3) |
z = 7.085 | Former most distant quasar. First quasar with z > 7.<ref name=SciAm-2011-06-29/> | |
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.<ref name=7-6-7 /><ref name=CFHQS4z6 /><ref name=mid2008 /><ref name=Q2007 /> | |
SDSS J114816.64+525150.3 (SDSS J1148+5251) |
z = 6.419 | Former most distant quasar.<ref name="z = 6.42">Template:Cite journal</ref><ref name=350u /><ref name=OoSmBH>Template:Cite arXiv</ref><ref name=Q2007 /><ref name="REIONz.gt.6">Template:Cite journal</ref><ref name=z~6 /> | |
SDSS J1030+0524 (SDSSp J103027.10+052455.0) |
z = 6.28 | Former most distant quasar. First quasar with z > 6.<ref name="VLT z = 6.28" /><ref name="REIONz.gt.6" /><ref name="SDSS1030+0524" /><ref name="Xray z = 6.30" /><ref name="z.gt.5.8" /><ref name=PSU2001 /><ref name=SDSS2001 /> | |
SDSS J104845.05+463718.3 (QSO J1048+4637) |
z = 6.23 | <ref name=z~6 /> | |
SDSS J162331.81+311200.5 (QSO J1623+3112) |
z = 6.22 | <ref name=z~6>Template:Cite journal</ref> | |
CFHQS J0033-0125 (CFHQS J003311-012524) |
z = 6.13 | <ref name=CFHQS4z6 /> | |
SDSS J125051.93+313021.9 (QSO J1250+3130) |
z = 6.13 | <ref name=z~6 /> | |
CFHQS J1509-1749 (CFHQS J150941-174926) |
z = 6.12 | <ref name=CFHQS4z6 /> | |
QSO B1425+3326 / QSO J1427+3312 | z = 6.12 | Most distant radio-quasar.<ref name=bbqsr /><ref>SIMBAD, Object query : QSO B1425+3326 Template:Webarchive, QSO J1427+3312 -- Quasar</ref> | |
SDSS J160253.98+422824.9 (QSO J1602+4228) |
z = 6.07 | <ref name=z~6 /> | |
SDSS J163033.90+401209.6 (QSO J1630+4012) |
z = 6.05 | <ref name=z~6 /> | |
CFHQS J1641+3755 (CFHQS J164121+375520) |
z = 6.04 | <ref name=CFHQS4z6 /> | |
SDSS J113717.73+354956.9 (QSO J1137+3549) |
z = 6.01 | <ref name=z~6 /> | |
SDSS J081827.40+172251.8 (QSO J0818+1722) |
z = 6.00 | <ref name=z~6 /> | |
SDSSp J130608.26+035626.3 (QSO J1306+0356) |
z = 5.99 | <ref name="z.gt.5.8">Template:Cite journal</ref><ref name=PSU2001 /><ref name=SDSS2001 /> | |
|
Type | Quasar | Date | Distance | Notes |
---|---|---|---|---|
Most distant | UHZ1 | 2023 | z = 10.2 | <ref name="2312.13837"/> |
Most distant radio loud quasar | QSO B1425+3326 / QSO J1427+3312 | 2008 | z = 6.12 | |
Most distant radio quiet quasar | ||||
Most distant OVV quasar |
Quasar | Date | Distance | Notes | |
---|---|---|---|---|
UHZ1 | 2023– | z = 10.2 | Current distance record holder <ref name="2312.13837"> Template:Citation </ref><ref name=APOD-20231110> {{#invoke:citation/CS1|citation | CitationClass=web
}} </ref> |
QSO J0313−1806 | 2021–2023 | z = 7.64 | <ref name=Temming2021/><ref name="2312.13837"/> | |
ULAS J1342+0928 | 2017–2021 | z = 7.54 | <ref name="NAT-20171206">Template:Cite journal</ref> | |
ULAS J1120+0641 | 2011–2017 | z = 7.085 | Not the most distant object when discovered. First quasar with z > 7.<ref name=SciAm-2011-06-29>Scientific American, "Brilliant, but Distant: Most Far-Flung Known Quasar Offers Glimpse into Early Universe", John Matson, 29 June 2011</ref> | |
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.<ref name=7-6-7>Discovery.com Black Hole Is Most Distant Ever Found Template:Webarchive 7 June 2007</ref><ref name=CFHQS4z6>Template:Cite journal</ref><ref name=mid2008>CFHQS UOttawa, Canada-France High-z Quasar Survey Template:Webarchive</ref><ref name=Q2007>CFH UHawaii, Astronomers find most distant black hole</ref><ref name=10Feb2005/><ref>Template:Cite journal</ref><ref>BBC News, Astronomers claim galaxy record, 11 July 2007, 17:10 GMT 18:10 UK</ref> | |
