Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\odot}$ from gravitational-wave observations
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2407.02460.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T05:06:55.350988Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-06-30T14:34:46.225574Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- unresolved0
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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 d48ee494-df45-4540-a866-5e2f7f9deaf4 · inbound
Using gravitational waves and multi-messenger Astronomy to reverse-engineer the properties of galactic nuclei cites this paper.
Using gravitational waves and multi-messenger Astronomy to reverse-engineer the properties of galactic nuclei A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\odot}$ from gravitational-wave observations
Reference 96
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T05:06:55.350988Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b7068314-d82d-4c91-9f99-c7e5c3a1e91e · inbound
Measurement prospects for the pair-instability mass cutoff with gravitational waves cites this paper.
Measurement prospects for the pair-instability mass cutoff with gravitational waves A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\odot}$ from gravitational-wave observations
Reference 103
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T05:37:23.696244Z
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.
Observation 5f53601f-478c-4f02-aefa-1638436931d5 · inbound
Emergent structure in the binary black hole mass distribution and implications for population-based cosmology cites this paper.
Emergent structure in the binary black hole mass distribution and implications for population-based cosmology A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\odot}$ from gravitational-wave observations
Reference 27
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-11T11:51:01.348342Z
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.
Observation 6c8a30aa-54da-4643-a322-b3eb5693f658 · inbound
Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation cites this paper.
Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\odot}$ from gravitational-wave observations
Reference 89
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T14:34:46.226852Z
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.
Observation ba274446-4089-4d1f-9689-9c46facc58e5 · inbound
High-mass binary black hole mergers from detailed binary evolution models cites this paper.
High-mass binary black hole mergers from detailed binary evolution models A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\odot}$ from gravitational-wave observations
Reference 76
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T22:07:32.529082Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.