Paper Citation Record · LEDGER

Inferring the pair-instability mass gap from gravitational wave data

As of 14 August 2026, this Paper Citation Record lists 100 of 105 outbound references and 9 inbound Pith citation observations for arXiv:2506.09154.

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

pith.paper-citation-record.v1
2506.09154 v2

Coverage vector

measured 100 of 105 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:02:01.193648Z

measured 109 of 109 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T10:56:35.192287Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

100 of 105 outbound references displayed

verified exact6
verified fuzzy0
unresolved92
parse uncertain0
malformed identifier1
metadata mismatch1

External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation da9d1ef6-4854-4042-ad27-3b1619767213 · outbound

This paper cites As in Ref.

Inferring the pair-instability mass gap from gravitational wave data As in Ref

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.920153Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 56aec29c-05f7-4f19-ab79-af718bbfbb8b · outbound

This paper cites (12) in which the spin distri- bution at high masses is described via a GP prior: p(χeff | m1) = ( N (χeff ; µ, σ) m1 < ˜m eΘ(χeff )/ R 1 −1 eΘ(χeff ) dχeff m1 ≥ ˜m.

Inferring the pair-instability mass gap from gravitational wave data (12) in which the spin distri- bution at high masses is described via a GP prior: p(χeff | m1) = ( N (χeff ; µ, σ) m1 < ˜m eΘ(χeff )/ R 1 −1 eΘ(χeff ) dχeff m1 ≥ ˜m

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.924292Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1224b4ee-9e5b-4d4a-b3da-c4f7677f51a1 · outbound

This paper cites However, we observe no- ticeable differences in the lower5% credible bound out- side the range0 ≲ χeff ≲ 0.7, where Model 2 leads to sig- nificantly lower probability values.

Inferring the pair-instability mass gap from gravitational wave data However, we observe no- ticeable differences in the lower5% credible bound out- side the range0 ≲ χeff ≲ 0.7, where Model 2 leads to sig- nificantly lower probability values

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.926772Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3e0aef1b-06bd-4d90-9490-ffdeabd201b6 · outbound

This paper cites GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs.

Inferring the pair-instability mass gap from gravitational wave data GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.929817Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 99dec2e0-2f2a-480f-83bb-268cf73ea073 · outbound

This paper cites Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo.

Inferring the pair-instability mass gap from gravitational wave data Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.932394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fe7c1510-615b-4d03-a2fe-3c14abbac844 · outbound

This paper cites GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run.

Inferring the pair-instability mass gap from gravitational wave data GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.937197Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf90a48f-71d2-4379-9d3c-a69b006b9f5f · outbound

This paper cites GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run.

Inferring the pair-instability mass gap from gravitational wave data GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.940779Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 59ac6ca7-7865-4f5e-83e7-3168c69a76f4 · outbound

This paper cites Spera, M.

Inferring the pair-instability mass gap from gravitational wave data Spera, M

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.943539Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 467c58ec-eebf-4b97-917d-8d3c2864b93a · outbound

This paper cites The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars.

Inferring the pair-instability mass gap from gravitational wave data The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.945607Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b6c7ce45-a94e-4013-9291-faed04bf9c0f · outbound

This paper cites Stevenson, F.

Inferring the pair-instability mass gap from gravitational wave data Stevenson, F

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.948391Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ab471781-3ba8-434f-b552-2830a86febbb · outbound

This paper cites an unresolved cited work.

Inferring the pair-instability mass gap from gravitational wave data Unresolved cited work

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.950288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 442378e7-6a7f-4f7b-952f-c7134ac3bd99 · outbound

This paper cites Is GW190521 the merger of black holes from the first stellar generations?.

Inferring the pair-instability mass gap from gravitational wave data Is GW190521 the merger of black holes from the first stellar generations?

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.952127Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 324d3d82-eecd-4582-b611-3fda2e56c330 · outbound

This paper cites The Formation of a 70 Msun Black Hole at High Metallicity.

