Paper Citation Record · LEDGER

Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 15 inbound Pith citation observations for arXiv:1706.06109.

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

pith.paper-citation-record.v1
1706.06109 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 15 of 15 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 15 of 15 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:02:00.958706Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T17:55:20.774037Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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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 0f091ad5-39fe-4a2a-9d0c-2b3ade91678e · inbound

GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run cites this paper.

GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 202

Resolution: verified exact; local_arxiv, observed 2026-05-16T07:47:32.863402Z

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 dd1f5034-b74f-4e3c-b739-1dc19084529c · inbound

Inferring the pair-instability mass gap from gravitational wave data cites this paper.

Inferring the pair-instability mass gap from gravitational wave data Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.958706Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2dc0ddac-5d42-4ad5-b95a-f2568e8c2afa · inbound

Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars cites this paper.

Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 25

Resolution: verified exact; doi, observed 2026-05-09T02:16:30.201309Z

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 386856c0-a73c-4b4d-a436-eaf3e6974182 · inbound

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap cites this paper.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-04T19:47:51.950204Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 49884e5c-a1db-4361-a0df-46df6fc1ea7c · inbound

A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff cites this paper.

A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-05-22T12:41:33.295210Z

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 02a5c46c-4f86-45fc-8e18-e72fbe9dc1ea · inbound

A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff cites this paper.

A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-04T08:07:38.691182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0abfc9d2-47d6-4584-9405-53606708e297 · inbound

Searching for binary black hole mergers with deep learning in Advanced LIGO's third observing run cites this paper.

Searching for binary black hole mergers with deep learning in Advanced LIGO's third observing run Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 106

Resolution: unresolved; no resolver link, observed 2026-08-03T18:39:21.092598Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 074b1f43-d6c9-47b1-8c64-d0d460d82fbf · inbound

Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters cites this paper.

Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-11T06:11:02.212264Z

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 2f6d047b-ef7e-4212-aaa5-c12f1e928231 · inbound

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions cites this paper.

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 168

Resolution: verified exact; local_arxiv, observed 2026-05-22T09:31:21.729944Z

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 46a8779c-7118-4ed4-8a9d-9dead0955da8 · inbound

Predicting intermediate-mass black hole formation in star clusters with machine learning cites this paper.

Predicting intermediate-mass black hole formation in star clusters with machine learning Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 67

Resolution: verified exact; local_arxiv, observed 2026-05-22T09:21:21.101861Z

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 1155f2e9-b0b3-49e1-9dd7-1418ea197ac4 · inbound

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

Can current models predict the local black hole merger rate? Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 11

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.942173Z

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 596af33c-61da-4492-96c2-1cd2590ff709 · 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 Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 48

Resolution: verified exact; local_arxiv, observed 2026-06-27T13:30:57.122955Z

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 9929fee8-38be-48d5-b28e-e1d3cd899178 · 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 Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 228

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e665d374-8a1c-4b98-a8c3-e817006e1266 · inbound

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap cites this paper.

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-07-08T17:55:20.775544Z

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 e5271d8b-b8c4-445a-adb6-91cda226e4b0 · inbound

A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations cites this paper.

A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 71

Resolution: unresolved; no resolver link, observed 2026-07-31T01:54:12.323690Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.