Wikipédia banwiki https://ban.wikipedia.org/wiki/Kaca_Utama MediaWiki 1.47.0-wmf.23 first-letter Média Kusus Pabligbagan Sang Anganggé Pabligbagan Sang Anganggé Wikipédia Pabligbagan Wikipédia Berkas Pabligbagan Berkas MédiaWiki Pabligbagan MédiaWiki Mal Pabligbagan Mal Wantuan Pabligbagan Wantuan Kategori Pabligbagan Kategori TimedText TimedText talk Modul Pabligbagan Modul Acara Pembicaraan Acara 0 41636 283471 283227 2026-10-14T02:03:56Z Cakraadi12 115725 283471 wikitext text/x-wiki '''I Gusti Ngurah Kesuma Kelakan''' , S.T., M.Si inggih punika silih tunggil politikus Indonésia sané mawit saking Bali. Dané embas ring Dénpasar, 4 April 1967. Dané makarya dados Anggota DPR-RI periode 2019–2024, 2024-2029. Sadurungnyané, dané makarya dados Anggota DPRD provinsi Bali 1999–2003, Wakil Gubernur Bali periode 2003–2008 nampingin Déwa Madé Beratha tur dados Anggota DPD-RI ring periode 2009–2014. [[File:Anggota Badan Pengkajian Majelis Permusyawaratan Rakyat Republik Indonesia I Gusti Ngurah Kesuma Kelakan.jpg|jmpl]] == Pendidikan == * SD , SD No. 20 Denpasar. Tahun: - 1980 * SMP , SMP Negeri 2 Denpasar. Tahun: - 1983 * SMA , SMA Negeri 1 Denpasar. Tahun: - 1986 * S1 , Univ. Udayana Fakultas Teknik Electro. Tahun: - 1997 * S2 , Univ. Udayana Kajian Budaya. Tahun: - 2005 == Pakaryan == * DPR RI, Sebagai: Anggota. Tahun: 2019 - 2024, 2024 - 2029 * DPD RI, Sebagai: Anggota. Tahun: 2009 - 2014 * Wakil Gubernur Bali Prov. Bali, Sebagai: Wakil Gubernur Bali. Tahun: 2003 - 2008 * DPRD Provinsi Bali, Sebagai: Ketua Komisi A. Tahun: 1999 - 2003 == Penghargaan == * Konferensi Memperkuat Partai Politik, Dari: Council of Asian Leberalis And Democrats (Cald), Alliance For Reform And Democracy In Asia (Arda), National Democratic Instituite For Internasional Affairs (Ndi), Tahun: 2002 * Sosialisasi Peraturan Otonomi Daerah Mendukung Dunia Usaha Bali, Dari: Yayasan Sanggar Seni Bidaya Bali, Tahun: 2001 * Seminar Reposisi Lembaga Pengawasan Daerah, Dari: Gubernur Bali, Tahun: 2000<ref>{{Cite web|url=https://www.cnbcindonesia.com/news/20191030063226-4-111185/catat-ini-daftar-anggota-dpr-ri-di-komisi-i-hingga-komisi-xi|title=Catat! Ini Daftar Anggota DPR RI di Komisi I Hingga Komisi XI|last=Putri|first=Cantika Adinda|website=CNBC Indonesia|language=id-ID|access-date=2023-08-08}}</ref> <references /> i9lp8ak2ecxheycdnpsr72trivw5ylq 0 82541 283470 283217 2026-10-13T17:17:26Z InternetArchiveBot 2766 Add 1 book for [[en:Wikipedia:Verifiability|verifiability]] (20261013sim)) #IABot (v2.0.9.6) ([[User:GreenC bot|GreenC bot]] 283470 wikitext text/x-wiki [[Berkas:BlackHole.jpg|jmpl|Kesan seniman indik [[lubang hitam supermasif]] bahan sane ngelekang saking [[piringan akresi]]]] Ring sor puniki lis '''lubang hitam''' sane pinih masif sane kapanggihin kantos mangkin (lan kandidatnyane), sane kaukur antuk satuan [[massa matahari]]. ({{Solar mass|link=yes}}), kirang langkung {{val|2|u=kilogram|ul=|e=30}}. == Lis == {{expand list|date=Juni 2017}} {| class="wikitable sortable" |+ Lis blungbang selem pinih ageng ! Aran ! [[Massa matahari]]<br />([[Matahari]] = 1) ! Cutetan |- |[[SDSS J123703.24+275819.5]] || '''{{val|2.202|e=11}}'''<ref name="Oei">{{Cite journal |last=Oei |first=Martijn S. S. L. |last2=Weeren |first2=Reinout J. van |last3=Gast |first3=Aivin R. D. J. G. I. B. |last4=Botteon |first4=Andrea |last5=Hardcastle |first5=Martin J. |last6=Dabhade |first6=Pratik |last7=Shimwell |first7=Tim W. |last8=Röttgering |first8=Huub J. A. |last9=Drabent |first9=Alexander |date=2023-04-01 |title=Measuring the giant radio galaxy length distribution with the LoTSS |url=https://www.aanda.org/articles/aa/full_html/2023/04/aa43572-22/aa43572-22.html |journal=Astronomy & Astrophysics |language=en |volume=672 |pages=A163 |doi=10.1051/0004-6361/202243572 |issn=0004-6361}}</ref> ||Lubang hitam sane pinih ageng sane naenin kapanggihin. Minab alitan mawinan nenten akurasi pangukuran. |- |[[SDSS J152156.48+520238.5]] |'''{{val|1.99|e=11}}'''<ref name=Rakshit2020 /> |Objek puniki madué akéh sané nénten pastika miwah minab ukurannyané alitan. |- | [[SDSS J140821.67+025733.2]] || '''{{Val|1.96|e=11}}'''<ref name=Kozlowski2017>{{Cite journal|title=Virial Black Hole Mass Estimates for 280,000 AGNs from the SDSS Broad-Band Photometry and Single Epoch Spectra|first=Szymon|last=Kozłowski|date=January 20, 2017|journal=[[The Astrophysical Journal Supplement Series]]|volume=228|issue=1|pages=9|doi=10.3847/1538-4365/228/1/9|arxiv=1609.09489|bibcode=2017ApJS..228....9K|s2cid=118422643}}</ref> ||Wenten malih 17 objek ring katalog quasar sane pateh antuk massa lubang hitam sane kakenehang lintangan saking 100 miliar. {{Solar mass}}. |- | [[SDSS J123132.37+013814.1]] || '''{{val|1.12|0.28|0.23|e=11}}'''<ref name=Rakshit2020>{{cite journal | url=https://ui.adsabs.harvard.edu/abs/2020ApJS..249...17R/abstract | bibcode=2020ApJS..249...17R | title=Spectral Properties of Quasars from Sloan Digital Sky Survey Data Release 14: The Catalog | last1=Rakshit | first1=Suvendu | last2=Stalin | first2=C. S. | last3=Kotilainen | first3=Jari | journal=The Astrophysical Journal Supplement Series | date=2020 | volume=249 | issue=1 | page=17 | doi=10.3847/1538-4365/ab99c5 | doi-access=free | arxiv=1910.10395 }}</ref><ref name=Rakshit_tabular1>{{cite web | url=https://vizier.cds.unistra.fr/viz-bin/VizieR-5?-ref=VIZ672025b136fc47&-out.add=.&-source=J/ApJS/249/17/dr14qpsp&recno=374296 | title=VizieR }}</ref> ||Santukan lubang hitam puniki masif pisan, ukurannyane minab alitan santukan jarak lan pangukuran. |- | [[SDSS J073739.96+384413.2]] || '''{{Val|1.04|e=11}}'''<ref name=Kozlowski2017 /> ||Gatra indik quasar puniki pinih kidik. |- | [[Gugus Phoenix#Lubang hitam supermasif|Phoenix A]] || '''{{val|1|e=11}}'''<ref name="Brockamp2016">{{cite journal |title=Unveiling Gargantua: A new search strategy for the most massive central cluster black holes |journal=Astronomy & Astrophysics |last1=Brockamp |first1=M. |last2=Baumgardt |first2=H. |last3=Britzen |first3=S. |last4=Zensus |first4=A. |volume=585 |at=A153 |date=January 2016 |doi=10.1051/0004-6361/201526873 |doi-access=free|bibcode=2016A&A...585A.153B |arxiv=1509.04782|s2cid=54641547 }}</ref> ||Kaperkiraang ngawigunayang model kalorimetri parilaksana adiabatik saking pertumbuhan malih inti miwah model inti-Sérsic sané kaasumsiang antuk n=4. Puniki manut sareng pemodelan evolusioner akresi gas miwah dinamika miwah profil kepadatan galaksi.<ref name="Brockamp2016" /> Lubang hitam ultramasif sane massanyane 100 miliar massa matahari. Massa punika durung langsung kaukur. |- | [[SDSS J140737.17+442856.2]] || '''{{Val|1|e=11}}'''<ref name=Ellison>{{Cite journal|title=Discovery of a dual active galactic nucleus with ~ 8 kpc separation|last1=Ellison|first1=Sara L.|last2=Secrest|first2=Nathan J.|last3=Mendel|first3=J. Trevor|last4=Satyapal|first4=Shobita|last5=Simard|first5=Luc|date=September 2017|journal=Monthly Notices of the Royal Astronomical Society|volume=470|issue=1|pages=L49–L53|doi=10.1093/mnrasl/slx076|arxiv=1705.05465|bibcode=2017MNRAS.470L..49E}}</ref> ||Objek puniki madue massa sane nenten pastika. |- | [[IC 1101]] || '''{{val|9.94|e=10}}'''<ref name="dullo2019" /><ref name="dullo2021a" /> ||Kaperkiraang saking jeriji-jeriji fraktur inti pusat; Model sadurungnyane nyihnayang indik objek puniki madue massa wantah 46 miliar M⊙.<ref>{{cite journal|last1=Dullo|first1=Bililign T.|last2=Graham|first2=Alister W.|last3=Knapen|first3=Johan H.|title=A remarkably large depleted core in the Abell 2029 BCG IC 1101|journal=Monthly Notices of the Royal Astronomical Society|date=October 2017|volume=471|issue=2|pages=2321–2333|doi=10.1093/mnras/stx1635|arxiv=1707.02277|bibcode=2017MNRAS.471.2321D|s2cid=119000593}}</ref> Massanyané sané pinih minab inggih punika 99,4 miliar M⊙. |- |[[NGC 3842]] || '''{{val|9.76|e=10}}'''<ref name=dullo2019/><ref name=dullo2021a/> || Galaksi sané pinih galang ring [[Gugus Leo]]; kakenehang nganggen jeriji-jeriji fraktur. Sadurungnyane kakenehang ngamolihang pikolih sane pinih kidik 9,7 miliar M⊙.<ref name="McConnell" /><ref name="mcconnell2012" /> Ukuran maksimum sane kakenehang prasida alitan, inggih punika 12,2 miliar M⊙. |- |[[ESO 444-46]] || '''{{val|7.76|e=10}}'''<ref name=dullo2019>{{cite journal|last=Dullo|first=B.T.|title=The Most Massive Galaxies with Large Depleted Cores: Structural Parameter Relations and Black Hole Masses|journal=The Astrophysical Journal|date=22 November 2019|volume=886|issue=2|page=80|arxiv=1910.10240|bibcode=2019ApJ...886...80D|doi=10.3847/1538-4357/ab4d4f|s2cid=204838306 |doi-access=free }}</ref><ref name=dullo2021a>{{cite journal|last1=Dullo|first1=B.T.|last2=de Paz|first2=A.G.|last3=Knapen|first3=J.H.|title=Ultramassive black holes in the most massive galaxies: M_BH−σ versus M_BH−R_b|journal=The Astrophysical Journal|date=18 February 2021|volume=908|issue=2|page=134|arxiv=2012.04471|bibcode=2021ApJ...908..134D|doi=10.3847/1538-4357/abceae|s2cid=227745078 |doi-access=free }}</ref> || Galaksi sane pinih galang ring gugus Abell 3558 magenah ring tengahing [[Supergugus Shapley]]; kakenehang nganggen jeriji-jeriji fraktur galaksi induk. Ukuran maksimum sane kakenehang prasida alitan, ring 501 yuta M⊙. |- | [[ESO 383-76]] || '''{{val|7.41|e=10}}'''<ref name="dullo2019" /><ref name="dullo2021a" /> ||Kaperkiraang ngawigunayang jeriji-jeriji fraktur inti pusat galaksi. Ukuran maksimum sane kakenehang prasida alitan, ring 10,2 miliar M⊙. |- | [[UGC 10143]] || '''{{val|7.24|e=10}}'''<ref name="dullo2019" /><ref name="dullo2021a" /> ||Galaksi sané pinih galang ring gugus Abell 2147; kakenehang nganggen jeriji-jeriji fraktur inti. Kirang langkung ukuran maksimum prasida alitan ring 9,5 miliar M⊙. |- | [[SDSS J150848.79+605551.9]] || '''{{val|6.8|0.42|0.46|e=10}}'''<ref name=Rakshit2020 /><ref name=Rakshit_tabular2>https://vizier.cds.unistra.fr/viz-bin/VizieR-5?-ref=VIZ6754269ef2e75&-out.add=.