Inferring the pair-instability mass gap from gravitational wave data The Formation of a 70 Msun Black Hole at High Metallicity

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.954466Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 989bcc70-29b2-4d8a-9451-3de150f78714 · outbound

This paper cites Pulsational Pair-Instability Supernovae.

Inferring the pair-instability mass gap from gravitational wave data Pulsational Pair-Instability Supernovae

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.956697Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dd1f5034-b74f-4e3c-b739-1dc19084529c · outbound

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

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 31381fa0-2c4d-4523-8d37-e425f32830bd · outbound

This paper cites Pulsational pair-instability supernovae in gravitational-wave and electromagnetic transients.

Inferring the pair-instability mass gap from gravitational wave data Pulsational pair-instability supernovae in gravitational-wave and electromagnetic transients

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.963063Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation acddbc22-e457-4f64-961d-749bd4c2e92a · outbound

This paper cites Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap.

Inferring the pair-instability mass gap from gravitational wave data Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.965293Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f1d2191-80e2-469d-b874-34d47e2fdc53 · outbound

This paper cites Pulsational Pair-instability Supernovae. I. Pre-collapse Evolution and Pulsational Mass Ejection.

Inferring the pair-instability mass gap from gravitational wave data Pulsational Pair-instability Supernovae. I. Pre-collapse Evolution and Pulsational Mass Ejection

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.967436Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 26d1d626-ad6f-4bb7-be5d-6f58acfe8903 · outbound

This paper cites Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog.

Inferring the pair-instability mass gap from gravitational wave data Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.969583Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b9cb3d92-9a26-4ec2-97ba-fa2eb9b179e4 · outbound

This paper cites Poking Holes: Looking for Gaps in LIGO/Virgo's Black Hole Population.

Inferring the pair-instability mass gap from gravitational wave data Poking Holes: Looking for Gaps in LIGO/Virgo's Black Hole Population

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.971573Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f1366899-f082-41b1-95ca-bf6d46e8f657 · outbound

This paper cites Non-parametric inference of the population of compact binaries from gravitational wave observations using binned Gaussian processes.

Inferring the pair-instability mass gap from gravitational wave data Non-parametric inference of the population of compact binaries from gravitational wave observations using binned Gaussian processes

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.975743Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b8d5805d-f11a-4469-b6b0-3c3fbd5b3d7c · outbound

This paper cites A Parameter-Free Tour of the Binary Black Hole Population.

Inferring the pair-instability mass gap from gravitational wave data A Parameter-Free Tour of the Binary Black Hole Population

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.977796Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d5a8e5fb-f590-4bd9-beea-c1a1ab541c97 · outbound

This paper cites Resolving the Stellar-Collapse and Hierarchical-Merger origins of the Coalescing Black Holes.

Inferring the pair-instability mass gap from gravitational wave data Resolving the Stellar-Collapse and Hierarchical-Merger origins of the Coalescing Black Holes

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.979848Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3f89799f-0487-4b0f-a73c-0fd50c5aeeaf · outbound

This paper cites Predicting the Heaviest Black Holes below the Pair Instability Gap.

Inferring the pair-instability mass gap from gravitational wave data Predicting the Heaviest Black Holes below the Pair Instability Gap

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.982222Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c1ce929b-bb91-452e-9988-e3acc1e787d4 · outbound

This paper cites Binary Mergers and Growth of Black Holes in Dense Star Clusters.

Inferring the pair-instability mass gap from gravitational wave data Binary Mergers and Growth of Black Holes in Dense Star Clusters

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.984154Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b3593234-2daf-447b-b1b8-b75be5ae3e74 · outbound

This paper cites Merging black hole binaries in galactic nuclei: implications for advanced-LIGO detections.

Inferring the pair-instability mass gap from gravitational wave data Merging black hole binaries in galactic nuclei: implications for advanced-LIGO detections

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.986188Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e4a05084-9804-471d-8177-284f9889c75b · outbound

This paper cites an unresolved cited work.