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.<ref name="z = 6.42" /><ref name="350u">Template:Cite journal</ref><ref name=OoSmBH /><ref name=Q2007 /><ref name=10Feb2005/><ref>New Scientist, New record for Universe's most distant object, 17:19 14 March 2002</ref><ref>BBC News, Far away stars light early cosmos, 14 March 2002, 11:38 GMT</ref><ref>BBC News, Most distant galaxy detected, 25 March 2003, 14:28 GMT</ref><ref>Template:Cite journal</ref><ref>Template:Cite journal</ref> | |
SDSS J1030+0524 (SDSSp J103027.10+052455.0) |
2001–2003 | z = 6.28 | Most distant object when discovered. First object with z > 6.<ref name="VLT z = 6.28">Template:Cite journal</ref><ref name="REIONz.gt.6" /><ref name="SDSS1030+0524">Template:Cite journal</ref><ref name="Xray z = 6.30">Template:Cite journal</ref><ref name=PSU2001 /><ref name=SDSS2001 /> | |
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.<ref name=Summer2000>Template:Cite magazine</ref><ref name="z = 5.74">Template:Cite journal</ref><ref name=PSU2001>Template:Cite news</ref><ref name=SDSS2001>SDSS, Early results from the Sloan Digital Sky Survey: From under our nose to the edge of the universe, June 2001</ref><ref name=10Feb2005 /><ref>PennState Eberly College of Science, X-rays from the Most Distant Quasar Captured with the XMM-Newton Satellite Template:Webarchive, Dec 2000</ref><ref>SPACE.com, Most Distant Object in Universe Comes Closer, 1 December 2000</ref> | |
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).<ref>NOAO Newsletter - NOAO Highlights - March 2000 - Number 61, The Most Distant Quasar Known</ref><ref>Template:Cite journal</ref><ref name="z = 5.74" /><ref name="x=5.501">Template:Cite journal</ref><ref name=10Feb2005 /> | |
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).<ref name="x=5.501" /><ref name=10Feb2005>UW-Madison Astronomy, Confirmed High Redshift (z > 5.5) Galaxies - (Last Updated 10 February 2005) Template:Webarchive</ref> | |
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).<ref name=10Feb2005 /><ref name=Summer2000 /><ref>SDSS 98-3 Scientists of Sloan Digital Sky Survey Discover Most Distant Quasar Dec 1998</ref><ref>Template:Cite journal</ref><ref>SIMBAD, Object query : SDSSp J033829.31+002156.3, QSO J0338+0021 -- Quasar</ref><ref>Template:Cite news</ref><ref>Template:Cite news</ref> | |
PC 1247+3406 | 1991–1998 | z = 4.897 | Most distant object when discovered.<ref name=Summer2000 /><ref>Template:Cite journal</ref><ref>New Scientist, issue 1842, 10 October 1992, page 17, Science: Infant galaxy's light show</ref><ref>FermiLab Scientists of Sloan Digital Sky Survey Discover Most Distant Quasar Template:Webarchive 8 December 1998</ref><ref name=472QSR401>Template:Cite journal</ref> | |
PC 1158+4635 | 1989–1991 | z = 4.73 | Most distant object when discovered.<ref name=Summer2000 /><ref name=472QSR401 /><ref name="z.gt.4">Template:Cite journal</ref><ref>SIMBAD, Object query : PC 1158+4635, QSO B1158+4635 -- Quasar</ref><ref>Template:Cite journal</ref><ref name=20NOV1989>The New York Times, Peering to Edge of Time, Scientists Are Astonished, 20 November 1989</ref> | |
