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Paper Citation Record · LEDGER

Deformations of Accreting Neutron Star Crusts and Gravitational Wave Emission

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0001136.

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

pith.paper-citation-record.v1
astro-ph/0001136 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 2026-08-17T06:30:58.91139+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T23:00:46.065220Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T10:26:51.918774Z

Reference resolution

0 of 0 outbound references displayed

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation d15507d6-4c79-40e5-b8f2-d3e524d17573 · inbound

Galactic double neutron stars as dual-line gravitational-wave sources: Prospects with LISA and Cosmic Explorer cites this paper.

Galactic double neutron stars as dual-line gravitational-wave sources: Prospects with LISA and Cosmic Explorer Deformations of Accreting Neutron Star Crusts and Gravitational Wave Emission

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-15T23:00:46.065220Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T23:00:46.065220Z digest=sha256:613f220b74a28b83dc1cc6ce5b62cd2f4b902c69a007ea1012e7b66b3776f97f

Observation 7bfa90f0-5496-4a38-9993-2fc5ff1cdbd2 · inbound

Magnetized neutron stars: perturbative versus fully-numerical approaches cites this paper.

Magnetized neutron stars: perturbative versus fully-numerical approaches Deformations of Accreting Neutron Star Crusts and Gravitational Wave Emission

Reference 19

Resolution
verified exact
local_arxiv, observed 2026-05-20T04:23:03.432656Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-05-20T04:21:04.916385Z digest=sha256:3cf45eee8cc29f1e22f32d4c9a03180dea35c99a4e70b3568628ec74fd5ff9d1

Observation d94de13a-e30e-4062-8e01-f979aecc77a4 · inbound

First Constraints on the Ellipticities of Self-Interacting Fermionic Dark Matter Admixed Neutron Stars from Continuous Gravitational-Wave Searches cites this paper.

First Constraints on the Ellipticities of Self-Interacting Fermionic Dark Matter Admixed Neutron Stars from Continuous Gravitational-Wave Searches Deformations of Accreting Neutron Star Crusts and Gravitational Wave Emission

Reference 35

Resolution
verified exact
local_arxiv, observed 2026-07-02T10:26:51.920079Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-06-28T05:03:42.639549Z digest=sha256:9d984a649c7bbfffe1b5c1b769fab7a015f072a66900556ac66216fcd0149bab