Inferring the pair-instability mass gap from gravitational wave data Unresolved cited work

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.988273Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bec004d7-626b-40b3-8bb1-311e1ff1eec0 · outbound

This paper cites Are merging black holes born from stellar collapse or previous mergers?.

Inferring the pair-instability mass gap from gravitational wave data Are merging black holes born from stellar collapse or previous mergers?

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.990567Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bce0713f-edc3-48c8-a723-843f40c64daa · outbound

This paper cites Hierarchical Black Hole Mergers in Active Galactic Nuclei.

Inferring the pair-instability mass gap from gravitational wave data Hierarchical Black Hole Mergers in Active Galactic Nuclei

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.994097Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8a582e60-25a8-4319-9b9d-5722f150e54d · outbound

This paper cites Black hole growth through hierarchical black hole mergers in dense star clusters: implications for gravitational wave detections.

Inferring the pair-instability mass gap from gravitational wave data Black hole growth through hierarchical black hole mergers in dense star clusters: implications for gravitational wave detections

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:00.996180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f30c079f-eb06-4215-95a7-5e00b87e6052 · outbound

This paper cites Black hole mergers from quadruples.

Inferring the pair-instability mass gap from gravitational wave data Black hole mergers from quadruples

Reference 34

Resolution: verified exact; local_arxiv, observed 2026-08-07T05:02:01.700838Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation fcd888f4-613a-455e-ab98-48ec0f598091 · outbound

This paper cites GW190521 formation via three-body encounters in young massive star clusters.

Inferring the pair-instability mass gap from gravitational wave data GW190521 formation via three-body encounters in young massive star clusters

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-08-07T05:02:01.691778Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 21bdf240-ca56-4739-b599-e124958965f3 · outbound

This paper cites Hierarchical black hole mergers in young, globular and nuclear star clusters: the effect of metallicity, spin and cluster properties.

Inferring the pair-instability mass gap from gravitational wave data Hierarchical black hole mergers in young, globular and nuclear star clusters: the effect of metallicity, spin and cluster properties

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.002929Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0a84e43c-86e7-4105-bedc-ccaeebd35f02 · outbound

This paper cites Signatures of Hierarchical Mergers in Black Hole Spin and Mass distribution.

Inferring the pair-instability mass gap from gravitational wave data Signatures of Hierarchical Mergers in Black Hole Spin and Mass distribution

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.005513Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 60eacb51-78f1-4588-98e1-3140329f8eaf · outbound

This paper cites Are LIGO's Black Holes Made From Smaller Black Holes?.

Inferring the pair-instability mass gap from gravitational wave data Are LIGO's Black Holes Made From Smaller Black Holes?

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.008488Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7cb620f7-134e-4d77-b092-f7266d723567 · outbound

This paper cites The mass gap, the spin gap, and the origin of merging binary black holes.

Inferring the pair-instability mass gap from gravitational wave data The mass gap, the spin gap, and the origin of merging binary black holes

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.010785Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bd5d2365-14b4-49ed-89fd-934e99392285 · outbound

This paper cites Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins.

Inferring the pair-instability mass gap from gravitational wave data Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.012970Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8d2d25bb-a07f-4f4b-81d3-6fffc7e16b84 · outbound

This paper cites Vitale, R.

Inferring the pair-instability mass gap from gravitational wave data Vitale, R

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.015398Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a7328344-f5a1-49d6-ba53-077a27d03ebb · outbound

This paper cites an unresolved cited work.

Inferring the pair-instability mass gap from gravitational wave data Unresolved cited work

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.017172Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a47d4ef3-99f5-4033-9e7f-fa8adc8ce56a · outbound

This paper cites Searching for structure in the binary black hole spin distribution.

Inferring the pair-instability mass gap from gravitational wave data Searching for structure in the binary black hole spin distribution

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.019102Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9779dffc-6df0-4743-98bd-ed1c5e26c173 · outbound

This paper cites Use of gravitational waves to probe the formation channels of compact binaries.

