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Paper Citation Record · LEDGER

Merging black hole binaries with the SEVN code

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1809.04605.

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

pith.paper-citation-record.v1
1809.04605 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T07:36:40.105989Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T01:14:08.104801Z

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 99f0e288-a0b1-474b-aa4f-9bc2e683472a · inbound

GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$ cites this paper.

GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$ Merging black hole binaries with the SEVN code

Reference 299

Resolution
verified exact
local_arxiv, observed 2026-05-16T03:16:33.647213Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b74ce3c4d4697481863bf4381dfddc2b489ca9f161f9c112735e6269f5298868

Observation 36185ce2-3721-42b3-966d-68eadf702b00 · inbound

Inferring the stochastic gravitational-wave background from eccentric stellar-mass binary black holes with spaceborne detectors cites this paper.

Inferring the stochastic gravitational-wave background from eccentric stellar-mass binary black holes with spaceborne detectors Merging black hole binaries with the SEVN code

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-04T07:36:40.105989Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T07:36:40.105989Z digest=sha256:2b009ef8a6d89d31a9aebbfcd65b10cd723cf8845ba07336e326bbf98eafae09

Observation e36f248c-04ed-4c7e-b604-ddbb9debf095 · inbound

Probing the origin of the kilonova candidate GRB 230307A: analysis of host galaxy and offset cites this paper.

Probing the origin of the kilonova candidate GRB 230307A: analysis of host galaxy and offset Merging black hole binaries with the SEVN code

Reference 62

Resolution
metadata mismatch
local_arxiv, observed 2026-05-16T23:28:40.109443Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b733d3027b562a6cbed4c9c0f0adcdb50a0961a44249a51ead09a84a8d4d7316

Observation 6e0fdefd-25a1-4bc6-8818-d8d3f75ea134 · inbound

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

Can current models predict the local black hole merger rate? Merging black hole binaries with the SEVN code

Reference 12

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:02:10.979062Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:522d98c256f32328fd49ff573d0a6d299d6f531edb86fb0f0f3aa043ea36910b

Observation 12e1ff2c-2589-4c10-93ec-17591fb22c5a · inbound

AGN-driven BBH mergers: Black hole populations and hierarchical growth across the AGN parameter space cites this paper.

AGN-driven BBH mergers: Black hole populations and hierarchical growth across the AGN parameter space Merging black hole binaries with the SEVN code

Reference 49

Resolution
verified exact
local_arxiv, observed 2026-06-27T13:20:57.488392Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:4c06831236a02193fc865bb63dd309147773a55a04dced30e1e3f444cf7e99d2

Observation e20daf90-0a78-405b-8cf5-b0ebbfdd5e42 · inbound

Lower Your Rates: On Claims of a Binary Black Hole Merger-Rate Crisis cites this paper.

Lower Your Rates: On Claims of a Binary Black Hole Merger-Rate Crisis Merging black hole binaries with the SEVN code

Reference 89

Resolution
verified exact
local_arxiv, observed 2026-06-30T01:14:08.106422Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8f794edb8c74499c2b400a97b257f4352505b192a7d7b711e0fd112550622528

Observation 5d60e7ae-d151-420d-941b-f2cf1312929a · inbound

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins cites this paper.

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins Merging black hole binaries with the SEVN code

Reference 194

Resolution
unresolved
no resolver link, observed 2026-07-11T06:51:42.465920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:51:42.465920Z digest=sha256:d77d95de25a0adc413fc761ea763d5c54dd591aee2e9a41a2285257684c404c5

Observation eae67920-db67-4feb-b16b-205d642d01f5 · inbound

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope cites this paper.

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope Merging black hole binaries with the SEVN code

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-01T09:38:54.213291Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T09:38:54.213291Z digest=sha256:583c448c3f843b1c73b142067089c147119e631cda430e3ccaf71343b2a0efc6