Paper Citation Record · LEDGER

Uncertainties in the supermassive black hole abundance and implications for the GW background

As of 8 August 2026, this Paper Citation Record lists 73 of 73 outbound references and 3 inbound Pith citation observations for arXiv:2509.08041.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2509.08041 v1

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Pith citing papers itemized under the disclosed page cap.

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A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

73 of 73 outbound references displayed

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arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation a36956e7-2808-4abb-acea-f5d692540e87 · outbound

This paper cites an unresolved cited work.

Uncertainties in the supermassive black hole abundance and implications for the GW background Unresolved cited work

Reference 1

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Observation 486726c5-d2db-46a7-bb6f-8b21c23661de · outbound

This paper cites sphere of influence.

Uncertainties in the supermassive black hole abundance and implications for the GW background sphere of influence

Reference 2

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Observation 05fa79f0-2f85-46e8-b24a-b459718d3422 · outbound

This paper cites an unresolved cited work.

Uncertainties in the supermassive black hole abundance and implications for the GW background Unresolved cited work

Reference 3

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Observation 44be112a-373c-4e84-85f1-3560e68974f8 · outbound

This paper cites an unresolved cited work.

Uncertainties in the supermassive black hole abundance and implications for the GW background Unresolved cited work

Reference 4

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Observation 5dfd24bc-f98b-4eae-947e-f761a1c776a7 · outbound

This paper cites When the velocity dispersion is used, the fundamental plane catalog is also resampled with replacement.

Uncertainties in the supermassive black hole abundance and implications for the GW background When the velocity dispersion is used, the fundamental plane catalog is also resampled with replacement

Reference 5

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Observation f08e64ba-1ce0-412c-b992-aefc312cc9a0 · outbound

This paper cites Since the full 6dFGS does not have velocity dispersion, if that is used as the mass proxy, we first fit the relation betweenX vir andσin the FP sample.

Uncertainties in the supermassive black hole abundance and implications for the GW background Since the full 6dFGS does not have velocity dispersion, if that is used as the mass proxy, we first fit the relation betweenX vir andσin the FP sample

Reference 6

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Observation ecbd1421-a5d5-4057-9581-2ad94fda4ebf · outbound

This paper cites The Astrophysics of Nanohertz Gravitational Waves.

Uncertainties in the supermassive black hole abundance and implications for the GW background The Astrophysics of Nanohertz Gravitational Waves

Reference 7

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Observation 3b3239f6-8735-4a43-8073-f8acadb6f78c · outbound

This paper cites Inward Bound—The Search For Supermassive Black Holes In Galactic Nuclei,.

Uncertainties in the supermassive black hole abundance and implications for the GW background Inward Bound—The Search For Supermassive Black Holes In Galactic Nuclei,

Reference 8

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This paper cites an unresolved cited work.

Uncertainties in the supermassive black hole abundance and implications for the GW background Unresolved cited work

Reference 9

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Observation 78f14cb8-f649-45d9-8183-c35406bc34c5 · outbound

This paper cites an unresolved cited work.

Uncertainties in the supermassive black hole abundance and implications for the GW background Unresolved cited work

Reference 10

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Observation b1f28fc5-7b66-44aa-abba-18e2e03fdb8c · outbound

This paper cites an unresolved cited work.

Uncertainties in the supermassive black hole abundance and implications for the GW background Unresolved cited work

Reference 11

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Observation 82d678cd-8a1f-4ea7-8def-137646187663 · outbound

This paper cites The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals.

Uncertainties in the supermassive black hole abundance and implications for the GW background The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

Reference 12

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Observation 5a98c605-f8ac-4fd7-9fcf-9a6a83dbefec · outbound

This paper cites Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array.

Uncertainties in the supermassive black hole abundance and implications for the GW background Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array

Reference 13

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Observation eefc7972-c3e4-4fc7-90c6-b801b21b4db2 · outbound

This paper cites Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I.

Uncertainties in the supermassive black hole abundance and implications for the GW background Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I

Reference 14

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Observation 6aea20fd-4d7f-4b8d-bc3c-867bdf78aefc · outbound

This paper cites The MeerKAT Pulsar Timing Array: The $4.5$-year data release and the noise and stochastic signals of the millisecond pulsar population.