&-source=J/ApJS/249/17/dr14qpsp&recno=409784</ref> ||Akidik pisan sane kauningin indik objek puniki. |- | [[TON 618]] || '''{{val|6.6|e=10}}'''<ref>{{cite journal|last1=Shemmer|first1=O.|last2=Netzer|first2=H.|last3=Maiolino|first3=R.|last4=Oliva|first4=E.|last5=Croom|first5=S.|last6=Corbett|first6=E.|last7=di Fabrizio|first7=L.|title=Near-infrared spectroscopy of high-redshift active galactic nuclei. I. A metallicity-accretion rate relationship|url=https://archive.org/details/sim_astrophysical-journal_2004-10-20_614_2/page/546|journal=The Astrophysical Journal|date=2004|volume=614|issue=2|pages=547–557|arxiv=astro-ph/0406559|bibcode=2004ApJ...614..547S|doi=10.1086/423607|s2cid=119010341}}</ref> ||Perkiraan dari korelasi garis emisi kuasar Hβ. |- |[[A2261-BCG|Abell 2261 BCG]] || '''{{Val|6.47|e=10}}'''<ref name="dullo2019" /><ref name="dullo2021a" /> ||Galaksi paling terang dalam gugus [[Abell 2261]]; diperkirakan menggunakan radius patahan yang sangat besar. Perkiraan ukuran maksimum, bisa lebih kecil yaitu 5.37 miliar M_⊙. |- |[[MS 0735.6+7421|4C +74.13]] || '''{{val|6.09|e=10}}'''<ref name=dullo2019/><ref name=dullo2021a/> || Menghasilkan letupan AGN kolosal setelah mengakumulasi materi senilai 600 juta M_⊙. Diperkirakan menggunakan radius patahan inti galaksi pusat sebesar 0,5 kpc.<ref name=dullo2019/><ref name=dullo2021a/> Asumsi tidak langsung sebelumnya tentang efisiensi akresi gas dan daya pancaran menghasilkan batas bawah 1 miliar M_⊙.<ref name="DS">[https://www.sciencedaily.com/releases/2005/01/050106091317.htm Most Powerful Eruption In The Universe Discovered] NASA/Marshall Space Flight Center (ScienceDaily) January 6, 2005</ref><ref name="mcnamara2005">{{cite journal | last1 = McNamara | first1 = B. R. | last2 = Nulsen | first2 = P. E. J. | last3 = Wise | first3 = M. W. | last4 = Rafferty | first4 = D. A. | last5 = Carilli | first5 = C. | last6 = Sarazin | first6 = C. L. | last7 = Blanton | first7 = E. L. | author7-link = Elizabeth Blanton | title = The heating of gas in a galaxy cluster by X-ray cavities and large-scale shock fronts | url = https://archive.org/details/sim_nature-uk_2005-01-06_433_7021/page/45 | year = 2005 | journal = [[Nature (journal)|Nature]] | volume = 433 | issue = 7021 | pages = 45–47 | doi = 10.1038/nature03202 | pmid = 15635404 | bibcode = 2005Natur.433...45M | s2cid = 4340763 }}</ref><ref name="rafferty2006">{{cite journal | last1 = Rafferty | first1 = D. A. | last2 = McNamara | first2 = B. R. | last3 = Nulsen | first3 = P. E. J. | last4 = Wise | first4 = M. W. | title = The Feedback-regulated Growth of Black Holes and Bulges through Gas Accretion and Starbursts in Cluster Central Dominant Galaxies | url = https://archive.org/details/sim_astrophysical-journal_2006-11-20_652_1/page/216 | year = 2006 | journal = [[The Astrophysical Journal]] | volume = 652 | issue = 1 | pages = 216–231 | doi = 10.1086/507672 | arxiv = astro-ph/0605323 | bibcode = 2006ApJ...652..216R | s2cid = 9481371 }}</ref> Menurut video dari Omega Comparisons, lubang hitam ini memiliki massa sekitar 60,9 miliar M_⊙. |- |[[Abell 402 BCG]] |'''{{Val|6|2|e=10}}'''<ref name="McDonald">{{Cite journal |last1=McDonald |first1=Michael |last2=Khullar |first2=Gourav |last3=Lagattuta |first3=David |last4=Mahler |first4=Guillaume |last5=Dattathri |first5=Shashank |last6=Diego |first6=Jose M. |last7=Edge |first7=Alastair C. |last8=Floyd |first8=Benjamin |last9=Gladders |first9=Michael D. |last10=Hughes |first10=Scott A. |last11=Jauzac |first11=Mathilde |last12=Khonji |first12=Nader |last13=Leroy |first13=Gavin |last14=Massey |first14=Richard |last15=Montes |first15=Mireia |date=2026-04-23 |title=A Kiloparsec-scale Stellar Cavity in the Center of A402-BCG May Be Caused by Dynamic Interactions with an Ultramassive Black Hole |journal=The Astrophysical Journal Letters |volume=1002 |issue=1 |pages=L19 |doi=10.3847/2041-8213/ae5bbe |doi-access=free |bibcode=2026ApJ..1002L..19M |issn=2041-8205|hdl=10261/432651 |hdl-access=free }}</ref> |Ini juga merupakan lubang hitam biner yang baru ditemukan.<ref>{{Cite web |last=Johnson-Groh |first=Mara |date=2026-05-11 |title=Astronomers may have found a record-breaking pair of black holes |url=https://www.sciencenews.org/article/largest-pair-black-holes-collision |access-date=2026-05-27 |website=ScienceNews |language=en-US}}</ref> |- |[[NeVe 1|LDC 1241 J1712-2322]] || '''{{Val|5.1|-|6.1|e=10}}'''<ref>{{Article|First name 1=Christopher|Last name 1=Marsden|First name 2=Francesco|Last name 2=Shankar|First name 3=Mitchele|Last name 3=Ginolfi|First name 4=Kastytis|Last name 4=Zubovas|Title=The Case for the Fundamental MBH-σ Relation|Periodical=Frontiers in Physics|Volume=8|Date=2020|issn=2296-424X|doi=10.3389/fphy.2020.00061/full|Read online=https://www.frontiersin.org/article/10.3389/fphy.2020.00061|Accessed=2022-04-17}}</ref> ||Lubang hitam ini adalah penyebab peristiwa paling energik di alam semesta yang diketahui. Tingkat energinya mencapai 5,7 juta kali lipat dari [[GRB 080916C]] dan 5 kali lipat dari [[MS 0735.6+7421]]. Perkiraan massanya berkisar hingga 400 miliar M_⊙, Namun, para ilmuwan umumnya sepakat pada massa antara 51 dan 61 miliar M_⊙. |- |[[MS 0735.6+7421|MS 0735.6+7421 BCG]] |'''{{val|5.1|e=10}}'''<ref name="dullo2019" /><ref name="dullo2021a" /> |Teleskop ruang angkasa Chandra mengamati proses penyerapan awan molekuler dengan massa 600 juta M_⊙. |- |[[NGC 8550]] |'''{{Val|5|e=10}}'''<ref>{{Web link| title=User contributions for 62.194.53.74 |url=https://universe-size-comparison.fandom.com/wiki/Special:Contributions/62.194.53.74 |consulted le=2025-04-29}}</ref> |Lubang hitam NGC terbesar yang diketahui. |- | [[HS 1946+7658]] | '''{{Val|5|e=10}}'''<ref name=":17">{{Lien web |titre=1995ApJ...438..643K Page 648 |url=https://articles.adsabs.harvard.edu//full/1995ApJ...438..643K/0000648.000.html |site=articles.adsabs.harvard.edu |consulté le=2022-07-07}}.</ref> | Dahulu dianggap sebagai kuasar paling terang di [[alam semesta]] yang dapat diamati.<ref name=":17" /> |- |[[3C 48]] |'''{{Val|5|e=10}}'''<ref>{{Web link |title=Validate User |url=https://academic.oup.com/crawlprevention/governor?content=%2fmnras%2farticle%2f368%2f3%2f1395%2f1025572 |site=academic.oup.com |consulted le=2022-04-03}}</ref> |Ini adalah salah satu kuasar pertama yang ditemukan. |- |[[SDSS J0841+3921|SDSS J0841+3921A]] |'''{{Val|4.8|e=10}}'''<ref name="Decarli">{{Article|langue=en|prénom1=Roberto|nom1=Decarli|prénom2=Fabrizio|nom2=Arrigoni-Battaia|prénom3=Joseph F.|nom3=Hennawi|prénom4=Fabian|nom4=Walter|titre=A search for dust and molecular gas in enormous Lyα nebulae at z ≈ 2|périodique=Astronomy & Astrophysics|volume=645|date=2021-01-01|issn=0004-6361|issn2=1432-0746|doi=10.1051/0004-6361/202039814|lire en ligne=https://www.aanda.org/articles/aa/abs/2021/01/aa39814-20/aa39814-20.html|consulté le=2022-05-02|pages=L3}}</ref> |Kuasar ini adalah yang paling terang dari kuadrupel pertama yang telah ditemukan. |- |[[Holmberg 15A]] || '''{{val|4.0|0.8|e=10}}'''<ref name=Merghwhatever>{{cite journal| | title = A 40-billion solar mass black hole in the extreme core of Holm 15A, the central galaxy of Abell 85 | year = 2019 | last1 = Mehrgan | first1 = K. | last2 = Thomas | first2 = J. | last3 = Saglia | first3 = R. | last4 = Massalay | first4 = X. | last5 = Erwin | first5 = P. | last6 = Bender | first6 = R. | last7 = Kluge | first7 = M. | last8 = Fabricius | first8 = M. | journal = The Astrophysical Journal | volume = 887 | issue = 2 | page = 195 | arxiv = 1907.10608 | doi = 10.3847/1538-4357/ab5856 | s2cid = 198899965 }}</ref>|| Massa yang ditentukan diperoleh melalui model Schwarzschild berbasis orbit dan simetris aksial. Perkiraan sebelumnya berkisar dari ~310 miliar M_⊙ hingga 3 miliar M_⊙, semuanya bergantung pada hubungan skala empiris dan karenanya diperoleh dari ekstrapolasi dan bukan dari pengukuran kinematika.<ref name=Cutie>{{cite journal| doi = 10.1088/2041-8205/795/2/L31 | title = The Brightest Cluster Galaxy in Abell 85: The Largest Core Known So Far | journal = The Astrophysical Journal | volume = 795 | issue = 2 | pages = L31 | year = 2014 | last1 = López-Cruz | first1 = O. | last2 = Añorve | first2 = C. | last3 = Birkinshaw | first3 = M. | last4 = Worrall | first4 = D. M. | last5 = Ibarra-Medel | first5 = H. J. | last6 = Barkhouse | first6 = W. A. | last7 = Torres-Papaqui | first7 = J. P. | last8 = Motta | first8 = V. | arxiv = 1405.7758 | bibcode = 2014ApJ...795L..31L }}</ref> |- |[[S5 0014+81#Supermassive black hole|S5 0014+81]] || '''{{val|4e10}}'''<ref name=Z1>{{cite journal| title = Chasing the heaviest black holes in active galactic nuclei, the largest black hole | journal = Monthly Notices of the Royal Astronomical Society | volume = 405 | issue = 1 | page = 387 | arxiv = 0912.0001 |bibcode = 2010MNRAS.405..387G |doi = 10.1111/j.1365-2966.2010.16449.x | year = 2010 | last1 = Ghisellini | first1 = G. | last2 = Ceca | first2 = R. Della | last3 = Volonteri | first3 = M. | last4 = Ghirlanda | first4 = G. | last5 = Tavecchio | first5 = F. | last6 = Foschini | first6 = L. | last7 = Tagliaferri | first7 = G. | last8 = Haardt | first8 = F. | last9 = Pareschi | first9 = G. | last10 = Grindlay | first10 = J. | s2cid = 40214759 }}</ref><ref name="G.Ghisellini, G.Ghirlanda">{{Cite journal|last1=Ghisellini|first1=G. |last2=Foschini|first2=L. |arxiv=0906.0575 |title=The blazar S5 0014+813: a real or apparent monster? |journal=Monthly Notices of the Royal Astronomical Society: Letters |volume=399 |issue=1 |pages=L24–L28 |date=14 July 2009 |version=v2 |last3=Volonteri |first3= M. |last4= Ghirlanda |first4=G. |last5= Haardt |first5=F. |last6= Burlon |first6=D. |last7= Tavecchio |first7=F. |doi=10.1111/j.1745-3933.2009.00716.x |bibcode = 2009MNRAS.399L..24G |s2cid=14438667 |display-authors=etal}}</ref><ref name="Bryan Gaensler">{{cite book |title=Extreme Cosmos: A Guided Tour of the Fastest, Brightest, Hottest, Heaviest, Oldest, and Most Amazing Aspects of Our Universe |url=https://books.google.com/books?id=RNvQsCMq920C&pg=PT103|isbn=978-1-101-58701-0 |last1=Gaensler |first1=Bryan |date=2012-07-03 }}</ref>|| Sebuah makalah 2010 mengusulkan bahwa sebuah corong mengkolimasi radiasi di sekitar sumbu jet, menciptakan ilusi optik dengan kecerahan sangat tinggi, dan dengan demikian kemungkinan terjadi sebuah overestimasi pada massa lubang hitam tersebut.