Q0051-279 | 1987–1989 | z = 4.43 | Most distant object when discovered.<ref name="z = 4.43">Template:Cite journal</ref><ref name="z.gt.4" /><ref name=20NOV1989 /><ref>Template:Cite journal</ref><ref>The New York Times, Objects Detected in Universe May Be the Most Distant Ever Sighted, 14 January 1988</ref><ref>Template:Cite news</ref> | |
Q0000-26 (QSO B0000-26) |
1987 | z = 4.11 | Most distant object when discovered.<ref name="z = 4.43" /><ref name="z.gt.4" /><ref>SIMBAD, Object query : Q0000-26, QSO B0000-26 -- Quasar</ref> | |
PC 0910+5625 (QSO B0910+5625) |
1987 | z = 4.04 | Most distant object when discovered; second quasar with z > 4.<ref name=Summer2000 /><ref name="z.gt.4" /><ref name="PC0910+5625">Template:Cite journal</ref><ref>SIMBAD, Object query : PC 0910+5625, QSO B0910+5625 -- Quasar</ref> | |
Q0046–293 (QSO J0048-2903) |
1987 | z = 4.01 | Most distant object when discovered; first quasar with z > 4.<ref name="z = 4.43" /><ref name="z.gt.4" /><ref name="PC0910+5625" /><ref>Template:Cite journal; First observation of a quasar with a redshift of 4</ref><ref>SIMBAD, Object query : Q0046-293, QSO J0048-2903 -- Quasar</ref> | |
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, 0.45Template:Pprime.<ref name="PC0910+5625" /><ref>SIMBAD, Object query : Q1208+1011, QSO B1208+1011 -- Quasar</ref><ref>NewScientist, Quasar doubles help to fix the Hubble constant, 16 November 1991</ref> | |
PKS 2000-330 (QSO J2003-3251, Q2000-330) |
1982–1986 | z = 3.78 | Most distant object when discovered.<ref name=UoM23 /><ref name="PC0910+5625" /><ref>Orwell Astronomical Society (Ipswich) - OASI; Archived Astronomy News Items, 1972 - 1997 Template:Webarchive</ref><ref>SIMBAD, Object query : PKS 2000-330, QSO J2003-3251 -- Quasar</ref> | |
OQ172 (QSO B1442+101) |
1974–1982 | z = 3.53 | Most distant object when discovered.<ref name=BigEarHist /><ref>SIMBAD, Object query : OQ172, QSO B1442+101 -- Quasar</ref><ref name=Q3Y /> | |
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".<ref name=BigEarHist>OSU Big Ear, History of the OSU Radio Observatory</ref><ref name=Q3Y /><ref>Template:Cite magazine</ref><ref>SIMBAD, Object query : OH471, QSO B0642+449 -- Quasar</ref><ref>Template:Cite journal</ref> | |
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.<ref name=UoM23 /><ref name=QSRPSR8>Quasars and Pulsars, Dewey Bernard Larson, (c) 1971; CHAPTER VIII - Quasars: The General Picture Template:Webarchive; LOC 75-158894</ref><ref name=Q3Y>QUASARS - THREE YEARS LATER, 1974 Template:Webarchive</ref><ref>Template:Cite journal</ref><ref name=4C05.34/> | |
5C 02.56 (7C 105517.75+495540.95) |
1968–1970 | z = 2.399 | Most distant object when discovered.<ref name=4C05.34>Template:Cite journal</ref><ref>SIMBAD, Object query : 5C 02.56, 7C 105517.75+495540.95 -- Quasar</ref><ref name=Illingworth /> | |
4C 25.05 (4C 25.5) |
1968 | z = 2.358 | Most distant object when discovered.<ref name=4C05.34 /><ref name=Illingworth /><ref name=zQSOg>Template:Cite journal</ref> | |
PKS 0237-23 (QSO B0237-2321) |