Uncertainties in the supermassive black hole abundance and implications for the GW background The MeerKAT Pulsar Timing Array: The $4.5$-year data release and the noise and stochastic signals of the millisecond pulsar population

Reference 15

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Observation 10515c02-b895-467f-9e08-44a19e8d52e3 · outbound

This paper cites Black Hole Demography: From scaling relations to models.

Uncertainties in the supermassive black hole abundance and implications for the GW background Black Hole Demography: From scaling relations to models

Reference 16

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Observation 10dcf774-3e34-493a-a0db-16beb995f145 · outbound

This paper cites A Practical Theorem on Gravitational Wave Backgrounds.

Uncertainties in the supermassive black hole abundance and implications for the GW background A Practical Theorem on Gravitational Wave Backgrounds

Reference 17

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Observation 43b434b3-810c-4c6b-b99e-ff5489270e22 · outbound

This paper cites Supermassive Black Holes and the Evolution of Galaxies.

Uncertainties in the supermassive black hole abundance and implications for the GW background Supermassive Black Holes and the Evolution of Galaxies

Reference 18

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Observation 7a63365c-6268-4b9d-bd78-12660cc655a0 · outbound

This paper cites Massive black hole binaries in active galactic nuclei,.

Uncertainties in the supermassive black hole abundance and implications for the GW background Massive black hole binaries in active galactic nuclei,

Reference 19

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Observation e38b0e45-b104-4ff4-a1da-b291be1379d4 · outbound

This paper cites Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies.

Uncertainties in the supermassive black hole abundance and implications for the GW background Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies

Reference 20

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Observation d8a8ab37-4f2c-4eb1-91e3-d2d1bbf5270b · outbound

This paper cites Revisiting the Scaling Relations of Black Hole Masses and Host Galaxy Properties.

Uncertainties in the supermassive black hole abundance and implications for the GW background Revisiting the Scaling Relations of Black Hole Masses and Host Galaxy Properties

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:30.205307Z

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Observation 63c3aace-df98-495f-8800-1fe7f1d6ec8f · outbound

This paper cites Local Supermassive Black Holes, Relics of Active Galactic Nuclei and the X-ray Background.

Uncertainties in the supermassive black hole abundance and implications for the GW background Local Supermassive Black Holes, Relics of Active Galactic Nuclei and the X-ray Background

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:30.283191Z

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Observation c2ee4d58-1742-4527-92dc-8d205795dc1f · outbound

This paper cites The Millennium Galaxy Catalogue: The $M_{bh}$--$L_{spheroid}$ derived supermassive black hole mass function.

Uncertainties in the supermassive black hole abundance and implications for the GW background The Millennium Galaxy Catalogue: The $M_{bh}$--$L_{spheroid}$ derived supermassive black hole mass function

Reference 23

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Observation 172fc1e4-b46d-452d-b462-6c26cd611a3e · outbound

This paper cites Self-Consistent Models of the AGN and Black Hole Populations: Duty Cycles, Accretion Rates, and the Mean Radiative Efficiency.

Uncertainties in the supermassive black hole abundance and implications for the GW background Self-Consistent Models of the AGN and Black Hole Populations: Duty Cycles, Accretion Rates, and the Mean Radiative Efficiency

Reference 24

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Observation 2d6f55c2-cbfb-4ecb-b4e0-05c39b00132e · outbound

This paper cites Selection bias in dynamically measured supermassive black hole samples: its consequences and the quest for the most fundamental relation,.

Uncertainties in the supermassive black hole abundance and implications for the GW background Selection bias in dynamically measured supermassive black hole samples: its consequences and the quest for the most fundamental relation,

Reference 25

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Observation 5e037b7d-ec66-4f31-8765-9f1d3b24ccf1 · outbound

This paper cites Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass.

Uncertainties in the supermassive black hole abundance and implications for the GW background Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass

Reference 26

Resolution: verified exact; local_arxiv, observed 2026-08-04T21:30:31.877530Z

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Observation a89ef11b-00a8-48f2-ae62-4ec2839d0ac1 · outbound

This paper cites Where are NANOGrav's big black holes?.