Inferring the pair-instability mass gap from gravitational wave data Use of gravitational waves to probe the formation channels of compact binaries

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.021241Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4550a592-102c-4f67-82ea-1e479147c0f5 · outbound

This paper cites Illuminating Black Hole Binary Formation Channels with Spins in Advanced LIGO.

Inferring the pair-instability mass gap from gravitational wave data Illuminating Black Hole Binary Formation Channels with Spins in Advanced LIGO

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.023783Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8907b362-e161-4730-a728-3c86da1f4c15 · outbound

This paper cites Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter.

Inferring the pair-instability mass gap from gravitational wave data Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.025998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2f8e1c83-d3ba-48a8-86b2-4e6374ffce47 · outbound

This paper cites One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways.

Inferring the pair-instability mass gap from gravitational wave data One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.028079Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6efcf010-7623-4bec-9682-621cba55c380 · outbound

This paper cites Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures.

Inferring the pair-instability mass gap from gravitational wave data Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.030505Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ff15c954-99b6-4aba-9dcd-70cb3d154f70 · outbound

This paper cites Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins.

Inferring the pair-instability mass gap from gravitational wave data Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.032530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 71ab6b3a-1b75-436a-b90e-5e2ab4b925c1 · outbound

This paper cites No evidence that the majority of black holes in binaries have zero spin.

Inferring the pair-instability mass gap from gravitational wave data No evidence that the majority of black holes in binaries have zero spin

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.034693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0af1116f-2bd7-4df8-82f2-61da40597fd0 · outbound

This paper cites Four eccentric mergers increase the evidence that LIGO--Virgo--KAGRA's binary black holes form dynamically.

Inferring the pair-instability mass gap from gravitational wave data Four eccentric mergers increase the evidence that LIGO--Virgo--KAGRA's binary black holes form dynamically

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.036899Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b3270b7-1777-404d-a178-f0992de61afb · outbound

This paper cites Understanding how fast black holes spin by analysing data from the second gravitational-wave catalogue.

Inferring the pair-instability mass gap from gravitational wave data Understanding how fast black holes spin by analysing data from the second gravitational-wave catalogue

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.038924Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bd648264-b94d-414f-a101-bee066d2532e · outbound

This paper cites Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes.

Inferring the pair-instability mass gap from gravitational wave data Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.040952Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5ea1adfc-350b-4db3-ad6e-c8303a5981bc · outbound

This paper cites Black hole genealogy: Identifying hierarchical mergers with gravitational waves.

Inferring the pair-instability mass gap from gravitational wave data Black hole genealogy: Identifying hierarchical mergers with gravitational waves

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.043084Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation afb89d6a-6776-4e51-89ee-6be5a2299ca1 · outbound

This paper cites Hierarchical Black-Hole Mergers in Multiple Systems: Constrain the Formation of GW190412, GW190814 and GW190521-like events.

Inferring the pair-instability mass gap from gravitational wave data Hierarchical Black-Hole Mergers in Multiple Systems: Constrain the Formation of GW190412, GW190814 and GW190521-like events

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.045393Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 31eae621-823b-439a-aac0-65533c89cce2 · outbound

This paper cites Searching for mass-spin correlations in the population of gravitational-wave events: the GWTC-3 case study.

Inferring the pair-instability mass gap from gravitational wave data Searching for mass-spin correlations in the population of gravitational-wave events: the GWTC-3 case study

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.047344Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 698ae5a4-1111-4906-9224-743d5353e82c · outbound

This paper cites The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data.

Inferring the pair-instability mass gap from gravitational wave data The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.049503Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3c99eb45-dee0-4181-9793-a0e49ff5cb4d · outbound

This paper cites PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions.

Inferring the pair-instability mass gap from gravitational wave data PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.051564Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6611a1ad-02ea-44c6-8ea3-7d7230f0f912 · outbound

This paper cites Nonparametric analysis of correlations in the binary black hole population with LIGO-Virgo-KAGRA data.

