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Paper Citation Record · LEDGER

Line-of-sight mass estimator and the masses of the Milky Way and Andromeda Galaxy

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2503.12612.

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

pith.paper-citation-record.v1
2503.12612 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T00:31:19.076878Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

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  • 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 fa9e4f54-0a12-4fc2-9568-e8694e883287 · inbound

Refining primordial black hole dark matter constraints with dust heating: the role of spin and halo profile dependence cites this paper.

Refining primordial black hole dark matter constraints with dust heating: the role of spin and halo profile dependence Line-of-sight mass estimator and the masses of the Milky Way and Andromeda Galaxy

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-02T00:31:19.076878Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T00:31:19.076878Z digest=sha256:56220bcdd902a8bff4d159854adc2620ae43fa1da42e820e9c84b15dbcb159de

Observation eaabf89b-eda7-48bc-aa5d-8d1b2ba255b0 · inbound

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters cites this paper.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Line-of-sight mass estimator and the masses of the Milky Way and Andromeda Galaxy

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-01T23:43:56.255781Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T23:43:56.255781Z digest=sha256:61d10d8e567d90d73b9dc1dc8f89563a39425fdcb8784ad9fde35d32b0ad7dd6