Uncertainties in the supermassive black hole abundance and implications for the GW background Where are NANOGrav's big black holes?

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:30.799001Z

Source-reported events for the cited work

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Observation 38633f5e-c214-4ae8-928f-f70afffb8584 · outbound

This paper cites The distribution of the gravitational-wave background from supermassive black holes.

Uncertainties in the supermassive black hole abundance and implications for the GW background The distribution of the gravitational-wave background from supermassive black holes

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:30.885037Z

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Observation 1d590198-3040-41f5-80e9-703450510e1d · outbound

This paper cites Evolution of SMBHs in light of PTA measurements: implications for growth by mergers and accretion.

Uncertainties in the supermassive black hole abundance and implications for the GW background Evolution of SMBHs in light of PTA measurements: implications for growth by mergers and accretion

Reference 29

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Observation d358442f-50f9-480f-a505-75820cfc67ef · outbound

This paper cites The Need For Speed: Rapid Refitting Techniques for Bayesian Spectral Characterization of the Gravitational Wave Background Using PTAs.

Uncertainties in the supermassive black hole abundance and implications for the GW background The Need For Speed: Rapid Refitting Techniques for Bayesian Spectral Characterization of the Gravitational Wave Background Using PTAs

Reference 30

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Observation 4f2f9a7e-7180-4afe-bd23-9f633955cb8c · outbound

This paper cites The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes,.

Uncertainties in the supermassive black hole abundance and implications for the GW background The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes,

Reference 31

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Observation ed0606f8-97ac-4074-a54d-6d452a143566 · outbound

This paper cites The M-Sigma Relation Derived from Sphere of Influence Arguments.

Uncertainties in the supermassive black hole abundance and implications for the GW background The M-Sigma Relation Derived from Sphere of Influence Arguments

Reference 32

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Observation 5dbcb6c5-4f56-425c-ac8d-14870bde4a01 · outbound

This paper cites On the inconsistency between the black hole mass function inferred from M_bh-sigma and M_bh-L correlation.

Uncertainties in the supermassive black hole abundance and implications for the GW background On the inconsistency between the black hole mass function inferred from M_bh-sigma and M_bh-L correlation

Reference 33

Resolution: verified exact; local_arxiv, observed 2026-08-04T21:30:31.909044Z

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Observation 5ec4502b-ed1a-47d1-a47a-5fe017196b30 · outbound

This paper cites Selection Bias in the M-σand M-L Correlations and Its Consequences,.

Uncertainties in the supermassive black hole abundance and implications for the GW background Selection Bias in the M-σand M-L Correlations and Its Consequences,

Reference 34

Resolution: verified fuzzy; raw_fallback, observed 2026-08-04T21:30:32.160238Z

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Observation b7581dc4-4576-4392-b409-734d44cf2e7a · outbound

This paper cites Selection bias in the M_BH-sigma and M_BH-L correlations and its consequences.

Uncertainties in the supermassive black hole abundance and implications for the GW background Selection bias in the M_BH-sigma and M_BH-L correlations and its consequences

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-08-04T21:30:31.897089Z

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Observation 5f4a5a95-2081-495c-bfc6-743fc0b6b8b8 · outbound

This paper cites The 6dF Galaxy Survey: Samples, Observational Techniques and the First Data Release.

Uncertainties in the supermassive black hole abundance and implications for the GW background The 6dF Galaxy Survey: Samples, Observational Techniques and the First Data Release

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.528942Z

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This paper cites The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures.

Uncertainties in the supermassive black hole abundance and implications for the GW background The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.532231Z

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Observation e481afdc-10e4-4c6d-b93e-c15808894be1 · outbound

This paper cites [43], and is com- monly adopted in the literature.

Uncertainties in the supermassive black hole abundance and implications for the GW background [43], and is com- monly adopted in the literature

Reference 38

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Observation 8a940d68-9669-43d7-bbe4-d68f2c105f54 · outbound

This paper cites The massive end of the luminosity and stellar mass functions: Dependence on the fit to the light profile.

