Pith. sign in

Paper Citation Record · LEDGER

The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1509.02131.

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

pith.paper-citation-record.v1
1509.02131 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T12:12:25.339035Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T07:49:38.885201Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • 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 15622cde-2d4d-4817-96aa-8fd31400d2f4 · inbound

On the formation of strange quark stars from supernova in compact binaries cites this paper.

On the formation of strange quark stars from supernova in compact binaries The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-06T12:12:25.339035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T12:12:25.339035Z digest=sha256:6a10dd2140a86362d7d2b05c1d48aea3c14d4c380ebb6ae8e690694fc55b6310

Observation c929fa37-6f26-4ee2-86c3-21304c8960a9 · inbound

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis cites this paper.

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems

Reference 49

Resolution
verified exact
local_arxiv, observed 2026-07-04T07:49:38.886455Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-26T12:50:53.032717Z digest=sha256:e2a314e62555ea5ec904fd04bc8d09c4683ee6689717f82905f85a391e7a00af

Observation 40f05e70-db5b-42fc-9e70-f91ccbc3fb4d · inbound

The equation of state for neutron stars cites this paper.

The equation of state for neutron stars The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:06.355493Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:06.355493Z digest=sha256:83b8fc57bdf4c1c0a29388a72c7064a2536e2361a0478698fb01f60133111555