<ref name=Z1 /> |- | [[PKS 0745-19]] || '''{{val|4|e=10}}'''<ref>{{Lien web |langue=en |titre=NASA - Monster Black Holes |url=https://www.nasa.gov/mission_pages/chandra/multimedia/monsterbh.html |site=nasa.gov |consulté le=2022-07-16 }}.</ref> ||Perkiraan ukuran maksimum, bisa lebih kecil yaitu 10 miliar M_⊙. |- | [[SDSS J0841+3921|SDSS J0841+3921B]] |'''{{val|3.7|e=10}}'''<ref name="Decarli" /> |Lubang hitam yang lebih kecil yang mengorbit SDSS J0841+3921 utama (lihat di atas); Kuasar ini adalah yang paling terang dari kuadrupel pertama yang telah ditemukan. |- | [[SDSS 143148.09+053558]] || '''{{val|3.64|e=10}}'''<ref name=Ge>{{cite journal|last1=Ge|first1=Xue|last2=Bi-Xuan|first2=Zhao|last3=Wei-Hao|first3= Bian|last4=Green Richard|first4=Frederick|title=The Blueshift of the C IV Broad Emission Line in QSOs|journal=The Astronomical Journal|date=21 March 2019|volume=157|issue=4|page=14|arxiv=1903.08830|bibcode=2019AJ....157..148G|doi=10.3847/1538-3881/ab0956|s2cid=84842636 |doi-access=free }}</ref> || |- |[[Cosmic Horseshoe|SDSS J114833.14+193003.2]] |'''{{val|3.631|0.550|0.625|e=10}}'''<ref name=Collett2025>{{Cite arXiv|display-authors=etal|date=19 February 2025|title=Unveiling a 36 Billion Solar Mass Black Hole at the Centre of the Cosmic Horseshoe Gravitational Lens|eprint=2502.13788v2 |class=astro-ph.GA |last1=Melo-Carneiro |first1=Carlos R. |last2=Collett |first2=Thomas E. |last3=Oldham |first3=Lindsay J. |last4=Enzi |first4=Wolfgang J. R. |last5=Furlanetto |first5=Cristina |last6=Chies-Santos |first6=Ana L. }}</ref> | |- |[[NGC 4874]] |'''{{val|3.47|6.30|2.24|e=10}}'''<ref name=dullo2019/><ref name=dullo2021a/> |Galaksi paling terang kedua dalam gugus [[Gugus Coma]]; diperkirakan menggunakan radius patahan inti. |- |[[SMSS J215728.21-360215.1]] || '''{{val|3.4|0.6|e=10}}'''<ref>{{citation|last1=Onken |first1=Christopher A. |last2=Bian |first2=Fuyan |last3=Fan |first3=Xiaohui |last4=Wang |first4=Feige |last5=Wolf |first5=Christian |last6=Yang |first6=Jinyi |title= thirty-four billion solar mass black hole in SMSS J2157–3602, the most luminous known quasar |journal=Monthly Notices of the Royal Astronomical Society |date=August 2020|volume=496|issue=2|page=2309|doi=10.1093/mnras/staa1635|arxiv=2005.06868|bibcode=2020MNRAS.496.2309O|doi-access=free}}</ref> ||Diperkirakan menggunakan pengukuran spektroskopi inframerah dekat dari doublet garis emisi Mg_II. |- |- |SDSS J102325.31+514251.0 || '''{{val|3.31|0.61|e=10}}'''<ref name=XA /> ||Perkiraan dari korelasi garis emisi quasar MgII. |- |[[Abell 1201 BCG]] || '''{{val|3.27|2.12}} × {{val|e=10}}'''<ref>{{citation |last1=Nightingale |first1=J. W. |last2=Smith |first2=Russell J. |last3=He |first3=Qiuhan |last4=o'Riordan |first4=Conor M. |last5=Kegerreis |first5=Jacob A. |last6=Amvrosiadis |first6=Aristeidis |last7=Edge |first7=Alastair C. |last8=Etherington |first8=Amy |last9=Hayes |first9=Richard G. |last10=Kelly |first10=Ash |last11=Lucey |first11=John R. |last12=Massey |first12=Richard J. |title= Abell 1201: detection of an ultramassive black hole in a strong gravitational lens |journal=Monthly Notices of the Royal Astronomical Society|volume =521|issue= 3|pages=3298–3322|doi=10.1093/mnras/stad587|date= May 2023|doi-access=free|arxiv=2303.15514 }} (published online 29 March 2023 )</ref> || Diperkirakan menggunakan pelensaan gravitasi yang kuat dari galaksi jauh yang berjarak 1,3 detik busur dari inti BCG. Perkiraan sebelumnya menunjukkan massa sebesar 1,3{{e|10}} {{massa Matahari}}.<ref name="smith2017a">{{cite journal | last1 = Smith | first1 = R. J. | last2 = Lucey | first2 = J. R. | last3 = Edge | first3 = A. C. | title = A counterimage to the gravitational arc in Abell 1201: Evidence for IMF variations or a 10¹⁰ M_sun black hole? | year = 2017 | journal = [[Monthly Notices of the Royal Astronomical Society]] | volume = 467 | issue = 1 | pages = 836–848 | doi = 10.1093/mnras/stx059 | doi-access = free | arxiv = 1701.02745 | bibcode = 2017MNRAS.467..836S | s2cid = 59965783 }}</ref> Waspadai ambiguitas antara penentuan massa lubang hitam dan profil materi gelap gugus galaksi.<ref name="smith2017b">{{cite journal | last1 = Smith | first1 = R. J. | last2 = Lucey | first2 = J. R. | last3 = Edge | first3 = A. C. | title = Stellar dynamics in the strong-lensing central galaxy of Abell 1201: A low stellar mass-to-light ratio a large central compact mass and a standard dark matter halo | year = 2017 | journal = [[Monthly Notices of the Royal Astronomical Society]] | volume = 1706 | issue = 1 | pages = 383–393 | arxiv = 1706.07055 | url = http://esoads.eso.org/abs/2017arXiv170607055S | bibcode = 2017MNRAS.471..383S | doi = 10.1093/mnras/stx1573 | doi-access = free | s2cid = 54757451 }} {{Dead link|date=October 2026 |bot=InternetArchiveBot |fix-attempted=yes }}</ref> |- |[[H1821+643]] || '''{{val|3e10}}'''<ref name=joe /> || Gugus galaksi terdekat yang mempunyai sebuah kuasar dalam intinya.<ref name=joe>{{cite journal |doi=10.1093/mnras/stu1067| arxiv=1405.7522v1 |last1 = Walker |first1 = S. A. |title = The effect of the quasar H1821+643 on the surrounding intracluster medium: Revealing the underlying cooling flow | journal=Monthly Notices of the Royal Astronomical Society | volume=442 | issue=3 | pages=2809 |last2 = Fabian |first2 = A. C. |last3 = Russell |first3 = H. R. |last4 = Sanders |first4 = J. S. |year = 2014 | bibcode=2014MNRAS.442.2809W | s2cid=118724526 }}</ref> |- |[[NGC 6166]] || '''{{val|3e10}}'''<ref>{{cite journal|last1=Magorrian|first1=J.|last2=Tremaine|first2=S.|last3=Richstone|first3=D.|last4=Bender|first4=R.|last5=Bower|first5=G.|last6=Dressler|first6=A.|last7=Faber|first7=S.~M.|last8=Gebhardt|first8=K.|last9=Green|first9=R.|last10=Grillmair|first10=C.|last11=Kormendy|first11=J.|last12=Lauer|first12=T.|title=The Demography of Massive Dark Objects in Galaxy Centers|url=https://archive.org/details/sim_astronomical-journal_1998-06_115_6/page/2285|journal=The Astronomical Journal|date=June 1998|volume=115|issue=6|pages=2285–2305|doi=10.1086/300353|ref=http://adsabs.harvard.edu/abs/1998AJ....115.2285M|arxiv = astro-ph/9708072 |bibcode = 1998AJ....115.2285M |s2cid=17256372}}</ref> || |- |[[APM 08279+5255]] || '''{{val|2.3|e=10}}'''<ref name="riechers2009">{{cite journal | last1 = Riechers | first1 = D. A. | last2 = Walter | first2 = F. | last3 = Carilli | first3 = C. L. | last4 = Lewis | first4 = G. F. | title = Imaging The Molecular Gas in a z = 3.9 Quasar Host Galaxy at 0farcs3 Resolution: A Central Sub-Kiloparsec Scale Star Formation Reservoir in APM 08279+5255 | url = https://archive.org/details/sim_astrophysical-journal_2009-01-01_690_1/page/462 | year = 2009 | journal = [[The Astrophysical Journal]] | volume = 690 | issue = 1 | pages = 463–485 | doi = 10.1088/0004-637X/690/1/463 | arxiv = 0809.0754 | bibcode = 2009ApJ...690..463R | s2cid = 13959993 }}</ref><br />'''{{val|1.0|0.17|0.13|e=10}}'''<ref name="saturni2016">{{cite journal | last1 = Saturni | first1 = F. G. | last2 = Trevese | first2 = D. | last3 = Vagnetti | first3 = F. | last4 = Perna | first4 = M. | last5 = Dadina | first5 = M. | title = A multi-epoch spectroscopic study of the BAL quasar APM 08279+5255. II. Emission- and absorption-line variability time lags | year = 2016 | journal = [[Astronomy and Astrophysics]] | volume = 587 | pages = A43 | doi = 10.1051/0004-6361/201527152 | arxiv = 1512.03195 | bibcode = 2016A&A...587A..43S | s2cid = 118548618 }}</ref> || Based on velocity width of CO line from orbiting molecular gas,<ref name="riechers2009" /> and [[reverberation mapping]] using SiIV and CIV emission lines.<ref name="saturni2016" /> |- |[[NGC 4889]] || '''{{val|2.1|1.6|e=10}}'''<ref name="McConnell">{{Cite journal|arxiv=1112.1078|last1= McConnell|first1= Nicholas J.|title= Two ten-billion-solar-mass black holes at the centres of giant elliptical galaxies|url=https://archive.org/details/sim_nature-uk_2011-12-08_480_7376/page/214|journal= Nature|volume= 480|issue= 7376|pages= 215–8|last2= Ma|first2= Chung-Pei|authorlink2=Chung-Pei Ma|last3= Gebhardt|first3= Karl|last4= Wright|first4= Shelley A.|last5= Murphy|first5= Jeremy D.|last6= Lauer|first6= Tod R.|last7= Graham|first7= James R.|last8= Richstone|first8= Douglas O.|year= 2011|doi= 10.1038/nature10636|pmid= 22158244|bibcode= 2011Natur.480..215M|s2cid= 4408896}}</ref><ref name="mcconnell2012">{{cite journal | last1 = McConnell | first1 = N. J. | last2 = Ma | first2 = C.-P. | last3 = Murphy | first3 = J. D. | last4 = Gebhardt | first4 = K. | last5 = Lauer | first5 = T. R. | last6 = Graham | first6 = J. R. | last7 = Wright | first7 = S. A. | last8 = Richstone | first8 = D. O. | title = Dynamical Measurements of Black Hole Masses in Four Brightest Cluster Galaxies at 100 Mpc | year = 2012 | journal = [[The Astrophysical Journal]] | volume = 756 | issue = 2 | pages = 179 | doi = 10.1088/0004-637X/756/2/179 | arxiv = 1203.1620 | bibcode = 2012ApJ...756..179M | s2cid = 119114155 }}</ref> ||Best fit: the estimate ranges from 6 billion to 37 billion {{Solar mass}}.