Inferring the pair-instability mass gap from gravitational wave data Nonparametric analysis of correlations in the binary black hole population with LIGO-Virgo-KAGRA data

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.053570Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 83c2d1fa-1983-465b-a6bb-f21050fb6f10 · outbound

This paper cites A Star Cluster Population of High Mass Black Hole Mergers in Gravitational Wave Data.

Inferring the pair-instability mass gap from gravitational wave data A Star Cluster Population of High Mass Black Hole Mergers in Gravitational Wave Data

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.055568Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4c54097e-190d-4c48-9f09-bedd70cc1462 · outbound

This paper cites Looking for the parents of LIGO's black holes.

Inferring the pair-instability mass gap from gravitational wave data Looking for the parents of LIGO's black holes

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-08-07T05:02:01.545448Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation f3dea4b4-8e4a-4376-b64b-ff7fbe2ba093 · outbound

This paper cites Merging Black Holes in the Low-mass and High-mass Gaps from 2+2 Quadruple Systems.

Inferring the pair-instability mass gap from gravitational wave data Merging Black Holes in the Low-mass and High-mass Gaps from 2+2 Quadruple Systems

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-08-07T05:02:01.536895Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 04b1afd5-2e59-4d24-b3cf-031ca6b8fa8c · outbound

This paper cites Mass-gap Mergers in Active Galactic Nuclei.

Inferring the pair-instability mass gap from gravitational wave data Mass-gap Mergers in Active Galactic Nuclei

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.063499Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82246718-0f6b-4c0e-b319-c28f200c1568 · outbound

This paper cites an unresolved cited work.

Inferring the pair-instability mass gap from gravitational wave data Unresolved cited work

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.075700Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ae712f88-4640-4e9c-9674-842374334a69 · outbound

This paper cites Fishbach, D.

Inferring the pair-instability mass gap from gravitational wave data Fishbach, D

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.085171Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c378974-775b-48b4-b979-8cc0f0bdea6d · outbound

This paper cites Callister, M.

Inferring the pair-instability mass gap from gravitational wave data Callister, M

Reference 67

Resolution: malformed identifier; no resolver link, observed 2026-08-07T05:02:01.096161Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8203c282-050f-45ca-80f1-5b501f502322 · outbound

This paper cites Cosmic Cousins: Identification of a Subpopulation of Binary Black Holes Consistent with Isolated Binary Evolution.

Inferring the pair-instability mass gap from gravitational wave data Cosmic Cousins: Identification of a Subpopulation of Binary Black Holes Consistent with Isolated Binary Evolution

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.106576Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 06c71ef2-fbed-4bd2-8011-79e10f365792 · outbound

This paper cites an unresolved cited work.

Inferring the pair-instability mass gap from gravitational wave data Unresolved cited work

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.108886Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d634c03f-f9e1-4a51-a5b9-168e7b0a6272 · outbound

This paper cites Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei.

Inferring the pair-instability mass gap from gravitational wave data Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.110833Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 88ecc16e-95b3-42a9-85f5-215c0a4e1f7b · outbound

This paper cites Sadiq, T.

Inferring the pair-instability mass gap from gravitational wave data Sadiq, T

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.113195Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 440237e4-df85-47fe-b5de-e40dd3a29811 · outbound

This paper cites The binary black hole spin distribution likely broadens with redshift.

Inferring the pair-instability mass gap from gravitational wave data The binary black hole spin distribution likely broadens with redshift

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.115118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 407d28e4-b52a-440b-9f5d-32ab875d0903 · outbound

This paper cites Probing Correlations in the Binary Black Hole Population with Flexible Models.

Inferring the pair-instability mass gap from gravitational wave data Probing Correlations in the Binary Black Hole Population with Flexible Models

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.117192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1c98047d-da37-4e67-9cc5-774d0b5b5f18 · outbound

This paper cites The population of merging compact binaries inferred using gravitational waves through GWTC-3.

