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Paper Citation Record · LEDGER

Spiral-wave wind for the blue kilonova

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1907.04872.

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

pith.paper-citation-record.v1
1907.04872 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 2026-08-21T06:32:19.484+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T10:20:11.860786Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T18:45:59.295955Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • malformed identifier0
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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 f1141a98-dd70-4c9c-bff0-269ad822b938 · inbound

kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter cites this paper.

kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter Spiral-wave wind for the blue kilonova

Reference 126

Resolution
unresolved
no resolver link, observed 2026-08-14T10:20:11.860786Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:20:11.860786Z digest=sha256:367ec297db7074bfafb62e556c4bb196fa803f4d7fad8918d3d9b16e1fb3a546

Observation 067ebe0b-0fe2-4b8e-abde-fb0f48499b76 · inbound

Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars cites this paper.

Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars Spiral-wave wind for the blue kilonova

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-11T18:36:01.119276Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T18:36:01.119276Z digest=sha256:d59090f6d44f6245f55261068705ff5cc92dfd09a8110425eeaf4e9f26d12321

Observation c6c9c27e-0507-4669-9f76-580bc21ebbb9 · inbound

Exact Mass Conservation in Binary Neutron Star Merger Simulations cites this paper.

Exact Mass Conservation in Binary Neutron Star Merger Simulations Spiral-wave wind for the blue kilonova

Reference 34

Resolution
verified exact
arxiv_id, observed 2026-06-29T05:53:09.169645Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-06-29T05:45:55.511016Z digest=sha256:a93d8cfb6a3a7c80e4abef43f5ecb105b75d301e81f480d07889e0ad7079822b

Observation cdcb21ab-9f66-41bd-ae2b-551a645b99f0 · inbound

Impact of neutrino-electron scattering and an improved treatment of pair processes on binary neutron star mergers cites this paper.

Impact of neutrino-electron scattering and an improved treatment of pair processes on binary neutron star mergers Spiral-wave wind for the blue kilonova

Reference 51

Resolution
verified exact
arxiv_id, observed 2026-07-01T18:45:59.297605Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-06-29T01:37:25.342025Z digest=sha256:7a67d6704a6b190b90aa71dca37e8e0b29da8ed5f8338da6cca64708dae0d9e4

Observation 599a3477-8382-4ecc-91c2-70053b653973 · inbound

Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology cites this paper.

Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology Spiral-wave wind for the blue kilonova

Reference 185

Resolution
unresolved
no resolver link, observed 2026-07-31T07:22:45.958702Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T07:22:45.958702Z digest=sha256:c48341bcc413621d8883213aee5edf11ca0790f05dd3f3e44995acff413a199e

Observation 619b12ff-6e5a-4d5c-ae07-b201812e0bed · inbound

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves cites this paper.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Spiral-wave wind for the blue kilonova

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.754414Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.754414Z digest=sha256:3582752219f91db2b4b83ccc3efac3f7cbbbb3bc3f0c1162528bcdff3f97fcde