<ref name="McConnell" /><ref name="mcconnell2012" /> |- | [[SDSS J074521.78+734336.1]] || '''{{val|1.95|0.05|e=10}}'''<ref name=XA /> ||Estimated from quasar MgII emission line correlation. |- |[[OJ 287]] primary || '''{{val|1.8e10}}'''<ref name="frostbite">{{Cite journal|arxiv =1208.0906 |last1 = Valtonen |first1 = M. J. |title = On the masses of OJ287 black holes |journal = Monthly Notices of the Royal Astronomical Society |volume = 427 |issue = 1 |pages = 77–83 |last2 = Ciprini |first2 = S. |last3 = Lehto |first3 = H. J. |year = 2012 |doi = 10.1111/j.1365-2966.2012.21861.x |bibcode = 2012MNRAS.427...77V |s2cid = 118483466 }}</ref> || A smaller 100 million {{Solar mass}} black hole orbits this one in a 12-year period (see ''OJ 287 secondary'' below). But this measurement is in question due to the limited number and precision of observed companion orbits. |- |[[QSO J0529-4351|SMSS J052915.80-435152.0]] |'''{{Val|1.7|e=10}}'''<ref>{{Cite web |last=University |first=Australian National |title=Supermassive black hole spews gas at record speeds, upending mass estimates |url=https://phys.org/news/2025-09-supermassive-black-hole-spews-gas.html |access-date=2025-09-30 |website=phys.org |language=en}}</ref> |Lubang hitam dengan pertumbuhan tercepat, objek paling bercahaya di alam semesta, cakram akresi terbesar (7 tahun cahaya). |- | [[NGC 1600]] || '''{{val|1.7|0.15|e=10}}'''<ref name="thomas2016">{{cite journal | last1 = Thomas | first1 = J. | last2 = Ma | first2 = C.-P. | last3 = McConnell | first3 = N. J. | last4 = Greene | first4 = J. E. | last5 = Blakeslee | first5 = J. P. | last6 = Janish | first6 = R. | title = A 17-billion-solar-mass black hole in a group galaxy with a diffuse core | year = 2016 | journal = [[Nature (journal)|Nature]] | volume = 532 | issue = 7599 | pages = 340–342 | doi = 10.1038/nature17197 | pmid = 27049949 | arxiv = 1604.01400 | bibcode = 2016Natur.532..340T | s2cid = 4454301 }}</ref><ref name="Behemoth Black Hole Found in an Unlikely Place">{{cite web|url=http://www.nasa.gov/feature/goddard/2016/behemoth-black-hole-found-in-an-unlikely-place|title=Behemoth Black Hole Found in an Unlikely Place|first=Ashley|last=Morrow|date=5 April 2016}}</ref> || Unprecedentedly massive in relation of its location: an elliptical galaxy host in a sparse environment. |- | [[SDSS J08019.69+373047.3]] || '''{{val|1.51|0.31|e=10}}'''<ref name=XA /> ||Estimated from quasar MgII emission line correlation. |- | [[SDSS J115954.33+201921.1]] || '''{{val|1.41|0.10|e=10}}'''<ref name=XA /> ||Estimated from quasar MgII emission line correlation. |- | [[SDSS J075303.34+423130.8]] || '''{{val|1.38|0.03|e=10}}'''<ref name=XA>{{Cite journal|arxiv =1412.2438 |last1 =Zuo |first1 =Wenwen |title =Black Hole Mass Estimates and Rapid Growth of Supermassive Black Holes in Luminous $z \sim$ 3.5 Quasars |journal =The Astrophysical Journal |volume =799 |issue =2 |pages =189 |last2 =Wu |first2 =Xue-Bing |last3 =Fan |first3 =Xiaohui |last4 =Green |first4 =Richard |last5 =Wang |first5 =Ran |last6 =Bian |first6 =Fuyan |year =2014 |doi =10.1088/0004-637X/799/2/189 |bibcode =2015ApJ...799..189Z |s2cid =73642040 }}</ref> ||Estimated from quasar Hβ emission line correlation. |- | [[SDSS J080430.56+542041.1]] || '''{{val|1.35|0.22|e=10}}'''<ref name=XA /> ||Estimated from quasar MgII emission line correlation. |- | [[SDSS J0100+2802]] || '''{{val|1.24|0.19|e=10}}'''<ref name="Wu">{{cite journal | last1 = Wu | first1 = X. | last2 = Wang | first2 = F. | last3 = Fan | first3 = X. | last4 = Yi | first4 = Weimin | last5 = Zuo | first5 = Wenwen | last6 = Bian | first6 = Fuyan | last7 = Jiang | first7 = Linhua | last8 = McGreer | first8 = Ian D. | last9 = Wang | first9 = Ran | last10 = Yang | first10 = Jinyi | last11 = Yang | first11 = Qian | last12 = Thompson | first12 = David | last13 = Beletsky | first13 = Yuri | title = An ultraluminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30 | url = https://archive.org/details/sim_nature-uk_nature_2015-02-26_518_7540/page/512 | journal = Nature | volume = 518| issue = 7540 | pages = 512–515 | date = 25 February 2015 |bibcode = 2015Natur.518..512W|doi = 10.1038/nature14241 | pmid = 25719667 |arxiv = 1502.07418| s2cid = 4455954 }}</ref><ref name="sci-news">{{cite web| title=Astronomers Discover Record-Breaking Quasar | work=Sci-News.com | url=http://www.sci-news.com/astronomy/science-sdss-j01002802-record-breaking-quasar-02539.html/ | date=2015-02-25 |access-date=2015-02-27 }}</ref>|| Estimated from quasar MgII emission line correlation. This object grew early in cosmic history ([[redshift]] 6.30). |- | [[SDSS J081855.77+095848.0]] || '''{{val|1.20|0.06|e=10}}'''<ref name=XA /> ||Estimated from quasar MgII emission line correlation. |- | [[NGC 1270]] || '''{{val|1.2|e=10}}'''<ref>{{Cite journal|last1=Ferré-Mateu|first1=Anna|last2=Mezcua|first2=Mar|last3=Trujillo|first3=Ignacio|last4=Balcells|first4=Marc|last5=Bosch|first5=Remco C. E. van den|date=2015-07-21|journal=The Astrophysical Journal|language=en|volume=808|issue=1|pages=79|doi=10.1088/0004-637X/808/1/79|issn=1538-4357|bibcode=2015ApJ...808...79F|arxiv=1506.02663|title=Massive Relic Galaxies Challenge the Co-Evolution of Super-Massive Black Holes and Their Host Galaxies|s2cid=118777377}}</ref> ||Elliptical galaxy located in the [[Perseus Cluster]]. Also is a low-luminosity [[Active galactic nucleus|AGN]] (LLAGN).<ref>{{Cite journal|last1=Park|first1=Songyoun|last2=Yang|first2=Jun|last3=Oonk|first3=J. B. Raymond|last4=Paragi|first4=Zsolt|date=2016-11-22|title=Discovery of five low-luminosity active galactic nuclei at the centre of the Perseus cluster|url=http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1611.05986|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=465|issue=4|pages=3943–3948|doi=10.1093/mnras/stw3012|issn=0035-8711|arxiv=1611.05986|bibcode=2017MNRAS.465.3943P|s2cid=53538944}}</ref> |- | [[SDSS J082535.19+512706.3]] || '''{{val|1.12|0.20|e=10}}'''<ref name=XA /> ||Estimated from quasar Hβ emission line |- | [[SDSS J013127.34-032100.1]] || '''{{val|1.1|0.2|e=10}}'''<ref name=Chitz>{{Cite journal|arxiv = 1501.07269|last1 = Ghisellini|first1 = G.|title = SDSS J013127.34-032100.1: A candidate blazar with a 11 billion solar mass black hole at $z$=5.18|journal = Monthly Notices of the Royal Astronomical Society: Letters|volume = 450|pages = L34–L38|last2 = Tagliaferri|first2 = G.|last3 = Sbarrato|first3 = T.|last4 = Gehrels|first4 = N.|year = 2015|doi = 10.1093/mnrasl/slv042|bibcode = 2015MNRAS.450L..34G|s2cid = 118449836}}</ref> || Estimated from accretion disk spectrum modelling.<ref name="Chitz" /> |- | PSO J334.2028+01.4075 || '''{{val|1e10}}'''<ref name=a7 /> || There are actually two black holes, orbiting at each other in a close pair with a 542-day period. The largest one is quoted, while the smaller one's mass is not defined.<ref name=a7>{{Cite journal|arxiv =1503.02083 |last1 =Liu |first1 =Tingting |title =A Periodically Varying Luminous Quasar at z=2 from the Pan-STARRS1 Medium Deep Survey: A Candidate Supermassive Black Hole Binary in the Gravitational Wave-Driven Regime |journal =The Astrophysical Journal |volume =803 |issue =2 |pages =L16 |last2 =Gezari |first2 =Suvi |last3 =Heinis |first3 =Sebastien |last4 = Magnier |first4 =Eugene A. |last5 = Burgett |first5 =William S. |last6 =Chambers |first6 =Kenneth |last7 =Flewelling |first7 =Heather |last8 =Huber |first8 =Mark |last9 = Hodapp |first9 =Klaus W. |last10 =Kaiser |first10 =Nicholas |last11 =Kudritzki |first11 =Rolf-Peter |last12 = Tonry |first12 =John L. |last13 = Wainscoat |first13 =Richard J. |last14 =Waters |first14 =Christopher |year =2015 |doi =10.1088/2041-8205/803/2/L16 |bibcode =2015ApJ...803L..16L |s2cid =118580031 }}</ref> |- |Black hole of central elliptical galaxy of [[RX J1532.9+3021]] || '''{{val|1e10}}'''<ref name="chandra">{{cite journal | lay-url =http://chandra.harvard.edu/photo/2014/rxj1532/|arxiv=1306.0907 |title=Probing the extreme realm of AGN feedback in the massive galaxy cluster, RX J1532.9+3021|journal=The Astrophysical Journal |volume=777 |issue=2 |pages=163 |doi=10.1088/0004-637X/777/2/163 |year=2013 |last1=Hlavacek-Larrondo |first1=J. |last2=Allen |first2=S. W. |last3=Taylor |first3=G. B. |last4=Fabian |first4=A. C. |last5=Canning |first5=R. E. Ato. |last6=Werner |first6=N. |last7=Sanders |first7=J. S. |last8=Grimes |first8=C. K. |last9=Ehlert |first9=S. |last10=von Der Linden |first10=A. |bibcode=2013ApJ...777..163H |s2cid=118597740 }}</ref> || |- | [[QSO B2126-158]]|| '''{{val|1e10}}'''<ref name=Z1 /> || |- | [[NGC 1281]] || '''{{val|1e10}}'''<ref>{{Cite journal|last1=Yıldırım|first1=Akın|last2=Bosch|first2=Van Den|last3=E|first3=Remco C.|last4=van de Ven|first4=Glenn|last5=Dutton|first5=Aaron|last6=Läsker|first6=Ronald|last7=Husemann|first7=Bernd|last8=Walsh|first8=Jonelle L.|last9=Gebhardt|first9=Karl|date=2016-02-11|title=The massive dark halo of the compact early-type galaxy NGC 1281|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=456|issue=1|pages=538–553|doi=10.1093/mnras/stv2665|issn=0035-8711|bibcode=2016MNRAS.456..538Y|arxiv=1511.03131|s2cid=118483580}}</ref> || Compact [[elliptical galaxy]] in the [[Perseus Cluster]]. Mass estimates range from 10 billion {{Solar mass}} down to <5 billion {{Solar mass}}.