Inferring the pair-instability mass gap from gravitational wave data The population of merging compact binaries inferred using gravitational waves through GWTC-3

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.119326Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 25e56cfa-c559-4d23-9b81-d6a4f8ba5d85 · outbound

This paper cites Revealing the $\chi_{\rm eff}$-$q$ Correlation among Coalescing Binary Black Holes and Tentative Evidence for AGN-driven Hierarchical Mergers.

Inferring the pair-instability mass gap from gravitational wave data Revealing the $\chi_{\rm eff}$-$q$ Correlation among Coalescing Binary Black Holes and Tentative Evidence for AGN-driven Hierarchical Mergers

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.122106Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 77e44b82-0d89-4ce3-b331-2a9ad0887460 · outbound

This paper cites Hut, Astronomy and Astrophysics (1981), URL http://adsabs.harvard.edu/full/1981A&A....99.

Inferring the pair-instability mass gap from gravitational wave data Hut, Astronomy and Astrophysics (1981), URL http://adsabs.harvard.edu/full/1981A&A....99

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.124303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 94f0410c-3e0f-4c27-bfc3-a8b560c6a84d · outbound

This paper cites Bimodal black-hole mass distribution and chirp masses of binary black-hole mergers.

Inferring the pair-instability mass gap from gravitational wave data Bimodal black-hole mass distribution and chirp masses of binary black-hole mergers

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.126510Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 212b043f-0510-4ad8-a818-62f4d1010b5c · outbound

This paper cites Binary Black Holes in Dense Star Clusters: Exploring the Theoretical Uncertainties.

Inferring the pair-instability mass gap from gravitational wave data Binary Black Holes in Dense Star Clusters: Exploring the Theoretical Uncertainties

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.128607Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f8646396-fb65-4ef6-81cc-71b23ae5184e · outbound

This paper cites Post-Newtonian Dynamics in Dense Star Clusters: Highly-Eccentric, Highly-Spinning, and Repeated Binary Black Hole Mergers.

Inferring the pair-instability mass gap from gravitational wave data Post-Newtonian Dynamics in Dense Star Clusters: Highly-Eccentric, Highly-Spinning, and Repeated Binary Black Hole Mergers

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.131570Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 101f9bc3-22dd-4214-866d-fab91c92debd · outbound

This paper cites Stellar Black Hole Binary Mergers in Open Clusters.

Inferring the pair-instability mass gap from gravitational wave data Stellar Black Hole Binary Mergers in Open Clusters

Reference 80

Resolution: verified exact; local_arxiv, observed 2026-08-07T05:02:01.414861Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 06936af4-17ef-43ea-b8f3-1134371f5e32 · outbound

This paper cites Intermediate mass black holes from stellar mergers in young star clusters.

Inferring the pair-instability mass gap from gravitational wave data Intermediate mass black holes from stellar mergers in young star clusters

Reference 81

Resolution: verified exact; local_arxiv, observed 2026-08-07T05:02:01.405146Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation be1071af-6576-4ff0-9cf2-e900b4d874d3 · outbound

This paper cites Stellar-mass black holes in young massive and open stellar clusters V: comparisons with LIGO-Virgo merger rate densities.

Inferring the pair-instability mass gap from gravitational wave data Stellar-mass black holes in young massive and open stellar clusters V: comparisons with LIGO-Virgo merger rate densities

Reference 82

Resolution: metadata mismatch; local_arxiv, observed 2026-08-07T05:02:01.392846Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation f18f93ed-155a-4511-bf25-31a3eae11561 · outbound

This paper cites Population synthesis of black hole binary mergers from star clusters.

Inferring the pair-instability mass gap from gravitational wave data Population synthesis of black hole binary mergers from star clusters

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.142155Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation efcf542a-c391-4d7b-969d-04a3454f3689 · outbound

This paper cites Coalescing black hole binaries from globular clusters: mass distributions and comparison to gravitational wave data from GWTC-3.

