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Paper Citation Record · LEDGER

Exploding neutron stars in close binaries

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1808.05287.

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

pith.paper-citation-record.v1
1808.05287 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T13:39:56.154587Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • malformed identifier0
  • metadata mismatch0

External citation measurements

33
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3d637641-2ec1-4673-82d1-c10036c7ffb3 · inbound

An Optically Led Search for Kilonovae to z$\sim$0.3 with the Kilonova and Transients Program (KNTraP) cites this paper.

An Optically Led Search for Kilonovae to z$\sim$0.3 with the Kilonova and Transients Program (KNTraP) Exploding neutron stars in close binaries

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-12T13:39:56.154587Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T13:39:56.154587Z digest=sha256:4f7119384d47d2b439c989ade3148ac7e8e8750e980c302ffcaa4ec2e8e4d9b1

Observation a6202928-f616-42c7-afae-42f1e869e48a · inbound

Multi-Peaked Non-Thermal Light Curves from Magnetar-Powered Gamma-Ray Bursts cites this paper.

Multi-Peaked Non-Thermal Light Curves from Magnetar-Powered Gamma-Ray Bursts Exploding neutron stars in close binaries

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-11T14:21:48.075007Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T14:21:48.075007Z digest=sha256:99dbb871fb1311adaae86b12661e69c692d78b63fd60fe8ffbf5efb567699422

Observation 01c32e49-ff6e-4ba9-9d80-1b4a4be8317f · inbound

Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta cites this paper.

Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta Exploding neutron stars in close binaries

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-05T15:52:56.317060Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T15:52:56.317060Z digest=sha256:3a4699eab37d894239314afe2c2b4972fd75dc679248f4bba9acb533619265ba

Observation 4caacad6-53c0-4900-af4a-a17b3dccffc2 · inbound

Wide Jets or Low Rates: Reconciling Short GRB and Gravitational-Wave Neutron Star Merger Rates cites this paper.

Wide Jets or Low Rates: Reconciling Short GRB and Gravitational-Wave Neutron Star Merger Rates Exploding neutron stars in close binaries

Reference 19

Resolution
verified exact
arxiv_id, observed 2026-05-10T19:40:46.165149Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-05-10T19:36:48.497341Z digest=sha256:625521fee1be7aaec4d4686a1e63b932fa11020807cbf981393939767a839c33

Observation 7421b510-6c7c-4fe4-86fa-d9ac1536ac15 · inbound

Subgrid Modelling for Relativistic Magnetohydrodynamics with Machine Learning cites this paper.

Subgrid Modelling for Relativistic Magnetohydrodynamics with Machine Learning Exploding neutron stars in close binaries

Reference 21

Resolution
verified exact
local_arxiv, observed 2026-07-04T07:29:39.554672Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-06-26T13:20:12.147520Z digest=sha256:cbe041d8af9504ebbecc883272fd69301f2e5567380975dadad58bac4d7c8673

Observation 448b3e41-e851-437d-b743-63a7702536f1 · inbound

4th TDAMM Workshop White Paper cites this paper.

4th TDAMM Workshop White Paper Exploding neutron stars in close binaries

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-01T04:57:58.116137Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T04:57:58.116137Z digest=sha256:62232a93b0b59da06aeafc5b45331e749a5fca93d4cbfb318a3f41e267557c69