<ref>{{Cite journal|last1=Ferré-Mateu|first1=Anna|last2=Mezcua|first2=Mar|last3=Trujillo|first3=Ignacio|last4=Balcells|first4=Marc|last5=Bosch|first5=Remco C. E. van den|date=2015-07-21|journal=The Astrophysical Journal|language=en|volume=808|issue=1|pages=79|doi=10.1088/0004-637x/808/1/79|issn=1538-4357|bibcode=2015ApJ...808...79F|arxiv=1506.02663|title=Massive Relic Galaxies Challenge the Co-Evolution of Super-Massive Black Holes and Their Host Galaxies|s2cid=118777377}}</ref> |- | [[SDSS J015741.57-010629.6]] || '''{{val|9.8|1.4|e=9}}'''<ref name=XA /> || |- | [[SDSS J230301.45-093930.7]] || '''{{val|9.12|0.88|e=9}}'''<ref name=XA /> ||Estimated from quasar MgII emission line correlation. |- | [[SDSS J075819.70+202300.9]] || '''{{val|7.8|3.9|e=9}}'''<ref name=XA /> ||Estimated from quasar Hβ emission line correlation. |- | [[CID-947]] || '''{{val|6.9|0.8|1.2|e=9}}'''<ref name=nugget>{{Cite journal|arxiv =1507.02290 |last1 =Trakhtenbrot |first1 =Benny |title =An Over-Massive Black Hole in a Typical Star-Forming Galaxy, 2 Billion Years After the Big Bang |journal =Science |volume =349 |issue =168 |last2 = Megan Urry |first2 =C. |last3 =Civano |first3 =Francesca |last4 = Rosario |first4 =David J. |last5 =Elvis |first5 =Martin |last6 =Schawinski |first6 =Kevin |last7 =Suh |first7 =Hyewon |last8 =Bongiorno |first8 =Angela |last9 = Simmons |first9 =Brooke D. |year =2015 |bibcode = 2015Sci...349..168T |doi = 10.1126/science.aaa4506 |pmid =26160942 |pages=168–171|s2cid =22406584 }}</ref> || Constitutes 10% of the total mass of its host galaxy. Estimated from quasar Hβ emission line correlation. |- | [[SDSS J080956.02+502000.9]] || '''{{val|6.46|0.45|e=9}}'''<ref name=XA /> ||Estimated from quasar Hβ emission line correlation. |- | [[SDSS J014214.75+002324.2]] || '''{{val|6.31|1.16|e=9}}'''<ref name=XA /> ||Estimated from quasar MgII emission line correlation. |- | [[Messier 87]] "''Powehi''"<ref>{{cite news |url = https://www.theguardian.com/science/2019/apr/12/powehi-black-hole-gets-a-name-meaning-the-adorned-fathomless-dark-creation |title = Powehi: black hole gets a name meaning 'the adorned fathomless dark creation' |access-date= 6 May 2019|newspaper = The Guardian |date = 2019-04-12 |agency = Associated Press }}</ref> || '''{{val|7.22|0.34|0.40|e=9}}'''<ref name="oldham2016">{{cite journal | last1 = Oldham | first1 = L. J. | last2 = Auger | first2 = M. W. | title = Galaxy structure from multiple tracers – II. M87 from parsec to megaparsec scales | year = 2016 | journal = [[Monthly Notices of the Royal Astronomical Society]] | volume = 457 | issue = 1 | pages = 421–439 | doi = 10.1093/mnras/stv2982 | arxiv = 1601.01323 | bibcode = 2016MNRAS.457..421O | s2cid = 119166670 }}</ref><br />'''{{val|6.3e9}}'''<ref name=jwalsh>{{cite journal | author=Walsh, Jonelle L. | author2= Barth, Aaron J. | author3= Ho, Luis C. | author4= Sarzi, Marc | title=The M87 Black Hole Mass from Gas-dynamical Models of Space Telescope Imaging Spectrograph Observations | journal=The Astrophysical Journal | volume=770 | issue=2 |page=86 |date=June 2013 | doi= 10.1088/0004-637X/770/2/86 | bibcode= 2013ApJ...770...86W |arxiv = 1304.7273 | s2cid= 119193955 }}</ref> || Central galaxy of the [[Virgo Cluster]]; the first black hole directly imaged. |- | NGC 5419 || '''{{val|7.2|2.7|1.9|e=9}}'''<ref name="mazzalay2016">{{cite journal | last1 = Mazzalay | first1 = X. | last2 = Thomas | first2 = J. | last3 = Saglia | first3 = R. P. | last4 = Wegner | first4 = G. A. | last5 = Bender | first5 = R. | last6 = Erwin | first6 = P. | last7 = Fabricius | first7 = M. H. | last8 = Rusli | first8 = S. P. | title = The supermassive black hole and double nucleus of the core elliptical NGC 5419 | year = 2016 | journal = [[Monthly Notices of the Royal Astronomical Society]] | volume = 462 | issue = 3 | pages = 2847–2860 | doi = 10.1093/mnras/stw1802 | arxiv = 1607.06466 | bibcode = 2016MNRAS.462.2847M | s2cid = 119236364 }}</ref> ||Estimated from the stellar velocity distribution. A secondary satellite SMBH may orbit around 70 parsecs.<ref name="mazzalay2016" /> |- | [[SDSS J025905.63+001121.9]] || '''{{val|5.25|0.73|e=9}}'''<ref name=XA /> ||Estimated from quasar Hβ emission line correlation. |- | [[SDSS J094202.04+042244.5]] || '''{{val|5.13|0.71|e=9}}'''<ref name=XA /> ||Estimated from quasar Hβ emission line correlation. |- | QSO B0746+254 || '''{{val|5e9}}'''<ref name=Z1 />|| |- | QSO B2149-306 || '''{{val|5e9}}'''<ref name=Z1 />|| |- | [[SDSS J090033.50+421547.0]] || '''{{val|4.7|0.2|e=9}}'''<ref name=XA /> ||Estimated from quasar MgII emission line correlation. |- |[[Messier 60]] || '''{{val|4.5|1.0|e=9}}'''<ref>{{cite journal|author=Juntai Shen |author2=Karl Gebhardt |date=2010 |title=The Supermassive Black Hole and Dark Matter Halo of NGC 4649 (M60) |journal=The Astrophysical Journal |volume=711 |issue=1 |pages=484–494 |arxiv=0910.4168|doi=10.1088/0004-637X/711/1/484 |bibcode = 2010ApJ...711..484S |s2cid=119291328 }}</ref>|| |- | [[SDSS J011521.20+152453.3]] || '''{{val|4.1|2.4|e=9}}'''<ref name=XA /> ||Estimated from quasar Hβ emission line correlation. |- | QSO B0222+185 || '''{{val|4e9}}'''<ref name=Z1 />|| |- |[[Hercules A]] (''3C 348'') || '''{{val|4e9}}''' || Notable for its million light-year long [[Polar jet#Relativistic jet|relativistic jet]]. |- | Abell 1836-BCG || '''{{val|3.61|0.41|0.50|e=9}}'''<ref name="dalla2009">{{cite journal | last1 = Dalla Bontà| first1 = E. | last2 = Ferrarese | first2 = L. | last3 = Corsini | first3 = E. M. | last4 = Miralda-Escudé | first4 = J. | last5 = Coccato | first5 = L. | last6 = Sarzi | first6 = M. | last7 = Pizzella | first7 = A. | last8 = Beifiori | first8 = A. | title = The High-Mass End of the Black Hole Mass Function: Mass Estimates in Brightest Cluster Galaxies | url = https://archive.org/details/sim_astrophysical-journal_2009-01-01_690_1/page/536| year = 2009 | journal = [[The Astrophysical Journal]] | volume = 690 | issue = 1 | pages = 537–559 | doi = 10.1088/0004-637X/690/1/537 | arxiv = 0809.0766 | bibcode = 2009ApJ...690..537D | s2cid = 17074507 }}</ref> || |- | [[SDSS J213023.61+122252.0]] || '''{{val|3.5|0.2|e=9}}'''<ref name=XA /> ||Estimated from quasar Hβ emission line correlation. |- | [[SDSS J173352.23+540030.4]] || '''{{val|3.4|0.4|e=9}}'''<ref name=XA />||Estimated from quasar MgII emission line correlation. |- | [[SDSS J025021.76-075749.9]] || '''{{val|3.1|0.6|e=9}}'''<ref name=XA />||Estimated from quasar MgII emission line correlation. |- | [[NGC 1271]] || '''{{Val|3.0|1.0|1.1|e=9}}'''<ref>{{Cite journal|last1=Walsh|first1=Jonelle L.|last2=Bosch|first2=Remco C. E. van den|last3=Gebhardt|first3=Karl|last4=Yildirim|first4=Akin|last5=Gültekin|first5=Kayhan|last6=Husemann|first6=Bernd|last7=Richstone|first7=Douglas O.|date=2015-08-03|url=http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1506.05129|journal=The Astrophysical Journal|language=en|volume=808|issue=2|pages=183|doi=10.1088/0004-637X/808/2/183|issn=1538-4357|bibcode=2015ApJ...808..183W|arxiv=1506.05129|title=The Black Hole in the Compact, High-Dispersion Galaxy NGC 1271|s2cid=41570998}}</ref> ||Compact [[Elliptical galaxy|elliptical]] or [[lenticular galaxy]] in the [[Perseus Cluster]].<ref>{{Cite journal|last1=Graham|first1=Alister W.|last2=Ciambur|first2=Bogdan C.|last3=Savorgnan|first3=Giulia A. D.|date=2016|title=Disky Elliptical Galaxies and the Allegedly Over-massive Black Hole in the Compact "ES" Galaxy NGC 1271|journal=The Astrophysical Journal|language=en|volume=831|issue=2|pages=132|doi=10.3847/0004-637X/831/2/132|issn=0004-637X|bibcode=2016ApJ...831..132G|arxiv=1608.00711|hdl=1959.3/432781|s2cid=118435675}}</ref> |- | [[SDSS J030341.04-002321.9]] || '''{{val|3.0|0.4|e=9}}'''<ref name=XA /> ||Estimated from quasar MgII emission line correlation. |- | QSO B0836+710 || '''{{val|3e9}}'''<ref name=Z1 /> || |- | [[SDSS J224956.08+000218.0]] || '''{{val|2.63|1.21|e=9}}'''<ref name=XA /> ||Estimated from quasar Hβ emission line correlation. |- | [[SDSS J030449.85-000813.4]] || '''{{val|2.4|0.50|e=9}}'''<ref name=XA /> ||Estimated from quasar Hβ emission line correlation. |- | [[SDSS J234625.66-001600.4]] || '''{{val|2.24|0.15|e=9}}'''<ref name=XA /> ||Estimated from quasar Hβ emission line correlation. |- | [[PKS 2128-123]] || '''{{val|2.02e9}}'''<ref name="ReferenceB">{{Cite journal|doi = 10.1086/341729|title = Black Hole Mass Estimates of Radio‐selected Quasars|url = https://archive.org/details/sim_astrophysical-journal_2002-09-01_576_1/page/80|year = 2002|last1 = Oshlack|first1 = A. Y. K. N.|last2 = Webster|first2 = R. L.|last3 = Whiting|first3 = M. T.|journal = The Astrophysical Journal|volume = 576|pages = 81–88|s2cid = 15343258}}</ref> || |- |[[ULAS J1120+0641]] || '''{{val|2e9}}'''<ref name=mortlock>{{cite journal |title=A luminous quasar at a redshift of z = 7.085 |url=https://archive.org/details/sim_nature-uk_2011-06-30_474_7353/page/616 |author=Daniel J. Mortlock |author2=Stephen J. Warren |author3=Bram P. Venemans |display-authors=etal |journal=Nature |volume=474 |issue=7353 |pages=616–619 |date=2011 |doi=10.1038/nature10159|pmid=21720366 |arxiv=1106.6088 |bibcode = 2011Natur.474..616M |last4=Patel |last5=Hewett |last6=McMahon |last7=Simpson |last8=Theuns |last9=Gonzáles-Solares |last10=Adamson |last11=Dye |last12=Hambly |last13=Hirst |last14=Irwin |last15=Kuiper |last16=Lawrence |last17=Röttgering |s2cid=2144362 }}</ref><ref name=SciAm-2011-06-29>{{cite magazine |title=Brilliant, but Distant: Most Far-Flung Known Quasar Offers Glimpse into Early Universe |author=John Matson |date=2011-06-29 |magazine=Scientific American |url=http://www.scientificamerican.com/article.cfm?id=farthest-quasar |access-date=2011-06-30 }}</ref> || |- | QSO 0537-286 || '''{{val|2e9}}'''<ref name=Z1 /> || |- |[[NGC 3115]] || '''{{val|2e9}}'''<ref>{{cite journal|bibcode=1992ApJ...393..559K|pages= 559–578|doi=10.1086/171528|title= Evidence for a supermassive black hole in NGC 3115|url=https://archive.org/details/sim_astrophysical-journal_1992-07-10_393_2/page/n155|journal= The Astrophysical Journal|volume= 393|year= 1992|last1= Kormendy|first1= John|last2= Richstone|first2= Douglas}}</ref> || |- | [[Q0906+6930]] || '''{{val|2e9}}'''<ref name=Romani2006>{{cite journal |last=Romani |first=Roger W. |title=The Spectral Energy Distribution of the High-z Blazar Q0906+6930 |url=https://archive.org/details/sim_astronomical-journal_2006-11_132_5/page/1959 |journal=The Astronomical Journal |volume=132 |issue=5 |pages=1959–1963 |date=2006 |doi=10.1086/508216 |bibcode=2006AJ....132.1959R |arxiv = astro-ph/0607581 |s2cid=119331684 }}</ref> || Most distant [[blazar]], at [[Redshift|z]] = 5.47 |- | QSO B0805+614 || '''{{val|1.5e9}}'''<ref name=Z1 /> || |- |[[Messier 84]] || '''{{val|1.5e9}}'''<ref name="Bower et al. 1998">{{cite journal | author=Bower, G.A. | date=1998| title=Kinematics of the Nuclear Ionized Gas in the Radio Galaxy M84 (NGC 4374) | url=https://archive.org/details/sim_astrophysical-journal_1998-01-01_492_1/page/110 | journal=[[Astrophysical Journal]] | volume=492 | issue=1 | pages=111–114 | bibcode=1998ApJ...492L.111B | doi=10.1086/311109|arxiv = astro-ph/9710264 | last2=Green | first2=R. F. | last3=Danks | first3=A. | last4=Gull | first4=T. | last5=Heap | first5=S. | last6=Hutchings | first6=J. | last7=Joseph | first7=C. | last8=Kaiser | first8=M. E. | last9=Kimble | first9=R. | last10=Kraemer| first10=S.