Pith. sign in

Paper Citation Record · LEDGER

Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1710.05846.

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

pith.paper-citation-record.v1
1710.05846 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 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 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T20:20:19.987666Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • 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 d3e8e87c-bcaa-4800-a2e4-f2edf57cb630 · inbound

Toward a Unified Understanding of the Dense Matter Equation of State cites this paper.

Toward a Unified Understanding of the Dense Matter Equation of State Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

Reference 224

Resolution
unresolved
no resolver link, observed 2026-08-03T20:20:19.987666Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T20:20:19.987666Z digest=sha256:6a7c27e4fe5f5c6a150f418236eb165ad86e89d84857aa4d6d1e9143477779cb

Observation 0dd305c3-d86d-441f-9d72-5375814b5b86 · 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 Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

Reference 8

Resolution
unresolved
no resolver link, observed 2026-07-31T07:22:45.414074Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T07:22:45.414074Z digest=sha256:c041b9f51d71c4144b8d3885dcd0c63f6af5c821e39cdd42673e8b0eb8394d64