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Paper Citation Record · LEDGER

Counting Black Holes: The Cosmic Stellar Remnant Population and Implications for LIGO

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1703.02551.

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

pith.paper-citation-record.v1
1703.02551 v2

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 2026-08-06T06:34:29.942622+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T20:06:29.044059Z

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 f3841b1e-1a93-4987-ac1a-23b25c0670db · inbound

Can current models predict the local black hole merger rate? cites this paper.

Can current models predict the local black hole merger rate? Counting Black Holes: The Cosmic Stellar Remnant Population and Implications for LIGO

Reference 250

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:02:10.806267Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b8ffbfba03e7a0531eb9d094a8f846752d11efd04a8abdf888134f1f20d0cf4d

Observation 419b00f5-3a33-4f4c-b16a-ba5c35e77136 · inbound

Too shy to spin? Cosmic wallflowers as proto-globular clusters cites this paper.

Too shy to spin? Cosmic wallflowers as proto-globular clusters Counting Black Holes: The Cosmic Stellar Remnant Population and Implications for LIGO

Reference 31

Resolution
verified exact
local_arxiv, observed 2026-06-29T02:13:00.598725Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6b520590864f0b7f5b4534cb929d88dafd0c1f16ac1fe12ceb923bd5c472872f

Observation d2cf38e6-e816-46c3-aada-c772062bddb3 · inbound

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers cites this paper.

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers Counting Black Holes: The Cosmic Stellar Remnant Population and Implications for LIGO

Reference 108

Resolution
verified exact
local_arxiv, observed 2026-07-09T20:06:29.045387Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:2537f1f820a374e206f245837a8b5580859198c1afeba686e3de910c356082b5