Pith. sign in

Paper Citation Record · LEDGER

The slope of the black-hole mass versus velocity dispersion correlation

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:astro-ph/0203468.

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

pith.paper-citation-record.v1
astro-ph/0203468 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T23:10:51.235976Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T18:10:02.402066Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation f4d0f1c5-9c24-4797-9234-1edb0efedece · inbound

What drives the growth of black holes: a decade of progress cites this paper.

What drives the growth of black holes: a decade of progress The slope of the black-hole mass versus velocity dispersion correlation

Reference 753

Resolution
unresolved
no resolver link, observed 2026-08-06T23:10:51.235976Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T23:10:51.235976Z digest=sha256:0c1353f557e11f260329bc5419e04c36d44b4f3d0a16718414c897c0667405d1

Observation 05f3159d-4e69-40f0-ae39-3eb47e08d938 · inbound

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap cites this paper.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The slope of the black-hole mass versus velocity dispersion correlation

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-04T19:47:51.926010Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T19:47:51.926010Z digest=sha256:89f97ae7a6c29067c5a231dc61585ddf137776500756d6d8b1ec926abea9bea1

Observation 180bfb58-8b02-4b18-bd05-3db28dcfa9fa · inbound

Mapping the nuclear environments of extreme coronal line emitting galaxies cites this paper.

Mapping the nuclear environments of extreme coronal line emitting galaxies The slope of the black-hole mass versus velocity dispersion correlation

Reference 121

Resolution
verified exact
local_arxiv, observed 2026-06-28T09:11:49.554491Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e64b35788245012795264af440822b4b8461774b1a6c2de1ab8f3f4164ae7366

Observation 776b3e20-0efe-4735-8c85-cb9ddf9fb9f0 · inbound

Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations cites this paper.

Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations The slope of the black-hole mass versus velocity dispersion correlation

Reference 62

Resolution
verified exact
local_arxiv, observed 2026-06-28T01:01:27.056836Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:a6daef24dd9d3b4d42ec53f30ca2b1c166ce95cfb72231f8048ae82b9de83dad

Observation cb528a27-928b-4fe1-bbf0-fcd932cfe49a · inbound

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 cites this paper.

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 The slope of the black-hole mass versus velocity dispersion correlation

Reference 62

Resolution
metadata mismatch
local_arxiv, observed 2026-07-04T18:10:02.403599Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-06-25T22:58:21.809334Z digest=sha256:a10228218ea6ebf45e3c6c778ca150efcdcfd67b5f7a6f3c8f6fe82e77150d6e

Observation 622ae314-1b23-4e55-b98b-9475874e27cf · inbound

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 cites this paper.

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 The slope of the black-hole mass versus velocity dispersion correlation

Reference 62

Resolution
metadata mismatch
local_arxiv, observed 2026-07-04T13:19:50.158393Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-06-26T05:24:52.713752Z digest=sha256:95204fceae4ce061870d9b7f40534bf3d0a5f88ef08929b345713f7e0fdc4e0d

Observation 8cc39252-31a2-4630-9431-34743e09de09 · inbound

Too shy to spin? Cosmic wallflowers as proto-globular clusters cites this paper.

Too shy to spin? Cosmic wallflowers as proto-globular clusters The slope of the black-hole mass versus velocity dispersion correlation

Reference 23

Resolution
verified exact
local_arxiv, observed 2026-06-29T02:13:00.683505Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:40654c2eab75c4ff83ebec325d956dc695c8e595da877438aad4d4bcaa70aaad

Observation a4fb6e6c-efba-4627-839f-4139d329d187 · inbound

Jet--ISM Interactions in Gaseous Disks: Simulating Kinetic Feedback in the Radio Galaxy 3C 326 N cites this paper.

Jet--ISM Interactions in Gaseous Disks: Simulating Kinetic Feedback in the Radio Galaxy 3C 326 N The slope of the black-hole mass versus velocity dispersion correlation

Reference 44

Resolution
unresolved
no resolver link, observed 2026-07-12T05:06:34.225475Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T05:06:34.225475Z digest=sha256:4758c00c148af5c2cae8a3c17a6241496bfd3652f8c024a3c0a9d0f81286dc82

Observation 82a768da-cb32-4bbf-9105-74272546ae7c · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ The slope of the black-hole mass versus velocity dispersion correlation

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-01T06:58:40.978772Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T06:58:40.978772Z digest=sha256:8fd3b40f66a0cd9e8397964d0138d313b71016c7fcf6a8190ce495038a9d645c

Observation fc90be7e-833e-4da8-86f8-772ccdf96028 · inbound

From S2 to LISA: Astrometric Bounds on Extreme-Mass-Ratio Inspirals and Bursts cites this paper.

From S2 to LISA: Astrometric Bounds on Extreme-Mass-Ratio Inspirals and Bursts The slope of the black-hole mass versus velocity dispersion correlation

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-01T00:50:15.960212Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:50:15.960212Z digest=sha256:45f40c6eeb7abe55f7d1cc97d9938498d70205234ea61aeb70929c585281bffb

Observation 6014e559-c2d0-48ac-926b-078deecdd45b · inbound

The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies cites this paper.

The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies The slope of the black-hole mass versus velocity dispersion correlation

Reference 247

Resolution
unresolved
no resolver link, observed 2026-08-06T00:06:27.394365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T00:06:27.394365Z digest=sha256:180f7bd3ea5020c7a1bb9ce39b7884d805bf7e16ae5f84d144d4761261dbe0e8