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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 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 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 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T10:18:53.940913Z

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

140
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 2bd1185c-3bbb-4032-85da-3d86f18b7be2 · inbound

Kilonovae cites this paper.

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

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-14T10:18:53.940913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:18:53.940913Z digest=sha256:3737bd0584ede8dde5f7dc69b2d460f6ca61b98db2916d05abf716b5e7bdba07

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b95e7dd947d098ec31971c10c1a2a1417f387aeaaf12ed65cbc7bbbf002cb4f3

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=sha256:6033718d42f1f7d1b71d4fd45d2ac8f2161969aa475549a22e71f0b27138bfc7

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=sha256:9ee4ff4cd5a4c94145546736a17b2f1a78e7dd4e0f8da1ca4f5e4768072575d7

Observation 145caba3-7db5-4ba4-8367-432914013eef · 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 Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.667404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.667404Z digest=sha256:d2ea31bbc142ef5c4d27148cf92f4a7e747edbec5c01f911d8ba14283f2e8fa2