| last11=Weistrop| first11=D.| last12=Woodgate| first12=B.| last13=Lindler| first13=D.| last14=Hill| first14=R. S.| last15=Malumuth| first15=E. M.| last16=Baum| first16=S.| last17=Sarajedini| first17=V.| last18=Heckman| first18=T. M.| last19=Wilson| first19=A. S.| last20=Richstone| first20=D. O.| s2cid=119456112}}</ref> || |- | [[Pōniuāʻena|J100758.264+211529.207 ("Pōniuāʻena")]] || '''{{val|1.5|0.2|e=9}}'''<ref>{{cite journal| title=Pōniuāʻena: A Luminous z=7.5 Quasar Hosting a 1.5 Billion Solar Mass Black Hole |authors=Jinyi Yang and Feige Wang and Xiaohui Fan and Joseph F. Hennawi and Frederick B. Davies and Minghao Yue and Eduardo Banados and Xue-Bing Wu and Bram Venemans and Aaron J. Barth and Fuyan Bian and Konstantina Boutsia and Roberto Decarli and Emanuele Paolo Farina and Richard Green and Linhua Jiang and Jiang-Tao Li and Chiara Mazzucchelli and Fabian Walter |year=2020 |doi=10.3847/2041-8213/ab9c26 |arxiv=2006.13452 |s2cid=220042206 }} </ref> || Second most-distant quasar known |- | [[PKS 2059+034]] | '''{{val|1.36e9}}'''<ref name="ReferenceB"/> | |- | Abell 3565-BCG || '''{{val|1.34|0.21|0.19|e=9}}'''<ref name="dalla2009" /> || |- |[[NGC 7768]] || '''{{val|1.3|0.5|0.4|e=9}}'''<ref name="mcconnell2012" /> || |- |[[NGC 1277]] || '''{{val|1.2e9}}'''<ref name=graham>{{cite journal|last1=Graham|first1=Alister W.|last2=Durré|first2=Mark|last3=Savorgnan|first3=Giulia A. D.|last4=Medling|first4=Anne M.|last5=Batcheldor|first5=Dan|last6=Scott|first6=Nicholas|last7=Watson|first7=Beverly|last8=Marconi|first8=Alessandro|title=A Normal Supermassive Black Hole in NGC 1277|journal=The Astrophysical Journal|date=1 March 2016|volume=819|issue=1|pages=43|doi=10.3847/0004-637X/819/1/43|issn=0004-637X|bibcode=2016ApJ...819...43G|arxiv = 1601.05151 |s2cid=36974319}}</ref>|| Once thought to harbor a black hole so large that it contradicted modern galaxy formation and evolutionary theories,<ref name=vandenBosch>{{cite journal |last1=van den Bosch |first1=Remco C. E. |last2=Gebhardt |first2=Karl |last3=Gültekin |first3=Kayhanl |last4=van de Ven |first4=Glenn |last5=van der Wel |first5=Arjen |last6=Walsh |first6=Jonelle L. |title=An over-massive black hole in the compact lenticular galaxy NGC 1277 |url=https://archive.org/details/sim_nature-uk_2012-11-29_491_7426/page/729 |journal=[[Nature (journal)|Nature]] |volume=491 |issue=7426 |pages=729–731 |date=29 Nov 2012 |doi=10.1038/nature11592 |arxiv = 1211.6429 |bibcode = 2012Natur.491..729V |pmid=23192149|s2cid=205231230 }}</ref> re-analysis of the data revised it downward to roughly a third of the original estimate.<ref name=Emsellem>{{cite journal |last=Emsellem |first=Eric |title=Is the black hole in NGC 1277 really overmassive? |journal=[[Monthly Notices of the Royal Astronomical Society]] |volume=433 |issue=3 |pages=1862–1870 |date=Aug 2013 |doi=10.1093/mnras/stt840 |bibcode = 2013MNRAS.433.1862E |arxiv = 1305.3630 |s2cid=54011632 }}</ref> and then one tenth.<ref name=graham /> |- | QSO B225155+2217 || '''{{val|1e9}}'''<ref name=Z1 /> || |- | QSO B1210+330 || '''{{val|1e9}}'''<ref name=Z1 /> || |- | [[NGC 6166]] || '''{{val|1e9}}'''<ref name="Di Matteo L19">{{cite journal |last1=Di Matteo |first1=Tiziana |last2=Johnstone |first2=Roderick M |last3=Allen |first3=Steven W. |last4=Fabian |first4=Andrew C. |date=March 8, 2001 |title=Accretion onto Nearby Supermassive Black Holes: Chandra Constraints on the Dominant Cluster Galaxy NGC 6166 |journal=The Astrophysical Journal |volume=550 |issue=1 |page=L19 |arxiv= astro-ph/0012194|bibcode = 2001ApJ...550L..19D |doi = 10.1086/319489 |s2cid=15581216 }}</ref> || Central galaxy of [[Abell 2199]]; notable for its hundred thousand light year long relativistic jet. |- | [[Cygnus A]] || '''{{val|1e9}}'''<ref name=Hubbubble>{{cite web|url=http://hubblesite.org/explore_astronomy/black_holes/encyc_mod1_q12.html |title=Black Holes: Gravity's Relentless Pull interactive: Encyclopedia |publisher=HubbleSite |date= |access-date=2015-05-20}}</ref> || Brightest extrasolar radio source in the sky as seen at frequencies above 1&nbsp;GHz |- | [[Sombrero Galaxy]] || '''{{val|1e9}}'''<ref name="kormendyetal1996">{{cite journal | author=J. Kormendy | author2=R. Bender | author3=E. A. Ajhar| author4=A. Dressler | author5=S. M. Faber| author6=K. Gebhardt | author7=C. Grillmair| author8=T. R. Lauer | author9=D. Richstone| author10=S. Tremaine | date=1996 | title=Hubble Space Telescope Spectroscopic Evidence for a 1 X 10 9 M_sun Black Hole in NGC 4594 | journal=[[Astrophysical Journal Letters]] | volume=473 | issue=2 | pages=L91–L94 | bibcode=1996ApJ...473L..91K | doi=10.1086/310399| doi-access=free }}</ref> || Bolometrically most luminous galaxy in the local universe and also the nearest billion-solar-mass black hole to Earth. |- | [[Markarian 501]] || '''{{val|9e8}}–{{val|3.4e9}}'''<ref name="Rieger">{{cite journal|doi=10.1051/0004-6361:20021482|bibcode=2003A&A...397..121R|title=On the central black hole mass in Mkn 501|arxiv=astro-ph/0210326v1|journal=Astronomy and Astrophysics|volume=397|pages=121–126|year=2003|last1=Rieger|first1=F. M.|last2=Mannheim|first2=K.|s2cid=14579804}}</ref> || Brightest object in the sky in very high energy gamma rays. |- | [[PG 1426+015]] || '''{{val|1.298|0.385|e=9}}'''<ref name="1A">{{cite journal | doi = 10.1007/s11214-013-9987-4 | title = Measuring the Masses of Supermassive Black Holes | journal = Space Science Reviews | volume = 183 | issue = 1–4 | page = 253 | url = http://www.astronomy.ohio-state.edu/~peterson/Docs/petersonISSI.pdf | year = 2013 | last1 = Peterson | first1 = Bradley M. | bibcode = 2014SSRv..183..253P | s2cid = 16464532 | access-date = 2015-03-12 | archive-date = 2019-07-26 | archive-url = https://web.archive.org/web/20190726032645/http://www.astronomy.ohio-state.edu/~peterson/Docs/petersonISSI.pdf | url-status = dead }}</ref><br />'''{{val|467740000}}'''<ref name="2A">{{cite journal|doi=10.1086/317314|title=Black Hole Mass, Velocity Dispersion, and the Radio Source in Active Galactic Nuclei|journal=The Astrophysical Journal|volume=544|issue=2|pages=L91–L94|year=2000|last1=Nelson|first1=Charles H.|bibcode=2000ApJ...544L..91N|arxiv = astro-ph/0009188 |s2cid=117449813}}</ref> || |- | [[3C 273]] || '''{{val|8.86|1.87|e=8}}'''<ref name= 1A /><br />'''{{val|550000000}}'''<ref name=2A /> || Kuasar terterang di langit |- | [[ULAS J1342+0928]] || '''{{val|8|e=8}}'''<ref name="NAT-20171206">{{cite journal |author=Bañados, Eduardo |display-authors=et al |title=An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5 |date=6 December 2017 |journal=[[Nature (journal)|Nature]] |volume=553 |issue=7689 |pages=473–476 |doi=10.1038/nature25180 |pmid=29211709 |arxiv=1712.01860 |bibcode=2018Natur.553..473B |s2cid=205263326 }}</ref> || Kuasar paling jauh<ref name="NAT-20171206" /> − saat ini tercatat sebagai kuasar terjauh dengan [[Pergeseran merah|z]]=7.54<ref name="NAT-20171206" /> |- | [[UGC 12591]] || '''{{val|6.18|2.61|e=8}}'''<ref>{{cite journal | doi=10.1093/mnras/stac2683 | title=Hubble Space Telescope Captures UGC 12591: Bulge/Disc properties, star formation and 'missing baryons' census in a very massive and fast-spinning hybrid galaxy | year=2022 | last1=Ray | first1=Shankar | last2=Bagchi | first2=Joydeep | last3=Dhiwar | first3=Suraj | last4=Pandge | first4=M. B. | last5=Mirakhor | first5=Mohammad | last6=Walker | first6=Stephen A. | last7=Mukherjee | first7=Dipanjan | journal=Monthly Notices of the Royal Astronomical Society | volume=517 | issue=1 | pages=99–117 | doi-access=free | bibcode=2022MNRAS.517...99R | arxiv=2203.02885 }}</ref> || |- | [[Messier 49]] || '''{{val|5.6e8}}'''<ref name=apj555_1_L21>{{cite journal | last1=Loewenstein | first1=Michael | last2=Mushotzky | first2=Richard F. | last3=Angelini | first3=Lorella | last4=Arnaud | first4=Keith A. | last5=Quataert | first5=Eliot | title=Chandra Limits on X-Ray Emission Associated with the Supermassive Black Holes in Three Giant Elliptical Galaxies | journal=The Astrophysical Journal | volume=555 | issue=1 | pages=L21–L24 |date=July 2001 | doi=10.1086/323157 | bibcode=2001ApJ...555L..21L |arxiv = astro-ph/0106326 | s2cid=14873290 | url=https://zenodo.org/record/1235686 }}</ref> || |- | [[NGC 1399]] || '''{{val|5e8}}'''<ref name="Gebhardt2007">{{Cite journal | last1 = GEBHARDT | first1 = K. | last2 = LAUER | first2 = T. R. | last3 = PINKNEY | first3 = J. | last4 = BENDER | first4 = R. | last5 = RICHSTONE | first5 = D. | last6 = ALLER | first6 = M. | last7 = BOWER | first7 = G. | last8 = DRESSLER | first8 = A. | date = December 2007 | journal = The Astrophysical Journal | volume = 671 | issue = 2 | pages = 1321–1328 | title = The Black Hole Mass and Extreme Orbital Structure in NGC 1399 | url = https://archive.org/details/sim_astrophysical-journal_2007-12-20_671_2/page/1320 |arxiv = 0709.0585 |bibcode = 2007ApJ...671.1321G |doi = 10.1086/522938 | s2cid = 12042010 }}</ref> || Central galaxy of the [[Fornax Cluster]] |- | [[PG 0804+761]] || '''{{val|6.93|0.83|e=8}}'''<ref name= 1A /><br />'''{{val|190550000}}'''<ref name=2A /> || |- | [[PG 1617+175]] || '''{{val|5.94|1.38|e=8}}'''<ref name= 1A /><br />'''{{val|275420000}}'''<ref name=2A /> || |- | [[PG 1700+518]] || '''{{val|7.81|+1.82|-1.65|e=8}}'''<ref name= 1A /><br />'''{{val|60260000}}'''<ref name=2A /> || |- | [[NGC 4261]] || '''{{val|4e8}}'''<ref name="STScI-1997-01">{{cite web |date=1997-01-13 |title=Massive Black Holes Dwell in Most Galaxies, According to Hubble Census |publisher=Hubblesite STScI-1997-01 |url=http://hubblesite.org/newscenter/archive/releases/1997/01/text/ |access-date=2010-05-02}}</ref> || Notable for its {{val|88000}} light-year long [[Polar jet#Relativistic jet|relativistic jet]].