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Paper Citation Record · LEDGER

Simulations of early kilonova emission from neutron star mergers

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2008.05495.

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

pith.paper-citation-record.v1
2008.05495 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:41:13.123596Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T13:17:05.604905Z

Reference resolution

0 of 0 outbound references displayed

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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 244a3bbb-3016-4084-ab7f-12a9aebca8fc · inbound

Science with the Einstein Telescope: a comparison of different designs cites this paper.

Science with the Einstein Telescope: a comparison of different designs Simulations of early kilonova emission from neutron star mergers

Reference 68

Resolution
verified exact
arxiv_id, observed 2026-05-17T21:43:30.203851Z

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.

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Observation a2d6659a-76ea-4e1d-8a08-23c469053718 · inbound

Calibrated Lanthanide Atomic Data for Kilonova Radiative Transfer. I. Atomic Structure and Opacities cites this paper.

Calibrated Lanthanide Atomic Data for Kilonova Radiative Transfer. I. Atomic Structure and Opacities Simulations of early kilonova emission from neutron star mergers

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-06T18:41:13.123596Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T18:41:13.123596Z digest=sha256:a9c3841480f8250ca5c39c3b9080a95e7cd7699d05f1d0e2c25316f420ffa7cc

Observation f7a06451-ecc2-4e45-9f12-05885692bc6c · inbound

A magnetar formation in binary neutron star merger cites this paper.

A magnetar formation in binary neutron star merger Simulations of early kilonova emission from neutron star mergers

Reference 11

Resolution
verified exact
arxiv_id, observed 2026-07-03T07:37:44.859332Z

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=2026-06-27T12:03:16.536504Z digest=sha256:f701a119d605dc526d233250d3267369637959dbfc2ba42e8dee72ce9d5a472d

Observation 418de965-b4c0-4842-86fe-e1fcc9f2e5b4 · inbound

Multi-wavelength Constraints on the Transient EP250905a cites this paper.

Multi-wavelength Constraints on the Transient EP250905a Simulations of early kilonova emission from neutron star mergers

Reference 267

Resolution
verified exact
local_arxiv, observed 2026-07-10T13:17:05.606400Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f1d31dfd0dcd4dc8472b4f15dfda70aa0e23737fd04a0e4fc2745711b2d47768