Pith. sign in

Paper Citation Record · LEDGER

The scenario of two families of compact stars 2. Transition from hadronic to quark matter and explosive phenomena

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1509.02134.

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

pith.paper-citation-record.v1
1509.02134 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 2026-08-09T06:31:02.800959+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T12:12:25.342204Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T07:49:38.952014Z

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 2390690d-d6ac-4959-bcdc-388da39bd21f · 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 2. Transition from hadronic to quark matter and explosive phenomena

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-06T12:12:25.342204Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T12:12:25.342204Z digest=sha256:1b100ad37bf9eeb85d87dbf24a34ffd3c4d943ce0e6592b6272eb23ecbd0afa8

Observation 62bc2ac5-19a4-47c3-a713-b9a3f1c07cc6 · 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 2. Transition from hadronic to quark matter and explosive phenomena

Reference 50

Resolution
verified exact
local_arxiv, observed 2026-07-04T07:49:38.953309Z

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:e7011aa6bcb90f594391790a7979754c3100bc7fdfb46f12464571282da35e07