Paper Citation Record · LEDGER

How Early Could the Milky Way's Disk Form?

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2409.18173.

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

pith.paper-citation-record.v1
2409.18173 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T12:53:27.963811Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

2
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 4dd7b24f-9679-44f5-93f0-4518e1b74fe3 · inbound

Rediscovering the Milky Way with orbit superposition approach and APOGEE data II. Chrono-chemo-kinematics of the disc cites this paper.

Rediscovering the Milky Way with orbit superposition approach and APOGEE data II. Chrono-chemo-kinematics of the disc How Early Could the Milky Way's Disk Form?

Reference 239

Resolution: unresolved; no resolver link, observed 2026-08-12T12:53:27.963811Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 52261bfb-6f47-418d-b2c3-8b39499465ca · inbound

Stellar Velocity Dispersion versus Age: Consistency across Observations and Simulations, with the Milky Way as an Outlier cites this paper.

Stellar Velocity Dispersion versus Age: Consistency across Observations and Simulations, with the Milky Way as an Outlier How Early Could the Milky Way's Disk Form?

Reference 245

Resolution: unresolved; no resolver link, observed 2026-08-07T04:10:57.193410Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 94525ee0-35f7-4485-bfa5-c402a1e61695 · inbound

Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way cites this paper.

Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way How Early Could the Milky Way's Disk Form?

Reference 124

Resolution: verified exact; arxiv_id, observed 2026-05-18T17:31:40.845492Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 44d4f180-409b-47b8-91d4-4ecb2130e550 · inbound

Resolved Ages and Stellar Metallicities in Progenitors of Milky Way Analogs: A Closer Look at their Star Formation Histories since $z=5$ cites this paper.

Resolved Ages and Stellar Metallicities in Progenitors of Milky Way Analogs: A Closer Look at their Star Formation Histories since $z=5$ How Early Could the Milky Way's Disk Form?

Reference 42

Resolution: metadata mismatch; arxiv_id, observed 2026-06-26T14:39:32.626613Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.