Paper Citation Record · LEDGER

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

As of 22 August 2026, this Paper Citation Record lists 12 of 12 outbound references and 2 inbound Pith citation observations for arXiv:2505.02920.

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

pith.paper-citation-record.v1
2505.02920 v1

Coverage vector

measured 12 of 12 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:45:44.874983Z

measured 14 of 14 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T22:32:18.362126Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-04T21:30:31.874198Z

Reference resolution

12 of 12 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 60315989-1599-4454-bf73-49249adb4990 · outbound

This paper cites The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies.

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-16T00:45:44.821385Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 24024596-08a3-4eb4-99ea-810b082313ca · outbound

This paper cites (2016, r ed stars), plus some galaxies from the SMBH sample of Beiﬁori et al.

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass (2016, r ed stars), plus some galaxies from the SMBH sample of Beiﬁori et al

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T00:45:44.986633Z

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Observation 94d47386-8d1d-436e-9be6-d3f779b7683c · outbound

This paper cites The SDSS galaxy sub - sample they chose for this step had total galaxy luminositie s de- rived by Hon et al.

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass The SDSS galaxy sub - sample they chose for this step had total galaxy luminositie s de- rived by Hon et al

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T00:45:45.062245Z

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Observation 376387ea-ca4b-493f-a30b-24b8bf4fe0cc · outbound

This paper cites To remark this point, we show two linear ﬁts to the Sahu et al.

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass To remark this point, we show two linear ﬁts to the Sahu et al

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T00:45:45.046902Z

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Observation c6375dd3-f15f-4e21-b0e8-546427f6d216 · outbound

This paper cites In addition, the S 4G sample with velocity dispersion measurements in the Hy- perleda database is around 1/4 of the original sample, and th us it could suffer from incompleteness.

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass In addition, the S 4G sample with velocity dispersion measurements in the Hy- perleda database is around 1/4 of the original sample, and th us it could suffer from incompleteness

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T00:45:45.032201Z

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Observation ec107352-56dd-40d6-9416-1c76a04435de · outbound

This paper cites Note that an off- © 2025 RAS, MNRAS 000, 1–23 20 F.

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass Note that an off- © 2025 RAS, MNRAS 000, 1–23 20 F

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T00:45:45.018123Z

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Observation 665fcdad-a114-4bb1-b394-009ba07c2fcc · outbound

This paper cites The SMBH sample has a tendency to be characterized, on average, by larger stella r velocity dispersions at ﬁxed luminosity.

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass The SMBH sample has a tendency to be characterized, on average, by larger stella r velocity dispersions at ﬁxed luminosity

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T00:45:45.002938Z

Source-reported events for the cited work

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Observation 9f3acdaf-dd2e-4720-a0df-6663acff199c · outbound

This paper cites At face value, this value of the mean SMBH mass would be signiﬁcantly higher © 2025 RAS, MNRAS 000, 1–23 Scalings and Residuals 21 Figure A3.

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass At face value, this value of the mean SMBH mass would be signiﬁcantly higher © 2025 RAS, MNRAS 000, 1–23 Scalings and Residuals 21 Figure A3

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T00:45:44.957274Z

Source-reported events for the cited work

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Observation 1898c7bd-5bc6-42c6-8ec5-eff31332eb9a · outbound

This paper cites (2016) at an av- erage stellar mass of Mgal = 1.

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass (2016) at an av- erage stellar mass of Mgal = 1

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T00:45:44.942006Z

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Observation 27d2e93a-8246-4486-8dc8-a805bfa7e225 · outbound

This paper cites equivalent.

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

Reference 12

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Observation 0afab8f5-566e-4dfd-b25e-7d4a34d332a5 · outbound

This paper cites an unresolved cited work.

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass Unresolved cited work

Reference 23

Resolution: unresolved; raw_fallback, observed 2026-08-16T00:45:44.972250Z

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Observation 1aee5e98-ff70-4201-a5d8-0579052e6142 · outbound

This paper cites (2014) and colour-dependent mass-to-lig ht ra- tios from Bell et al.

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass (2014) and colour-dependent mass-to-lig ht ra- tios from Bell et al

Reference 1968

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T00:45:45.077310Z

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Pith citing papers

Observation f04975a9-fe3a-4caf-b179-dd03db0ab0a5 · inbound

AGN with massive black holes have closer galactic neighbors: k-Nearest-Neighbor statistics of an unbiased sample of AGN at z~0.03 cites this paper.

AGN with massive black holes have closer galactic neighbors: k-Nearest-Neighbor statistics of an unbiased sample of AGN at z~0.03 Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-06T22:32:18.362126Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Uncertainties in the supermassive black hole abundance and implications for the GW background cites this paper.

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

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.