数据大部分来自维基条目:list of most masive   black holes    部分来自于相关论文

质量≤100亿M⊙的黑洞选择部分收录，天体简介内容使用原文

太阳质量= 1M⊙(1.89*10³ºkg)

银河系质量≈5*10¹¹M⊙

地球质量≈0.000003M⊙

                                                                                   

Phoenix A

质量:1*10¹¹M⊙

简介:Estimated using a calorimetric model on the adiabatic behavior of core regrowth and an assumed core-Sérsic model of n=4. It is consistent with evolutionary modelling of gas accretion and the dynamics and density profiles of the galaxy. Mass has not been measured directly

4C +74.13

质量:5.13(+9.66/-3.35)*10¹ºM⊙

简介:Produced a colossal AGN outburst after accreting 600 million M☉ worth of material.

Estimated using the break radius of 0.5 kpc core of the central galaxy. Previous indirect assumptions about the efficiencies of gas accretion and jet power yield a lower limit of 1 billion M☉.

现宇宙演化阶段黑洞理论质量上限:5×10¹ºM⊙

TON 618

质量:4.07*10¹ºM⊙

简介:Estimated from quasar Hβ emission line correlation.

Holmberg 15A

质量:(4.0±0.8)*10¹ºM⊙

简介:Mass specified obtained through orbit-based, axisymmetric Schwarzschild models. Earlier estimates range from ~310 billion M☉ down to 3 billion M☉, all relying on empirical scaling relations and are thus obtained from extrapolation and not from kinematical measurement.

IC 1101

质量:(4-10)*10¹ºM⊙

简介:Estimated from properties of the host galaxy; mass has not been measured directly.

S5 0014+81

质量:4*10¹ºM⊙

简介:A 2010 paper suggested that a funnel collimates the radiation around the jet axis, creating an optical illusion of very high brightness, and thus a possible overestimation of the black hole mass.

SMSS J215728.21-360215.1

质量:(3.4±0.6)*10¹ºM⊙

SDSS J102325.31+514251.0

质量:(3.31±0.61)*10¹ºM⊙

简介:Estimated from quasar MgII emission line correlation.

H1821+643

质量:3*10¹ºM⊙

简介:Value obtained as an indirect estimate using a model of minimum Eddington luminosity required to account for the Compton cooling of the surrounding cluster.

NGC 6166

质量:3×10¹ºM⊙

简介:Central galaxy of Abell 2199; notable for its hundred thousand light year long relativistic jet.

APM 08279+5255

质量:2.3×10¹ºM⊙或(1.02±0.15)×10¹ºM⊙

简介:Based on velocity width of CO line from orbiting molecular gas, and reverberation mapping using SiIV and CIV emission lines.

NGC 4889

质量:(2.1±1.6)×10¹ºM⊙

简介:Best fit: the estimate ranges from 6 billion to 37 billion M☉.

Central black hole of Phoenix Cluster

质量:2×10¹ºM⊙

简介:This black hole is continuously growing at the rate of ~60 M☉ per year.

SDSS J074521.78+734336.1

质量:(1.95±0.05)×10¹ºM⊙

简介:Estimated from quasar MgII emission line correlation.

OJ 287

质量:1.8×10¹ºM⊙

简介:OJ 287(SMBH) is aextremely large black hole,A smaller 100 million M☉ 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.

NGC 1600

质量:(1.7±0.15)×10¹ºM⊙

简介:Unprecedentedly massive in relation of its location: an elliptical galaxy host in a sparse environment.

SDSS J08019.69+373047.3

质量:(1.51±0.31)×10¹ºM⊙

简介:Estimated from quasar MgII emission line correlation.

SDSS J115954.33+201921.1

质量:(1.41±0.10)×10¹ºM⊙

简介:Estimated from quasar MgII emission line correlation.

SDSS J075303.34+423130.8

质量:(1.38±0.03)×10¹ºM⊙

简介:Estimated from quasar Hβ emission line correlation.

SDSS  J080430.56+542041.1

质量:(1.35±0.22)×10¹ºM⊙

简介:Estimated from quasar MgII emission line correlation.

Abell 1201 BCG

质量:(1.3±0.6)×10¹ºM⊙

简介:Estimated from the strong gravitational lensing of a background galaxy behind the BCG. Beware of ambiguity between the BH mass determination and the galaxy cluster's dark matter profile.

SDSS J0100+2802

质量:(1.24±0.19)×10¹ºM⊙

简介:Estimated from quasar MgII emission line correlation. This object grew early in cosmic history (redshift 6.30).

SDSS J081855.77+095848.0

质量:(1.20±0.06)×10¹ºM⊙

简介:Estimated from quasar MgII emission line correlation.

NGC 1270 

质量:1.2×10¹ºM⊙

简介:Elliptical galaxy located in the Perseus Cluster. Also is a low-luminosity AGN (LLAGN).

SDSS J082535.19+512706.3

质量:(1.12±0.20)×10¹ºM⊙

简介:Estimated from quasar Hβ emission line.

SDSS J013127.34-032100.1

质量:(1.1±0.2)×10¹ºM⊙

简介:Estimated from accretion disk spectrum modelling.

PSO J334.2028+01.4075

 质量:10¹ºM⊙

简介: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.

RX J1532.9+3021

质量:10¹ºM⊙

QSO B2126-158

质量:10¹ºM⊙

NGC 1281

质量:10¹ºM⊙

简介:Compact elliptical galaxy in the Perseus Cluster. Mass estimates range from 10 billion M☉ down to <5 billion M☉

质量≤100亿M⊙的部分黑洞

?.SDSS J140821.67+025733.2

质量:8 000 000 000M⊙

?.M87

质量:(7.2±3.6)×1 000 000 000M⊙

?.Hercules A (3C 348)

质量:4 000 000 000M⊙

?.NGC 6166

质量:1 000 000 000M⊙

?.人马座A*

质量:4 000 000M⊙

                                                                                   

维基列表未收录的特大质量黑洞

QSO J084538.66+342043.6

质量:1.64*10¹ºM⊙

来源:https://doi.org/10.1111/j.1365-2966.2010.18099.x

PG 0050+124

质量:≧10¹ºM⊙

来源:

NEAR-INFRARED ADAPTIVE OPTICS IMAGING OF QSO HOST GALAXIES

IRAS F

质量:10¹ºM⊙

来源:

CATALOG OF SUPERMASSIVE BLACK HOLES FOR INTERFEROMETRIC OBSERVATIONS

                                                                                   

更新记录:

创建日期:2021.4.2

更新日期:2021.4.8(NGC6166简介变动)

更新日期:2021.4.11(SDSS J073739.96+384413.2，SDSS J132624.76+131727.4，SDSS J221511.93-004550.0，SDSS J014036.47+000335.8信息删除 )

更新日期:2021.4.14(OJ 287信息补充)

更新日期:2021.4.15(RBS 2043信息补充)

更新日期:2021.4.18(H1821+643信息修改)

更新日期:2021.6.8(添加IRIS-F)

更新日期:2022.10.18(删除Central black hole of Phoenix Cluster.RBS 2043.增加Phoenix,

4C +74.13)

更新日期:2023.1.22(TON618数据下调)