<ref name="astro162">{{cite web |title=The Giant Elliptical Galaxy NGC 4261 |publisher=Astronomy 162 (Dept. Physics & Astronomy University of Tennessee) |url=http://csep10.phys.utk.edu/astr162/lect/active/ngc4261.html |access-date=2010-05-02}}</ref> |- | [[PG 1307+085]] || '''{{val|4.4|1.23|e=8}}'''<ref name= 1A /><br />'''281 840 000'''<ref name=2A /> || |- | [[SAGE0536AGN]] || '''{{val|3.5|0.8|e=8}}'''<ref name="van_loon2015">{{cite journal | last1 = van | first1 = Loon J. T. | last2 = Sansom | first2 = A. E. | title = An evolutionary missing link? A modest-mass early-type galaxy hosting an oversized nuclear black hole | year = 2015 | journal = [[Monthly Notices of the Royal Astronomical Society]] | volume = 453 | issue = 3 | pages = 2341–2348 | doi = 10.1093/mnras/stv1787 | arxiv = 1508.00698 | bibcode = 2015MNRAS.453.2341V | s2cid = 56459588 }}</ref><ref name=SAGE0536AGN>{{Cite web|url=https://phys.org/news/2015-09-black-hole-size.html|title=Black hole is 30 times expected size|website=phys.org}}</ref> || Constitutes 1.4% of the mass of its host galaxy |- | [[NGC 1275]] || '''{{val|3.4e8}}'''<ref name=Wilman2005>{{cite journal | volume = 359 | issue = 2 | pages = 755–764 | last1 = Wilman | first1 = R. J. | last2 = Edge | first2 = A. C. | last3 = Johnstone | first3 = R. M. | title = The nature of the molecular gas system in the core of NGC 1275 | journal = Monthly Notices of the Royal Astronomical Society | date = 2005 |bibcode = 2005MNRAS.359..755W | doi = 10.1111/j.1365-2966.2005.08956.x |arxiv = astro-ph/0502537 | s2cid = 18190288 }}</ref><ref>{{cite journal | volume = 359 | issue = 2 | pages = 755–764 | last1 = Wilman | first1 = R. J. | last2 = Edge | first2 = A. C. | last3 = Johnstone | first3 = R. M. | title = The nature of the molecular gas system in the core of NGC 1275 | journal = Monthly Notices of the Royal Astronomical Society | date = 2005 |bibcode = 2005MNRAS.359..755W | doi = 10.1111/j.1365-2966.2005.08956.x|arxiv = astro-ph/0502537 | s2cid = 18190288 }}</ref> || Central galaxy of the [[Perseus Cluster]] |- | [[3C 390.3]] || '''{{val|2.87|0.64|e=8}}'''<ref name= 1A /><br />'''{{val|338840000}}'''<ref name=2A /> || |- | [[II Zwicky 136]] || '''{{val|4.57|0.55|e=8}}'''<ref name= 1A /><br />'''{{val|144540000}}'''<ref name=2A /> || |- | [[PG 0052+251]] || '''{{val|3.69|0.76|e=8}}'''<ref name= 1A /><br />'''{{val|218780000}}'''<ref name=2A /> || |- | [[Messier 59]] || '''{{val|2.7e8}}'''<ref name="Wrobel2008">{{cite journal| author=Wrobel, J. M.| author2=Terashima, Y.| author3=Ho, L. C. | date=2008 | title=Outflow-dominated Emission from the Quiescent Massive Black Holes in NGC 4621 and NGC 4697 | url=https://archive.org/details/sim_astrophysical-journal_2008-03-10_675_2/page/1040| journal=The Astrophysical Journal | volume=675 | issue= 2 | pages=1041–1047 | bibcode=2008ApJ...675.1041W | doi=10.1086/527542|arxiv = 0712.1308 | s2cid=119208491}}</ref> || Lubang hitam tersebut memiliki sebuah rotasi retrograd.<ref name="Wernli2001">{{cite journal | author=Wernli, F. | author2=Emsellem, E. | author3=Copin, Y. | year=2002 | title=A 60 pc counter-rotating core in NGC 4621 | journal=Astronomy & Astrophysics | volume=396 | pages=73–81 | bibcode=2002A&A...396...73W | doi=10.1051/0004-6361:20021333|arxiv = astro-ph/0209361 | s2cid=18545003 }}</ref> |- | [[PG 1411+442]] || '''{{val|4.43|1.46|e=8}}'''<ref name= 1A /><br />'''{{val|79430000}}'''<ref name=2A /> || |- | [[Markarian 876]] || '''{{val|2.79|1.29|e=8}}'''<ref name= 1A /><br />'''{{val|240000000}}'''<ref name=2A /> || |- | [[Galaksi Andromeda]]|| '''{{val|2.3e8}}''' || Galaksi besar terdekat ke [[Bima Sakti]] |- | [[PG 0953+414]] || '''{{val|2.76|0.59|e=8}}'''<ref name= 1A /><br />'''{{val|182000000}}'''<ref name=2A /> || |- | [[PG 0026+129]] || '''{{val|3.93|0.96|e=8}}'''<ref name= 1A /><br />'''{{val|53700000}}'''<ref name=2A /> || |- | [[Fairall 9]] || '''{{val|2.55|0.56|e=8}}'''<ref name= 1A /><br />'''{{val|79430000}}'''<ref name=2A /> || |- | [[Markarian 1095]] || '''{{val|1.5|0.19|e=8}}'''<ref name= 1A /><br />'''{{val|182000000}}'''<ref name=2A /> || |- | [[Messier 105]] || '''{{val|1.4e8}}–{{val|2e8}}'''<ref name="thilker2009">{{cite journal | author=Thilker, David A. | author2=Donovan, Jennifer | author3=Schiminovich, David | author4=Bianchi, Luciana | author5=Boissier, Samuel | author6=Gil de Paz | author7= Armando | author8=Madore, Barry F. | author9=Martin, D. Christopher | author10=Seibert, Mark | date=2009 | title=Massive star formation within the Leo 'primordial' ring | url=https://archive.org/details/sim_nature-uk_2009-02-19_457_7232/page/990 | journal=Nature | volume=457 | issue=7232 | pages=990–993 | bibcode=2009Natur.457..990T | doi=10.1038/nature07780 | pmid=19225520| s2cid=4424307 }}</ref>|| |- | [[Markarian 509]] || '''{{val|1.43|0.12|e=8}}'''<ref name= 1A /><br />'''{{val|57550000}}'''<ref name=2A /> || |- | Sekunder dari OJ 287 || '''{{val|1e8}}'''<ref name="frostbite" /> || The smaller black hole orbiting OJ 287 primary (see above). |- | [[RX J1242-11|RX J124236.9-111935]] || '''{{val|1e8}}'''<ref name="kom" /> || Observed by the [[Chandra X-ray Observatory]] to be tidally disrupting a star.<ref name="kom">{{cite journal | last1 = Komossa | first1 = S. | last2 = Halpern | first2 = J. | last3 = Schartel | first3 = N. | last4 = Hasinger | first4 = G. |last5 = Santos-Lleo | first5 = M. | last6 = Predehl | first6 = P. | title = A Huge Drop in the X-Ray Luminosity of the Nonactive Galaxy RX J1242.6-1119A, and the First Postflare Spectrum: Testing the Tidal Disruption Scenario | journal = The Astrophysical Journal Letters | volume = 603 | issue = 1 | pages = L17–L20 | date = May 2004 |arxiv = astro-ph/0402468 |bibcode = 2004ApJ...603L..17K |doi = 10.1086/382046 | s2cid = 53724998 }}</ref><ref>NASA: [http://www.nasa.gov/home/hqnews/2004/feb/HQ_04061_black_hole.html "Giant Black Hole Rips Apart Unlucky Star"] {{Webarchive|url=https://web.archive.org/web/20160304072637/http://www.nasa.gov/home/hqnews/2004/feb/HQ_04061_black_hole.html |date=2016-03-04 }}</ref> |- | [[Messier 85]] || '''{{val|1e8}}'''<ref name="KormendyBender2009">{{cite journal | author=Kormendy, John | author2=Bender, Ralf | date=2009 | title=Correlations between Supermassive Black Holes, Velocity Dispersions, and Mass Deficits in Elliptical Galaxies with Cores | journal=[[Astrophysical Journal Letters]] | volume=691 | issue=2 | pages=L142–L146 | bibcode=2009ApJ...691L.142K | doi=10.1088/0004-637X/691/2/L142|arxiv = 0901.3778 | s2cid=18919128 }}</ref>|| |- | [[NGC 5548]] || '''{{val|6.71|0.26|e=7}}'''<ref name= 1A /><br />'''{{val|123000000}}'''<ref name=2A /> || |- | [[PG 1211+143]] || '''{{val|1.46|0.44|e=8}}'''<ref name= 1A /><br />'''{{val|40740000}}'''<ref name=2A /> || |- | [[Messier 88]] || '''{{val|8e7}}'''<ref>{{cite journal | author=Merloni, Andrea | author2=Heinz, Sebastian | author3=di Matteo, Tiziana | date=2003 | title=A Fundamental Plane of black hole activity | journal=[[Monthly Notices of the Royal Astronomical Society]] | volume=345 | issue=4 | pages=1057–1076 | doi=10.1046/j.1365-2966.2003.07017.x |arxiv = astro-ph/0305261 |bibcode = 2003MNRAS.345.1057M | s2cid=14310323 }}</ref> || |- | [[Messier 81]] (''Galaksi Bode'') || '''{{val|7e7}}'''<ref name="devereuxetal2003">{{cite journal | author=N. Devereux | author2= H. Ford | author3=Z. Tsvetanov | author4=J. Jocoby | name-list-style=amp | date=2003 | title=STIS Spectroscopy of the Central 10 Parsecs of M81: Evidence for a Massive Black Hole | url=https://archive.org/details/sim_astronomical-journal_2003-03_125_3/page/1226 | journal=[[Astronomical Journal]] | volume=125 | issue=3 | pages=1226–1235 | bibcode=2003AJ....125.1226D | doi=10.1086/367595| doi-access=free }}</ref> || |- | [[Markarian 771]] || '''{{val|7.32|3.52|e=7}}'''<ref name= 1A /><br />'''{{val|7.586e7}}'''<ref name=2A /> || |- | [[Messier 58]] || '''{{val|7e7}}'''<ref name="Merloni2003">{{cite journal | author=Merloni, Andrea | author2=Heinz, Sebastian | author3=di Matteo, Tiziana | date=2003 | title=A Fundamental Plane of black hole activity | journal=Monthly Notices of the Royal Astronomical Society | volume=345 | issue=4 | pages=1057–1076 | bibcode=2003MNRAS.345.1057M | doi=10.1046/j.1365-2966.2003.07017.x|arxiv = astro-ph/0305261 | s2cid=14310323 }}</ref> || |- | [[PG 0844+349]] || '''{{val|9.24|3.81|e=7}}'''<ref name= 1A /><br />'''{{val|2.138e7}}'''<ref name=2A /> || |- | [[Centaurus A]] || '''{{val|5.5e7}}'''<ref>{{cite web|title=Radio Telescopes Capture Best-Ever Snapshot of Black Hole Jets|url=http://www.nasa.gov/topics/universe/features/radio-particle-jets.html|publisher=NASA|access-date=2012-10-02}}</ref> || Also notable for its million light-year long [[Polar jet#Relativistic jet|relativistic jet]].