Uncertainties in the supermassive black hole abundance and implications for the GW background The massive end of the luminosity and stellar mass functions: Dependence on the fit to the light profile

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.501698Z

Source-reported events for the cited work

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Observation eb3d86cc-7528-4629-8722-9fe8a56de035 · outbound

This paper cites The Massive End of the Stellar Mass Function.

Uncertainties in the supermassive black hole abundance and implications for the GW background The Massive End of the Stellar Mass Function

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.504653Z

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Observation db8739b3-703e-4641-8aac-8e288b6c7b7b · outbound

This paper cites A New Census of the 0.2 < z < 3.0 Universe, Part I: The Stellar Mass Function.

Uncertainties in the supermassive black hole abundance and implications for the GW background A New Census of the 0.2 < z < 3.0 Universe, Part I: The Stellar Mass Function

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.507491Z

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Observation 038693f8-9ae5-45b8-a11c-d360c471c2a5 · outbound

This paper cites We therefore correct the magnitude and size in 2MASS in order to match the properties measured in both references and compare the 3 properties to study this effect.

Uncertainties in the supermassive black hole abundance and implications for the GW background We therefore correct the magnitude and size in 2MASS in order to match the properties measured in both references and compare the 3 properties to study this effect

Reference 42

Resolution: verified fuzzy; raw_fallback, observed 2026-08-04T21:30:32.259840Z

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Observation 643f5565-d298-419e-a5ae-80b5c1d80c0d · outbound

This paper cites Big Galaxies and Big Black Holes: The Massive Ends of the Local Stellar and Black Hole Mass Functions and the Implications for Nanohertz Gravitational Waves.

Uncertainties in the supermassive black hole abundance and implications for the GW background Big Galaxies and Big Black Holes: The Massive Ends of the Local Stellar and Black Hole Mass Functions and the Implications for Nanohertz Gravitational Waves

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.510273Z

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Observation ad763feb-987d-40ba-9f0e-f2216cbc2f51 · outbound

This paper cites Galaxy luminosities, stellar masses, sizes, velocity dispersions as a function of morphological type,.

Uncertainties in the supermassive black hole abundance and implications for the GW background Galaxy luminosities, stellar masses, sizes, velocity dispersions as a function of morphological type,

Reference 44

Resolution: verified fuzzy; raw_fallback, observed 2026-08-04T21:30:32.142308Z

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Observation a072745c-0d4b-4775-8d8b-2c7556ded895 · outbound

This paper cites The Structure of Galaxies I: Surface Photometry Techniques,.

Uncertainties in the supermassive black hole abundance and implications for the GW background The Structure of Galaxies I: Surface Photometry Techniques,

Reference 45

Resolution: verified fuzzy; raw_fallback, observed 2026-08-04T21:30:32.115190Z

Source-reported events for the cited work

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Observation 10abf949-4528-48d9-844d-a000faa881c1 · outbound

This paper cites Quashing a suspected selection bias in galaxy samples having dynamically-measured supermassive black holes.

Uncertainties in the supermassive black hole abundance and implications for the GW background Quashing a suspected selection bias in galaxy samples having dynamically-measured supermassive black holes

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-08-04T21:30:31.812182Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 6fa85135-58dc-40e4-9912-ade9280810cd · outbound

This paper cites The MASSIVE Survey - I. A Volume-Limited Integral-Field Spectroscopic Study of the Most Massive Early-Type Galaxies within 108 Mpc.

Uncertainties in the supermassive black hole abundance and implications for the GW background The MASSIVE Survey - I. A Volume-Limited Integral-Field Spectroscopic Study of the Most Massive Early-Type Galaxies within 108 Mpc

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.523535Z

Source-reported events for the cited work

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Observation 4d12c188-78ed-4a36-88b8-d29f948fe8dd · outbound

This paper cites The Two Micron All Sky Survey (2MASS),.