Inferring the pair-instability mass gap from gravitational wave data Coalescing black hole binaries from globular clusters: mass distributions and comparison to gravitational wave data from GWTC-3

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.144730Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1cc67ba1-526e-4ff9-afbb-b2e6f6d06e91 · outbound

This paper cites Constraining the LIGO/Virgo AGN channel with black hole spins.

Inferring the pair-instability mass gap from gravitational wave data Constraining the LIGO/Virgo AGN channel with black hole spins

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.146854Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 20b4db85-9f18-4ac7-a75c-04dcc4f8413f · outbound

This paper cites Mandel, MNRAS456, 578 (2016).

Inferring the pair-instability mass gap from gravitational wave data Mandel, MNRAS456, 578 (2016)

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.148749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 762385e9-1873-44c7-8f71-f35690167b70 · outbound

This paper cites Most Black Holes are Born Very Slowly Rotating.

Inferring the pair-instability mass gap from gravitational wave data Most Black Holes are Born Very Slowly Rotating

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.151490Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c38b559f-13ea-426d-93a8-b256c0c2f057 · outbound

This paper cites Chemically Homogeneous Evolution: A rapid population synthesis approach.

Inferring the pair-instability mass gap from gravitational wave data Chemically Homogeneous Evolution: A rapid population synthesis approach

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.154891Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 704e3b52-c5c1-4f82-87e0-ebf524412e7d · outbound

This paper cites Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations.

Inferring the pair-instability mass gap from gravitational wave data Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.157340Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d73c62a0-3b05-4e3e-9cef-aaa15b3c5c16 · outbound

This paper cites Spinning spectral sirens: Robust cosmological measurement using mass-spin correlations in the binary black hole population.

Inferring the pair-instability mass gap from gravitational wave data Spinning spectral sirens: Robust cosmological measurement using mass-spin correlations in the binary black hole population

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.160006Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 512a9b00-abed-4730-8dd2-02eadb75a79a · outbound

This paper cites The Effect of Pair-Instability Mass Loss on Black Hole Mergers.

Inferring the pair-instability mass gap from gravitational wave data The Effect of Pair-Instability Mass Loss on Black Hole Mergers

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.162353Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5652980e-19b7-424f-9d2c-8a349025064e · outbound

This paper cites Constraints from gravitational wave detections of binary black hole mergers on the $^{12}\rm{C}\left(\alpha,\gamma\right)^{16}\!\rm{O}$ rate.

Inferring the pair-instability mass gap from gravitational wave data Constraints from gravitational wave detections of binary black hole mergers on the $^{12}\rm{C}\left(\alpha,\gamma\right)^{16}\!\rm{O}$ rate

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.164536Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 265df369-3402-4141-893b-107c93c969b6 · outbound

This paper cites an unresolved cited work.

Inferring the pair-instability mass gap from gravitational wave data Unresolved cited work

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.166758Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1c7facd2-1506-4d74-8605-3d8d56cda698 · outbound

This paper cites The impact of stellar rotation on the black hole mass-gap from pair-instability supernovae.

Inferring the pair-instability mass gap from gravitational wave data The impact of stellar rotation on the black hole mass-gap from pair-instability supernovae

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.168540Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6096db00-7b90-4be8-b8c9-609e021bcdc8 · outbound

This paper cites The Pair-Instability Mass Gap for Black Holes.

Inferring the pair-instability mass gap from gravitational wave data The Pair-Instability Mass Gap for Black Holes

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.171263Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1cc2c7a1-5df8-415d-81bd-69179f58d3d1 · outbound

This paper cites Pulsational pair-instability supernovae in very close binaries.

Inferring the pair-instability mass gap from gravitational wave data Pulsational pair-instability supernovae in very close binaries

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.174193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e8b74a53-fb93-48db-babe-2d2cab4cf47b · outbound

This paper cites Greenfield, T.

Inferring the pair-instability mass gap from gravitational wave data Greenfield, T

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.176385Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 88cad857-7b17-4d4f-b279-a43609d6ab4b · outbound

This paper cites Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy.