<ref>{{Cite APOD|title=Centaurus Radio Jets Rising|access-date=2011-04-16|date=2011-04-13}}</ref> |- | [[Markarian 79]] || '''{{val|5.24|1.44|e=7}}'''<ref name= 1A /><br />'''{{val|5.25e7}}'''<ref name=2A /> || |- | [[Messier 96]] || '''{{val|48000000}}'''<ref name=mnras403_2_646>{{cite journal | last1=Nowak | first1=N. | last2=Thomas | first2=J. | last3=Erwin | first3=P. | last4=Saglia | first4=R. P. | last5=Bender | first5=R. | last6=Davies | first6=R. I. | title=Do black hole masses scale with classical bulge luminosities only? The case of the two composite pseudo-bulge galaxies NGC 3368 and NGC 3489. | journal=[[Monthly Notices of the Royal Astronomical Society]] | volume=403 | issue=2 | pages=646–672 |date=April 2010 | doi=10.1111/j.1365-2966.2009.16167.x | bibcode=2010MNRAS.403..646N |arxiv = 0912.2511 | s2cid=59580555 }}</ref> || Estimates can be as low as 1.5 million solar masses |- | [[Markarian 817]] || '''{{val|4.94|0.77|e=7}}'''<ref name= 1A /><br />'''{{val|4.365e7}}'''<ref name=2A />|| |- | [[NGC 3227]] || '''{{val|4.22|2.14|e=7}}'''<ref name=1A /><br />'''{{val|3.89e7}}'''<ref name=2A />|| |- | [[NGC 4151]] primary || '''{{val|4e7}}'''<ref>{{cite web|title=NGC 4151: An active black hole in the "Eye of Sauron"|url=http://www.astronomy.com/News-Observing/News/2011/03/NGC%204151%20active%20black%20hole%20in%20the%20Eye%20of%20Sauron.aspx|publisher=Astronomy magazine|access-date=2011-03-14|date=2011-03-11|archive-date=2019-03-29|archive-url=https://web.archive.org/web/20190329112815/http://www.astronomy.com/News-Observing/News/2011/03/NGC|url-status=dead}}</ref><ref name="ReferenceA">{{cite journal| arxiv=1209.4524 | author1=Bon | author2=Jovanović | author3=Marziani | author4=Shapovalova | author5=Bon | author6=Borka Jovanović | author7=Borka | author8=Sulentic | author9=Popović | title=The First Spectroscopically Resolved Sub-parsec Orbit of a Supermassive Binary Black Hole | journal=The Astrophysical Journal | volume=759 | issue=2 | pages=118–125 | date=2012| doi=10.1088/0004-637X/759/2/118 |bibcode = 2012ApJ...759..118B | s2cid=119257514 }}</ref> || |- | [[3C 120]] || '''{{val|5.55|+3.14|-2.25|e=7}}'''<ref name=1A /><br />'''{{val|2.29e7}}'''<ref name=2A /> || |- | [[Markarian 279]] || '''{{val|3.49|0.92|e=7}}'''<ref name=1A /><br />'''{{val|4.17e7}}'''<ref name=2A /> || |- | [[NGC 3516]] || '''{{val|4.27|1.46|e=7}}'''<ref name=1A /><br />'''{{val|2.3e7}}'''<ref name=2A /> || |- | [[NGC 863]] || '''{{val|4.75|0.74|e=7}}'''<ref name=1A /><br />'''{{val|1.77e7}}'''<ref name=2A /> || |- | [[Messier 82]] (''Cigar Galaxy'') || '''{{val|3e7}}'''<ref>{{cite journal | author=Gaffney, N. I. | author2=Lester, D. F. | author3=Telesco, C. M. | name-list-style=amp | date = 1993 | title = The stellar velocity dispersion in the nucleus of M82 | journal=[[Astrophysical Journal Letters]] | volume = 407 | pages = L57–L60 | doi = 10.1086/186805 | bibcode = 1993ApJ...407L..57G}}</ref> || Prototype [[starburst galaxy]].<ref name="Barkeretal2008">{{cite journal | last1 = Barker | first1 = S. | last2 = de Grijs | first2 = R. | last3 = Cerviño | first3 = M. | date = 2008 | title = Star cluster versus field star formation in the nucleus of the prototype starburst galaxy M 82 | journal=[[Astronomy and Astrophysics]] | volume = 484 | issue = 3 | pages = 711–720 | bibcode = 2008A&A...484..711B | doi = 10.1051/0004-6361:200809653|arxiv = 0804.1913 | s2cid = 18885080 }}</ref> |- | [[Messier 108]] || '''{{val|2.4e7}}'''<ref>{{cite journal | author=Satyapal, S. |display-authors=etal | date=2008 | title=Spitzer Uncovers Active Galactic Nuclei Missed by Optical Surveys in Seven Late-Type Galaxies | url=https://archive.org/details/sim_astrophysical-journal_2008-04-20_677_2/page/926 | journal=[[Astrophysical Journal]] | volume=677 | issue=2 | pages=926–942 | doi=10.1086/529014 | bibcode=2008ApJ...677..926S |arxiv = 0801.2759 |last2=Vega |first2=D. |last3=Dudik |first3=R. P. |last4=Abel |first4=N. P. |last5=Heckman |first5=T. |s2cid=16050838 }}</ref> || |- | [[M60-UCD1]] || '''{{val|2e7}}'''<ref name="Strader2013">{{cite journal | author=Strader, J. | display-authors=etal | date=2013 | title=The Densest Galaxy | journal=The Astrophysical Journal | volume=775 | issue=1 | pages=L6 | bibcode=2013ApJ...775L...6S | arxiv=1307.7707 | doi=10.1088/2041-8205/775/1/L6| s2cid=52207639 }}</ref> || Constitutes 15% of the mass of its host galaxy. |- | [[NGC 3783]] || '''{{val|2.98|0.54|e=7}}'''<ref name=1A /><br />'''{{val|9300000}}'''<ref name=2A /> || |- | [[Markarian 110]] || '''{{val|2.51|0.61|e=7}}'''<ref name=1A /><br />'''{{val|5620000}}'''<ref name=2A /> || |- | [[Markarian 335]] || '''{{val|1.42|0.37|e=7}}'''<ref name=1A /><br />'''{{val|6310000}}'''<ref name=2A /> || |- | NGC 4151 secondary || '''{{val|10000000}}'''<ref name="ReferenceA" /> || |- | [[NGC 7469]] || '''{{val|12.2|1.4|e=6}}'''<ref name=1A /><br />'''{{val|6460000}}'''<ref name=2A /> || |- | [[IC 4329]] A || '''{{val|9.90|+17.88|-11.88|e=6}}'''<ref name=1A /><br />'''{{val|5010000}}'''<ref name=2A /> || |- | [[NGC 4593]] || '''{{val|5.36|+9.37|-6.95|e=6}}'''<ref name=1A /><br />'''{{val|8130000}}'''<ref name=2A /> || |- | [[Messier 61]] || '''{{val|5e6}}'''<ref name="Pastorini2007">{{cite journal | last1=Pastorini |first1=G. |last2=Marconi |first2=A. |last3=Capetti |first3=A. |last4=Axon |first4=D. J. |last5=Alonso-Herrero |first5=A. |last6=Atkinson |first6=J. |author7-link=Daniel Batcheldor |last7=Batcheldor, D.|last8=Carollo |first8=C. M. | authorlink8= C. Marcella Carollo| last9=Collett |first9=J. |last10=Dressel |first10=L. |last11=Hughes |first11=M. A. |last12=Macchetto |first12=D. |last13=Maciejewski |first13=W. |last14=Sparks |first14=W. |last15=van der Marel |first15=R. | date=2007 | title=Supermassive black holes in the Sbc spiral galaxies NGC 3310, NGC 4303 and NGC 4258 | journal=[[Astronomy and Astrophysics]] | volume=469 |issue=2 |pages=405–423 | doi=10.1051/0004-6361:20066784 | bibcode=2007A&A...469..405P | arxiv=astro-ph/0703149 |s2cid=849621 }}</ref> || |- | [[Messier 32]] || '''{{val|1.5e6}}–{{val|5e6}}'''<ref>{{Cite journal | last1 = Valluri | first1 = M. | last2 = Merritt | first2 = D. |author2-link=David Merritt | last3 = Emsellem | first3 = E. | title = Difficulties with Recovering the Masses of Supermassive Black Holes from Stellar Kinematical Data | url = https://archive.org/details/sim_astrophysical-journal_2004-02-10_602_1/page/66 | journal = [[Astrophysical Journal]] | volume = 602 | issue = 1| pages = 66–92 | date = 2004 | bibcode = 2004ApJ...602...66V | doi = 10.1086/380896 |arxiv = astro-ph/0210379 | s2cid = 16899097 }}</ref> || Sebuah galaksi satelit katai di [[Galaksi Andromeda]]. |- | [[Sagittarius A*]] || '''{{val|4.3e6}}'''<ref name="Ghez08">{{cite journal | author = Ghez, A. M. |display-authors=etal | title = Measuring Distance and Properties of the Milky Way's Central Supermassive Black Hole with Stellar Orbits | url = https://archive.org/details/sim_astrophysical-journal_2008-12-20_689_2/page/1044 | journal = Astrophysical Journal | date = 2008 | volume = 689 | issue = 2 | pages = 1044–1062 | doi = 10.1086/592738 | bibcode = 2008ApJ...689.1044G | arxiv=0808.2870|last2=Salim |last3=Weinberg |last4=Lu |last5=Do |last6=Dunn |last7=Matthews |last8=Morris |last9=Yelda |last10=Becklin |last11=Kremenek |last12=Milosavljevic |last13=Naiman |s2cid=18335611 }}</ref> || Lubang hitam di pusat [[Bima Sakti]]. |- | [[NGC 4395]] || '''{{val|3.599e5}}'''<ref>{{Cite journal |last1=Peterson |first1=Bradley M. |last2=Bentz |first2=Misty C. |last3=Desroches |first3=Louis-Benoit |last4=Filippenko |first4=Alexei V. |last5=Ho |first5=Luis C. |last6=Kaspi |first6=Shai |last7=Laor |first7=Ari |last8=Maoz |first8=Dan |last9=Moran |first9=Edward C. |last10=Pogge |first10=Richard W. |last11=Quillen |first11=Alice C. |date=2005-10-20 |title=Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC 4395. I. A Reverberation-Based Measurement of the Black Hole Mass |url=https://archive.org/details/sim_astrophysical-journal_2005-10-20_632_2/page/799 |journal=The Astrophysical Journal |volume=632 |issue=2 |pages=799–808 |doi=10.1086/444494 |arxiv=astro-ph/0506665 |bibcode=2005ApJ...632..799P |hdl=1811/48314 |s2cid=13886279 |issn=0004-637X}}</ref> <br/>'''{{val|1.7|0.3|e=4}}'''<ref>{{Cite journal |last1=Cho |first1=Hojin |last2=Woo |first2=Jong-Hak |last3=Treu |first3=Tommaso |last4=Williams |first4=Peter R. |last5=Armen |first5=Stephen F. |last6=Barth |first6=Aaron J. |last7=Bennert |first7=Vardha N. |last8=Cho |first8=Wanjin |last9=Filippenko |first9=Alexei V. |last10=Gallo |first10=Elena |last11=Geum |first11=Jaehyuk |last12=González-Buitrago |first12=Diego |last13=Gültekin |first13=Kayhan |last14=Hodges-Kluck |first14=Edmund |last15=Horst |first15=John C. |date=2021-11-01 |title=Hα Reverberation Mapping of the Intermediate-mass Active Galactic Nucleus in NGC 4395 |journal=The Astrophysical Journal |language=en |volume=921 |issue=2 |pages=98 |arxiv=2108.07756 |bibcode=2021ApJ...921...98C |doi=10.3847/1538-4357/ac1e92 |doi-access=free |issn=0004-637X }}</ref> <br/>'''{{val|1e4}}'''<ref>{{Cite journal |last=Woo |first=Jong-Hak |display-authors=etal |date=10 July 2019 |title=A 10,000-solar-mass black hole in the nucleus of a bulgeless dwarf galaxy |journal=[[Nature Astronomy]] |volume=3 |issue=8 |pages=755–759 |arxiv=1905.00145 |bibcode=2019NatAs...3..755W |doi=10.1038/s41550-019-0790-3 |issn=2397-3366 |s2cid=189762554}}</ref> <br/> '''{{val|8|4|e=3}}'''<ref name=Huapeng2024>{{Cite journal |last1=Huapeng |first1=Gu |last2=Xue-Bing |first2=Wu |last3=Yuhan |first3=Wen |last4=Qinchun |first4=Ma |last5=Hengxiao |first5=Guo |date=June 2024 |title=H α reverberation mapping from broad-band photometry of dwarf type 1 Seyfert galaxy NGC 4395 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=530 |issue=4 |page=3578 |arxiv=2404.11495 |bibcode=2024MNRAS.530.3578G |doi=10.1093/mnras/stae1063 |doi-access=free |issn=0035-8711 }}</ref>||Mungkin merupakan [[lubang hitam supermasif]] terkecil. Mungkin juga disebut "[[lubang hitam bermassa menengah]]".<ref name=Huapeng2024/> |} == Cingak malih == {{Portal|Astronomi}} * [[Lis struktur kosmik pinih ageng]] * [[Lis galaksi pinih ageng]] * [[Batasan Tolman–Oppenheimer–Volkoff#Lis blungbang selem pinih nenten ageng|Lis blungbang selem pinih nenten ageng]] * [[Lis eksoplanet pinih ageng]] == Pustaka == {{Reflist|30em}} {{Blungbang selem}} {{portal bar|Astronomi|Fisika|Antariksa|Bintang}} [[Kategori:Lubang hitam supermasif|*]] [[Kategori:Lis indik astronomi]] 4speivtys1n0s4wcomtajpsvrkmh1nn