Uncertainties in the supermassive black hole abundance and implications for the GW background The Two Micron All Sky Survey (2MASS),

Reference 48

Resolution: verified fuzzy; raw_fallback, observed 2026-08-04T21:30:32.133934Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 7a52d4e8-9f24-4da3-989a-309d2000dfea · outbound

This paper cites Velocity Dispersion $\sigma_{\rm aper}$ Aperture Corrections as a Function of Galaxy Properties from Integral-field Stellar Kinematics of 10,000 MaNGA Galaxies.

Uncertainties in the supermassive black hole abundance and implications for the GW background Velocity Dispersion $\sigma_{\rm aper}$ Aperture Corrections as a Function of Galaxy Properties from Integral-field Stellar Kinematics of 10,000 MaNGA Galaxies

Reference 49

Resolution: verified exact; local_arxiv, observed 2026-08-04T21:30:31.695762Z

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Observation 4fdd9a30-ab76-47d9-89de-c8199f179767 · outbound

This paper cites Extracting distribution parameters from multiple uncertain observations with selection biases.

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Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.563345Z

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Observation 44c8aff8-fea5-4163-ac6d-f5df84a1855e · outbound

This paper cites The 6dF Galaxy Survey: Fundamental Plane Data.

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Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.534756Z

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Observation 2655ee9a-5187-4234-9b6f-06478358f565 · outbound

This paper cites The 6dF Galaxy Survey: The Near-Infrared Fundamental Plane of Early-Type Galaxies.

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Reference 52

Resolution: verified exact; local_arxiv, observed 2026-08-04T21:30:31.766978Z

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Observation 44c28b7d-e39d-494d-b758-1c7d7cef4b78 · outbound

This paper cites Unification of the Fundamental Plane and Super-Massive Black Holes Masses.

Uncertainties in the supermassive black hole abundance and implications for the GW background Unification of the Fundamental Plane and Super-Massive Black Holes Masses

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.539819Z

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Observation b11a91ae-42e0-4125-ac80-6698f43c6c23 · outbound

This paper cites The MASSIVE Survey. XVIII. Deep Wide-Field $K$-band Photometry and Local Scaling Relations for Massive Early-Type Galaxies.

Uncertainties in the supermassive black hole abundance and implications for the GW background The MASSIVE Survey. XVIII. Deep Wide-Field $K$-band Photometry and Local Scaling Relations for Massive Early-Type Galaxies

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.542388Z

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Observation 1047acfb-6466-460a-bf69-d36d599f47c4 · outbound

This paper cites Spectroscopy for E and S0 galaxies in nine clusters,.

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Reference 55

Resolution: verified fuzzy; raw_fallback, observed 2026-08-04T21:30:32.124563Z

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Observation b02325f1-7155-4c00-b4b6-3d47b36ef633 · outbound

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Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.547660Z

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Observation b4a73e84-0e36-4d95-836f-ea441a116796 · outbound

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Uncertainties in the supermassive black hole abundance and implications for the GW background On the hunt for ultramassive black holes in brightest cluster galaxies

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.584805Z

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Observation da5d1986-3338-4d82-b560-0975a45d8a0a · outbound

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Uncertainties in the supermassive black hole abundance and implications for the GW background The SAURON project - IV. The mass-to-light ratio, the virial mass estimator and the fundamental plane of elliptical and lenticular galaxies

Reference 58

Resolution: verified exact; local_arxiv, observed 2026-08-04T21:30:31.729051Z

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Observation 877fffe0-8a93-4e22-b92a-acab6aab6c27 · outbound

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Uncertainties in the supermassive black hole abundance and implications for the GW background Stellar kinematics across the Hubble sequence in the CALIFA survey: General properties and aperture corrections

Reference 59

Resolution: verified exact; local_arxiv, observed 2026-08-04T21:30:31.716845Z

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Observation 586d51c6-1434-41be-95be-0a908953ff67 · outbound

This paper cites The MASSIVE Survey - VIII. Stellar Velocity Dispersion Profiles and Environmental Dependence of Early-Type Galaxies.

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Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.558291Z

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Observation 82a02387-8fe1-4360-bcbc-8b115bf43528 · outbound

This paper cites The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III,.

