Paper Citation Record · LEDGER

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$

As of 15 August 2026, this Paper Citation Record lists 15 of 15 outbound references and 2 inbound Pith citation observations for arXiv:2505.24129.

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

pith.paper-citation-record.v1
2505.24129 v1

Coverage vector

measured 15 of 15 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T12:38:45.549160Z

measured 17 of 17 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T17:33:44.864314Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T18:16:17.926450Z

Reference resolution

15 of 15 outbound references displayed

verified exact1
verified fuzzy10
unresolved0
parse uncertain0
malformed identifier4
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 40abf389-8d82-4b73-b24e-7ab828783dea · outbound

This paper cites MSA-3D: dissecting galaxies at z~1 with high spatial and spectral resolution.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ MSA-3D: dissecting galaxies at z~1 with high spatial and spectral resolution

Reference 1

Resolution: verified exact; local_arxiv, observed 2026-08-07T12:38:45.849836Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation c2c6eabd-5a86-443f-bcf2-d35ded89d04a · outbound

This paper cites (2013) 14:19:40.10 52:49:39.10 1.230 CO( 3−.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2013) 14:19:40.10 52:49:39.10 1.230 CO( 3−

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:50.163285Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 390e6c22-eaa7-4c5d-b4fa-5874271087ed · outbound

This paper cites (2013) 14:19:45.00 52:52:28.00 1.530 CO( 3−.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2013) 14:19:45.00 52:52:28.00 1.530 CO( 3−

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:49.802454Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation daf1fc9d-fec9-4a0d-ba61-344cac3e8ff0 · outbound

This paper cites (2018) 04:19:26.66 52:51:17.00 1.400 CO( 3−.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2018) 04:19:26.66 52:51:17.00 1.400 CO( 3−

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:49.512299Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 28b0d650-8717-4007-a5d6-13ad90b47816 · outbound

This paper cites (2023).

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2023)

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:49.207914Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 6b78a2ed-7f84-4c77-8081-f84b59680c32 · outbound

This paper cites (2023).

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2023)

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:48.878534Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation b6e62f97-5481-48df-b45e-3a80936d9a64 · outbound

This paper cites 2021); GALPAK3D (Bouché et al.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ 2021); GALPAK3D (Bouché et al

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:48.557616Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 6c65d72b-9d67-4555-b012-d793c12ff037 · outbound

This paper cites (2013) 94.0 Tacconi et al.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2013) 94.0 Tacconi et al

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:48.009783Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation d1899ac1-8fcd-4d66-a915-da4ed8d2025d · outbound

This paper cites (2013) 200.0 Tacconi et al.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2013) 200.0 Tacconi et al

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:47.710291Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 905aac8a-f95d-446b-aa7e-3b3227c02673 · outbound

This paper cites (2013) 373.0 Tacconi et al.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2013) 373.0 Tacconi et al

Reference 11

Resolution: malformed identifier; raw_fallback, observed 2026-08-07T12:38:47.397544Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 89fc5c04-7953-4111-87bc-6623dd78f436 · outbound

This paper cites (2018) 98.8 Übler et al.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2018) 98.8 Übler et al

Reference 12

Resolution: malformed identifier; raw_fallback, observed 2026-08-07T12:38:47.130722Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 5aa515f9-3eec-4d62-ad77-f23cd17f322f · outbound

This paper cites (2016) 1700.0 Tsukui et al.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2016) 1700.0 Tsukui et al

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:46.854619Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 59f5a019-bfe0-4e15-8ec7-852e3ede9fd9 · outbound

This paper cites (2023) 81.0 Liu et al.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2023) 81.0 Liu et al

Reference 14

Resolution: malformed identifier; raw_fallback, observed 2026-08-07T12:38:46.496158Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 9e99b79e-1980-4c11-85aa-7fe4bdcb6e28 · outbound

This paper cites (2023) 115.0 Liu et al.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2023) 115.0 Liu et al

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T12:38:46.127676Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation cfd25652-c38b-44d0-9b4c-f22821a33b5a · outbound

This paper cites (2013) 10.86 CO( 3−.

Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$ (2013) 10.86 CO( 3−

Reference 2015

Resolution: malformed identifier; raw_fallback, observed 2026-08-07T12:38:48.303872Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Pith citing papers

Observation 4ec29169-edcb-4ee4-9987-ea7521be3137 · inbound

Globular cluster formation from inertial inflows: accreting extremely massive stars as the origin of abundance anomalies cites this paper.

Globular cluster formation from inertial inflows: accreting extremely massive stars as the origin of abundance anomalies Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$

Reference 273

Resolution: verified exact; local_arxiv, observed 2026-08-10T17:33:45.014986Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 5ff1892c-e554-42da-b314-5adbb3c20299 · inbound

A quiescent galaxy in a gas-rich cosmic web node at z~3 cites this paper.

A quiescent galaxy in a gas-rich cosmic web node at z~3 Evolution of Gas Velocity Dispersion in Discs from $z\sim8$ to $z\sim0.5$

Reference 110

Resolution: unresolved; no resolver link, observed 2026-08-03T07:26:14.106724Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.