Inferring the pair-instability mass gap from gravitational wave data Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.178364Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cb91650f-7137-4397-b985-685441fee128 · outbound

This paper cites Bradbury, R.

Inferring the pair-instability mass gap from gravitational wave data Bradbury, R

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.180785Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c1057258-f214-42c4-9375-dacc086d12bc · outbound

This paper cites Array Programming with NumPy.

Inferring the pair-instability mass gap from gravitational wave data Array Programming with NumPy

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.183521Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c0439da6-dbd6-49b3-b403-4b4520d5e7a3 · outbound

This paper cites Composable Effects for Flexible and Accelerated Probabilistic Programming in NumPyro.

Inferring the pair-instability mass gap from gravitational wave data Composable Effects for Flexible and Accelerated Probabilistic Programming in NumPyro

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.186032Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b1b29b3-a986-47ad-a473-d6f3f416798f · outbound

This paper cites Bingham, J.

Inferring the pair-instability mass gap from gravitational wave data Bingham, J

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.188315Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8c18e20d-4092-428f-b0e1-2a2d5d4fa373 · outbound

This paper cites Virtanen, R.

Inferring the pair-instability mass gap from gravitational wave data Virtanen, R

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.190993Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1c529f5b-189b-4b59-97d7-4d2daa4dc9f4 · outbound

This paper cites The Emergence of Structure in the Binary Black Hole Mass Distribution.

Inferring the pair-instability mass gap from gravitational wave data The Emergence of Structure in the Binary Black Hole Mass Distribution

Reference 104

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.193648Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation a71130ed-477e-42ff-b64b-150540bacb6f · inbound

Spectral siren cosmology from gravitational-wave observations in GWTC-4.0 cites this paper.

Spectral siren cosmology from gravitational-wave observations in GWTC-4.0 Inferring the pair-instability mass gap from gravitational wave data

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-05T10:56:35.192287Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 25010a56-5226-4ea4-a5dc-75961afb9ddc · inbound

Evidence of the pair instability gap from black hole masses cites this paper.

Evidence of the pair instability gap from black hole masses Inferring the pair-instability mass gap from gravitational wave data

Reference 31

Resolution: verified exact; arxiv_id, observed 2026-05-18T19:22:49.195453Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation e410493d-247f-4feb-ab8c-deec4df2f7a5 · 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 Inferring the pair-instability mass gap from gravitational wave data

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-04T19:47:52.091394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d5ab4023-e073-4326-9d77-dd5967df0fb3 · inbound

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset cites this paper.

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset Inferring the pair-instability mass gap from gravitational wave data

Reference 89

Resolution: verified exact; arxiv_id, observed 2026-05-09T02:57:53.095035Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 2b8c62bd-29cf-4621-b841-0b446af4ad85 · inbound

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset cites this paper.

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset Inferring the pair-instability mass gap from gravitational wave data

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-03T11:02:35.648146Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b7892f90-5d5a-40e5-9935-670009e7804d · 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 Inferring the pair-instability mass gap from gravitational wave data

Reference 55

Resolution: verified exact; arxiv_id, observed 2026-05-16T05:37:23.691381Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation bb34b9cf-632f-42cd-9cd4-26a327530550 · 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 Inferring the pair-instability mass gap from gravitational wave data

Reference 76

Resolution: verified exact; arxiv_id, observed 2026-05-11T06:11:02.315103Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 439162b0-b5dd-442e-b891-9ab4f6495cb5 · inbound

How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4 cites this paper.

How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4 Inferring the pair-instability mass gap from gravitational wave data

Reference 91

Resolution: metadata mismatch; arxiv_id, observed 2026-05-08T23:14:24.766179Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation ecbdeaf8-4bf9-498d-9e1f-1441bec8ee7a · inbound

Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 cites this paper.

Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 Inferring the pair-instability mass gap from gravitational wave data

Reference 62

Resolution: verified exact; arxiv_id, observed 2026-07-03T12:58:07.781761Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.