1967–1968 | z = 2.225 | Most distant object when discovered.<ref name=UoM23 /><ref name=zQSOg /><ref>Time Magazine, A Farther-Out Quasar, 7 April 1967</ref><ref>SIMBAD, Object query : QSO B0237-2321, QSO B0237-2321 -- Quasar</ref><ref name=lambdaQSO>Template:Cite journal</ref> | |
4C 12.39 (Q1116+12, PKS 1116+12) |
1966–1967 | z = 2.1291 | Most distant object when discovered.<ref name=Illingworth /><ref name=lambdaQSO /><ref name=ManOnMnt /><ref>SIMBAD, Object query : Q1116+12, 4C 12.39 -- Quasar</ref> | |
4C 01.02 (Q0106+01, PKS 0106+1) |
1965–1966 | z = 2.0990 | Most distant object when discovered.<ref name=Illingworth /><ref name=lambdaQSO /><ref name=ManOnMnt>Time Magazine, The Man on the Mountain, Friday, Mar. 11, 1966</ref><ref>SIMBAD, Object query : Q0106+01, 4C 01.02 -- Quasar</ref> | |
3C 9 | 1965 | z = 2.018 | Most distant object when discovered; first quasar with z > 2.<ref name="Toward the Edge of the Universe"/><ref name=Quasi-Quasars /><ref name=lambdaQSO /><ref>Template:Cite book</ref><ref>Template:Cite journal</ref><ref>Template:Cite book</ref> | |
3C 147 | 1964–1965 | z = 0.545 | First quasar to become the most distant object in the universe, beating radio galaxy 3C 295.<ref name=3C47>Template:Cite journal</ref><ref>Template:Cite book</ref><ref>Template:Cite journal</ref><ref>Template:Cite news</ref> | |
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.<ref name=AIP /><ref name=UoM23>The Structure of the Physical Universe, Volume III - The Universe of Motion, CHAPTER 23 - Quasar Redshifts Template:Webarchive, by Dewey Bernard Larson, Library of Congress Catalog Card No. 79-88078, Template:ISBN, Copyright 1959, 1971, 1984</ref><ref>Template:Cite journal</ref><ref name=1961May12 /><ref name=z3C295 /><ref name=Maaarten>Interview; {{#invoke:citation/CS1|citation | CitationClass=web
}} Template:Small; 11 April and 2 & 15 May 1996</ref><ref name=3C47 /> |
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.<ref name=AIP /><ref name=Maaarten /><ref name=1961May12>Template:Cite journal</ref><ref name=z3C295>Template:Cite journal</ref><ref>The Origin of Matter Part 4</ref> |
Most powerful quasarsEdit
Rank | Quasar | Data | Refs. |
---|---|---|---|
1 | SMSS J215728.21-360215.1 | Intrinsic bolometric luminosity of ~ 6.9 × 1014 Suns or ~ 2.6 × 1041 watts | <ref>Template:Cite journal</ref> |
2 | HS 1946+7658 | Intrinsic bolometric luminosity in excess of 1014 Suns or 1041 watts | <ref>Template:Cite journal</ref><ref>Template:Cite journal</ref> |
3 | SDSS J155152.46+191104.0 | Luminosity of over 1041 watts | <ref>Template:Cite journal</ref><ref>Template:Cite journal</ref> |
4 | HS 1700+6416 | Luminosity of over 1041 watts | <ref name="arXiv.org">Template:Cite journal</ref> |
5 | SDSS J010013.02+280225.8 | Luminosity of around 1.62 × 1041 watts | <ref>Template:Cite journal</ref> |
6 | SBS 1425+606 | Luminosity of over 1041 watts – optically brightest for z>3 | <ref>Template:Cite journal</ref> |
J1144-4308 | Luminosity of 4.7 × 1040 watts or M_i(z=2) = −29.74 mag, optically brightest in last 9 Gyr | <ref>Template:Cite journal</ref> | |
SDSS J074521.78+473436.2 | <ref>Template:Cite journal</ref><ref>Template:Cite journal</ref> | ||
S5 0014+813 | <ref name="arXiv.org"/><ref>Template:Cite journal</ref> | ||
SDSS J160455.39+381201.6 | z = 2.51, M(i) = 15.84 | ||
SDSS J085543.40-001517.7 | <ref>Template:Cite journal</ref> |