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Paper Citation Record · LEDGER

Upper limit set by causality on the tidal deformability of a neutron star

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1701.03797.

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

pith.paper-citation-record.v1
1701.03797 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:44:03.573657Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T14:35:13.155510Z

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 7cfa204a-ed0d-4d80-b3aa-de6eaf9a05c9 · inbound

Explainable autoencoder for neutron star dense matter parameter estimation cites this paper.

Explainable autoencoder for neutron star dense matter parameter estimation Upper limit set by causality on the tidal deformability of a neutron star

Reference 13

Resolution
verified exact
local_arxiv, observed 2026-08-10T14:35:13.160482Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-08-10T14:35:12.304121Z digest=sha256:f7f9cc01e0427fc202792f587401e7bc2b7db3da422ba366aa566948b0686cea

Observation 963dd86c-7243-42a7-b7f9-6e5fc07ac6e8 · inbound

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression cites this paper.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Upper limit set by causality on the tidal deformability of a neutron star

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-16T05:44:03.573657Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T05:44:03.573657Z digest=sha256:78b394670cf8c9d6652d1d538ffcbc13f216faef5218235d4e4351afdf109239