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Paper Citation Record · LEDGER

Electromagnetic emission from long-lived binary neutron star merger remnants II: lightcurves and spectra

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1508.07939.

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

pith.paper-citation-record.v1
1508.07939 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 2026-08-10T06:31:04.303077+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T16:33:53.557652Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T03:48:57.622638Z

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 3934f709-00e0-4fa4-8049-a6fdd74e2ef7 · inbound

Science Case for the Einstein Telescope cites this paper.

Science Case for the Einstein Telescope Electromagnetic emission from long-lived binary neutron star merger remnants II: lightcurves and spectra

Reference 101

Resolution
verified exact
local_arxiv, observed 2026-05-16T00:13:19.162055Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-16T00:13:18.137293Z digest=sha256:0b9f1c6a5f851ca831fecaa534a4575e951041d3638f6b1e8365f8bfbbc27bd7

Observation ad55d88a-df00-4e99-9526-a3f4d310c073 · inbound

Optical observations of candidate host galaxies of eight fast X-ray transients cites this paper.

Optical observations of candidate host galaxies of eight fast X-ray transients Electromagnetic emission from long-lived binary neutron star merger remnants II: lightcurves and spectra

Reference 154

Resolution
verified exact
local_arxiv, observed 2026-06-26T03:48:57.624087Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d894fc4248202cc19e86008c40d3ae83f188d59e0c64ae0c396300e90f31b5bc

Observation 445df0d4-bad5-4c46-a8b7-953609083c11 · inbound

Detectability of Gravitational-wave counterparts of EP-FXTs observed during the O4b LIGO-Virgo-KAGRA Observing Run cites this paper.

Detectability of Gravitational-wave counterparts of EP-FXTs observed during the O4b LIGO-Virgo-KAGRA Observing Run Electromagnetic emission from long-lived binary neutron star merger remnants II: lightcurves and spectra

Reference 126

Resolution
unresolved
no resolver link, observed 2026-08-01T21:06:23.500952Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T21:06:23.500952Z digest=sha256:3a320ab59e7b545ad37735836d33e939dce03cb21cb015d9394c2fff44d9eda6

Observation 36e8f6df-87fc-481e-91ec-19cde8476ed7 · inbound

A JWST redshift for the host galaxy of EP250207b of z=3.2: a collapsar origin is viable cites this paper.

A JWST redshift for the host galaxy of EP250207b of z=3.2: a collapsar origin is viable Electromagnetic emission from long-lived binary neutron star merger remnants II: lightcurves and spectra

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-05T16:33:53.557652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T16:33:53.557652Z digest=sha256:90488b74f9d85062406994308be9013f7b7248373b8b7eec2b8052067cd8fca8