Uncertainties in the supermassive black hole abundance and implications for the GW background The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III,

Reference 63

Resolution: verified fuzzy; raw_fallback, observed 2026-08-04T21:30:32.106251Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 1700e16c-61e7-42a0-9b8c-ea050a6d73d5 · outbound

This paper cites Near-infrared Imaging of Early-Type Galaxies. II. Global Photometric Parameters,.

Uncertainties in the supermassive black hole abundance and implications for the GW background Near-infrared Imaging of Early-Type Galaxies. II. Global Photometric Parameters,

Reference 65

Resolution: verified fuzzy; raw_fallback, observed 2026-08-04T21:30:32.096928Z

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Observation f364c245-1869-45ad-938e-e998e8b08680 · outbound

This paper cites The Scaling of Stellar Mass and Central Stellar Velocity Dispersion for Quiescent galaxies at z < 0.7.

Uncertainties in the supermassive black hole abundance and implications for the GW background The Scaling of Stellar Mass and Central Stellar Velocity Dispersion for Quiescent galaxies at z < 0.7

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.573857Z

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Observation 52324c1a-6e7b-4669-a343-d5e889d92198 · outbound

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Uncertainties in the supermassive black hole abundance and implications for the GW background The Bolometric Quasar Luminosity Function at z = 0-7

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.576654Z

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Observation 2ac7221c-e28a-4487-9381-adf12885ca56 · outbound

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Uncertainties in the supermassive black hole abundance and implications for the GW background The Lvpropσ 8 Correlation for Elliptical Galaxies with Cores: Relation with Black Hole Mass,

Reference 68

Resolution: verified fuzzy; raw_fallback, observed 2026-08-04T21:30:32.088077Z

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Observation a3bfdaa5-a061-4d41-b01f-5f8221a52ba9 · outbound

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Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.582050Z

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Observation 7f252450-4973-401f-8875-6d68b4ce9054 · outbound

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Reference 71

Resolution: verified fuzzy; raw_fallback, observed 2026-08-04T21:30:32.079585Z

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Observation d95b0ea0-e07d-4aa5-9277-d8e08727e427 · outbound

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Uncertainties in the supermassive black hole abundance and implications for the GW background The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.592840Z

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Observation fda0d322-d5e3-42f2-a344-8f62879ecb87 · outbound

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Uncertainties in the supermassive black hole abundance and implications for the GW background A Log-Quadratic Relation Between the Nuclear Black-Hole Masses and Velocity Dispersions of Galaxies

Reference 2006

Resolution: verified exact; local_arxiv, observed 2026-08-04T21:30:31.633484Z

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Observation 38cd40bf-7a20-4453-af65-713b7e1d03b5 · outbound

This paper cites The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes.

Reference 2007

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.352497Z

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Observation 78534ebe-67ab-4259-a176-6fd15972f7ed · outbound

This paper cites Galaxy luminosities, stellar masses, sizes, velocity dispersions as a function of morphological type.

Uncertainties in the supermassive black hole abundance and implications for the GW background Galaxy luminosities, stellar masses, sizes, velocity dispersions as a function of morphological type

Reference 2010

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.515679Z

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Observation 8514b4b7-769a-409b-be95-83dbec851843 · outbound

This paper cites The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III.

Uncertainties in the supermassive black hole abundance and implications for the GW background The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III

Reference 2011

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.568218Z

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Observation 74ca75da-6076-4851-9572-af6b34e5addf · outbound

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Uncertainties in the supermassive black hole abundance and implications for the GW background Selection bias in dynamically-measured super-massive black hole samples: its consequences and the quest for the most fundamental relation

Reference 2016

Resolution: unresolved; no resolver link, observed 2026-08-04T21:30:31.496357Z

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Dark QCD Origin of the NANOGrav Signal and Self-Interacting Dark Matter Uncertainties in the supermassive black hole abundance and implications for the GW background

Reference 38

Resolution: verified exact; arxiv_id, observed 2026-05-16T16:03:04.208816Z

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Reference 155

Resolution: verified exact; arxiv_id, observed 2026-06-28T21:42:38.996643Z

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Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-07T10:59:31.828971Z

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