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Paper Citation Record · LEDGER

Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1710.05844.

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

pith.paper-citation-record.v1
1710.05844 v1

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 2026-08-04T06:34:03.388597+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T00:44:17.955713Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T06:15:00.866473Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 6c10d294-7578-4da1-9ab0-5be49f93ca55 · inbound

Rapid and robust simulation-based inference for kilonovae cites this paper.

Rapid and robust simulation-based inference for kilonovae Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration

Reference 147

Resolution
verified exact
local_arxiv, observed 2026-05-15T02:39:40.631274Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:413c354b6e23a309c37661959d80248985811cfefcab051d6499ee9dd039d6e9

Observation b997d72b-90ab-4e4a-98d4-f8271776af60 · inbound

Gamma-ray burst progenitors revisited cites this paper.

Gamma-ray burst progenitors revisited Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-01T00:44:17.955713Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:44:17.955713Z digest=sha256:06f9b3679f4c1d5d4e1c1fd136de3496346b922f9b39a73282afc58cf7ef1050

Observation 24eab095-cb4b-4856-8885-ec1ed4e7396e · 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 Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration

Reference 259

Resolution
unresolved
no resolver link, observed 2026-07-31T07:22:46.199642Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T07:22:46.199642Z digest=sha256:73fc6eec7c4bb8aeed5d54d6475178bbe1f2bc66417b488c1ff666c37e4900dd