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Paper Citation Record · LEDGER

New Understanding of Large Magellanic Cloud Structure, Dynamics and Orbit from Carbon Star Kinematics

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0205161.

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

pith.paper-citation-record.v1
astro-ph/0205161 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:29:15.435479Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T14:52:18.966933Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • malformed identifier0
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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 0bb17d1d-6aa4-42f2-94be-6e85d38b537f · inbound

Tidal Suppression of Fuzzy Dark Matter Heating in Milky Way Satellite Galaxies cites this paper.

Tidal Suppression of Fuzzy Dark Matter Heating in Milky Way Satellite Galaxies New Understanding of Large Magellanic Cloud Structure, Dynamics and Orbit from Carbon Star Kinematics

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-06T20:52:50.490129Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T20:52:50.490129Z digest=sha256:cb34700badca46e3f1f302a30627d7657589f5f0090cf56b326719a8c8fb43df

Observation 63d5211f-1a26-40ed-895d-0fb8a96a40a3 · inbound

A New Record Census of Dwarf AGN and a Bimodal $M_{\rm BH}$-$M_{\star}$ Scaling Relation with DESI DR1 cites this paper.

A New Record Census of Dwarf AGN and a Bimodal $M_{\rm BH}$-$M_{\star}$ Scaling Relation with DESI DR1 New Understanding of Large Magellanic Cloud Structure, Dynamics and Orbit from Carbon Star Kinematics

Reference 218

Resolution
verified exact
local_arxiv, observed 2026-06-28T14:52:18.968621Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:67657d51466da110f14811f8f57ab5c13829b80c5a85da6065cff20d827fc8a4

Observation db45db40-80c6-4b18-b667-27ffa43cf84b · inbound

The VMC survey -- LV. The coherent expansion of the SMC cites this paper.

The VMC survey -- LV. The coherent expansion of the SMC New Understanding of Large Magellanic Cloud Structure, Dynamics and Orbit from Carbon Star Kinematics

Reference 155

Resolution
verified exact
local_arxiv, observed 2026-06-28T10:12:02.275077Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:93362a6631d43c507a71ab2ed0bd733c457d1f07cff41dc8791e142b76382f17

Observation 832ac43a-c245-4118-b916-6cbf3ce227b6 · inbound

Dark Matter in Draco and Bo\"otes I: Hints of a Core in an Ultra-Faint Dwarf from Simulation-Based Inference cites this paper.

Dark Matter in Draco and Bo\"otes I: Hints of a Core in an Ultra-Faint Dwarf from Simulation-Based Inference New Understanding of Large Magellanic Cloud Structure, Dynamics and Orbit from Carbon Star Kinematics

Reference 71

Resolution
verified exact
local_arxiv, observed 2026-06-26T01:58:54.421104Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:640589befe22f1f47f1dda244cae7088a0af0822af37052283cfbbf9c026e83e

Observation 5c3e3e15-d731-4ce5-bb5a-5f930e0465a6 · inbound

Deep MUSE observations of SNR 0509-67.5 reveal a double degenerate merger progenitor cites this paper.

Deep MUSE observations of SNR 0509-67.5 reveal a double degenerate merger progenitor New Understanding of Large Magellanic Cloud Structure, Dynamics and Orbit from Carbon Star Kinematics

Reference 111

Resolution
unresolved
no resolver link, observed 2026-08-16T00:29:15.435479Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:29:15.435479Z digest=sha256:beadad858ab5075bb64cd37a202a94560f5e06708ef00692c7c1f1e16f600d1f