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Paper Citation Record · LEDGER

GW190814: Circumstantial Evidence for Up-Down Quark Star

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2009.00942.

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

pith.paper-citation-record.v1
2009.00942 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 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T05:13:19.994572Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T19:08:50.116879Z

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 95ab50ba-da3e-4c0d-bbe5-e5a81cf50fa1 · inbound

Interacting quark matter and $f(Q)$ gravity: A new paradigm in exploring the properties of quark stars cites this paper.

Interacting quark matter and $f(Q)$ gravity: A new paradigm in exploring the properties of quark stars GW190814: Circumstantial Evidence for Up-Down Quark Star

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-12T05:13:19.994572Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T05:13:19.994572Z digest=sha256:8ca8449fba60de50a92335433ed45f5951b62acf8b1db692f283c710872d4349

Observation 5725a98f-73f7-4ecc-abb4-97c5b14fa69a · inbound

Can a Slow and Strong Phase Transition in Neutron Stars Relieve Major Compact-Star Observation Tensions? cites this paper.

Can a Slow and Strong Phase Transition in Neutron Stars Relieve Major Compact-Star Observation Tensions? GW190814: Circumstantial Evidence for Up-Down Quark Star

Reference 63

Resolution
verified exact
arxiv_id, observed 2026-07-03T19:08:50.120341Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-06-27T02:06:36.071557Z digest=sha256:b7132704e06b73b2493ef586cb98070daad8db2cbe45c6d592619d21a5592c0b