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Paper Citation Record · LEDGER

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

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 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 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:51:46.753375Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T04:51:47.136532Z

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 71f8cf9b-3408-4e17-82c1-67b830a138a4 · inbound

Radioactive heating rate of r-process elements and macronova light curve cites this paper.

Radioactive heating rate of r-process elements and macronova light curve Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

Reference 2

Resolution
metadata mismatch
local_arxiv, observed 2026-08-14T04:51:47.140867Z

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=2026-08-14T04:51:46.753375Z digest=sha256:06d2fed1182419392fd9a8fc843915be7068f4455e679da519f1c4e837064e1c

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=sha256:768f40e38ec7e1b3e8f829ae90b7895198c336fcc047de3fce8657896db97549

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=sha256:470172ab44d94c2419af97ce14d95fe2ad4069ef5265baa2b0141c5124a97b14