Pith. sign in

Paper Citation Record · LEDGER

A method for constructing the joint mass function of binary stars

As of 14 August 2026, this Paper Citation Record lists 3 of 3 outbound references and 0 inbound Pith citation observations for arXiv:2602.10186.

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

pith.paper-citation-record.v1
2602.10186 v2

Coverage vector

measured 3 of 3 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-03T01:18:55.023492Z

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

3 of 3 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved3
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation a497be1d-2ba4-4698-b221-b7388a21a95e · outbound

This paper cites E., 1997, The Numerical Solution of Integral Equa- tions of the Second Kind.

A method for constructing the joint mass function of binary stars E., 1997, The Numerical Solution of Integral Equa- tions of the Second Kind

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-03T01:18:54.857247Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T01:18:54.857247Z digest=sha256:8efeaaf49dc55d8f0c17b9bb7349317b7f73e40e0da1e12e29595e2afbcf82cd

Observation 777a09af-a16b-4edc-9244-b1eb0885130e · outbound

This paper cites This equation does not have closed- form solution but we can instead use a numerical method, specifically the Nyström method ( Hackbusch 1995).

A method for constructing the joint mass function of binary stars This equation does not have closed- form solution but we can instead use a numerical method, specifically the Nyström method ( Hackbusch 1995)

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-03T01:18:55.023492Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T01:18:55.023492Z digest=sha256:f23a0688e0112d69f182d55bbdd1e75399f318df621bcdd8e0386f7dcaae778b

Observation 04a3fdff-986b-4db7-9817-dfa539f11cf8 · outbound

This paper cites The initial mass function of stars.

A method for constructing the joint mass function of binary stars The initial mass function of stars

Reference 120

Resolution
unresolved
no resolver link, observed 2026-08-03T01:18:54.929526Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T01:18:54.929526Z digest=sha256:c0671b7a8b847aba6ee85d4f993a06ba946695c148d6084a8a33ced4115e7d24

Pith citing papers

No inbound Pith citation observations are available.