Pith. sign in

Paper Citation Record · LEDGER

How Many Kilonovae Can Be Found in Past, Present, and Future Survey Datasets?

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1710.05845.

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

pith.paper-citation-record.v1
1710.05845 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 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-31T07:22:45.594768Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T19:01:08.933320Z

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 7ad0fa62-0f58-4866-91fa-a72d17518d99 · inbound

A Multi-Wavelength View of the First Type Ic-BL Supernova with an Einstein Probe X-ray Shock Breakout cites this paper.

A Multi-Wavelength View of the First Type Ic-BL Supernova with an Einstein Probe X-ray Shock Breakout How Many Kilonovae Can Be Found in Past, Present, and Future Survey Datasets?

Reference 230

Resolution
verified exact
local_arxiv, observed 2026-06-27T19:01:08.940049Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8900f9fd4b80a8cca9433672e590b813fd87fddd51a31d6e2be2f7a1bec6e042

Observation dedee20c-d162-4c23-88e9-ccf2597383b1 · 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 How Many Kilonovae Can Be Found in Past, Present, and Future Survey Datasets?

Reference 66

Resolution
unresolved
no resolver link, observed 2026-07-31T07:22:45.594768Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T07:22:45.594768Z digest=sha256:b3a7d125f11e57fd520b1e70ca93bb8071eb8cda38b5c47a3cfa50d92754a486