Paper Citation Record · LEDGER

A Milky Way with a massive, centrally concentrated thick disc: new Galactic mass models for orbit computations

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1611.07979.

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

pith.paper-citation-record.v1
1611.07979 v1

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 2026-08-15T06:32:42.880941+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T14:57:14.206805Z

measured 1 of 1 external citation measurements

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

Source: pith, 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

67
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 6aefd397-5179-4dc2-a0ba-9d8ad9e95c0d · inbound

Theoretical Predictions for the Inner Dark Matter Distribution in the Milky Way Informed by Simulations cites this paper.

Theoretical Predictions for the Inner Dark Matter Distribution in the Milky Way Informed by Simulations A Milky Way with a massive, centrally concentrated thick disc: new Galactic mass models for orbit computations

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-10T14:57:14.206805Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 10155437-b81e-4a74-bddb-3774a15a18b1 · inbound

Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison cites this paper.

Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison A Milky Way with a massive, centrally concentrated thick disc: new Galactic mass models for orbit computations

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-05-19T20:22:44.966361Z

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 a497c5e1-29fb-434e-9b08-7e9ae005e1ea · inbound

Bar-induced deflection of open cluster tidal tails cites this paper.

Bar-induced deflection of open cluster tidal tails A Milky Way with a massive, centrally concentrated thick disc: new Galactic mass models for orbit computations

Reference 5

Resolution: verified exact; local_arxiv, observed 2026-06-28T01:31:29.539213Z

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 39fc5e09-e107-4e15-b7c9-938726f38673 · inbound

Fractional-Dimension Gravity and the Milky Way Galaxy cites this paper.

Fractional-Dimension Gravity and the Milky Way Galaxy A Milky Way with a massive, centrally concentrated thick disc: new Galactic mass models for orbit computations

Reference 73

Resolution: verified exact; local_arxiv, observed 2026-07-03T19:28:52.235559Z

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.