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Paper Citation Record · LEDGER

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap

As of 11 August 2026, this Paper Citation Record lists 84 of 84 outbound references and 18 inbound Pith citation observations for arXiv:2509.09123.

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

pith.paper-citation-record.v1
2509.09123 v1

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measured 84 of 84 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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

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Outbound references

Observation 80dcd77b-0534-4c9d-8cab-2ca93d0e203c · outbound

This paper cites Nature Rev.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Nature Rev

Reference 1

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Observation 9900c1dd-7320-4d27-9d7c-c62559a24ec7 · outbound

This paper cites Gravitational Wave Physics and Astronomy in the nascent era.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Gravitational Wave Physics and Astronomy in the nascent era

Reference 2

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Observation f6b54dfd-0c9b-4131-9280-81347e16451f · outbound

This paper cites https://doi.org/10.1007/978-981-15-4702-7 16-1.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap https://doi.org/10.1007/978-981-15-4702-7 16-1

Reference 3

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Observation 22593605-45b7-4f5a-9d6f-edcc337e7253 · outbound

This paper cites Compact object mergers: exploring uncertainties from stellar and binary evolution with SEVN.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Compact object mergers: exploring uncertainties from stellar and binary evolution with SEVN

Reference 4

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Observation 45346953-ee32-43bc-8b4d-ad3b3a816cc3 · outbound

This paper cites Accuracy of inference on the physics of binary evolution from gravitational-wave observations.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Accuracy of inference on the physics of binary evolution from gravitational-wave observations

Reference 5

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Observation e6f28ff2-513b-4dd7-9994-42329b76c928 · outbound

This paper cites Double Compact Objects I: The Significance Of The Common Envelope On Merger Rates.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Double Compact Objects I: The Significance Of The Common Envelope On Merger Rates

Reference 6

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Observation 2e5c04bb-58c6-4b33-9684-ff2459019d8f · outbound

This paper cites The Mass Distribution of Stellar Black Holes.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The Mass Distribution of Stellar Black Holes

Reference 7

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Observation d0f3597b-6698-4b18-8841-dbb4e083029c · outbound

This paper cites Binary Black Hole Mergers in the first Advanced LIGO Observing Run.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Binary Black Hole Mergers in the first Advanced LIGO Observing Run

Reference 8

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Observation 25f10a0c-b928-4fb0-be26-9ba6b59b585d · outbound

This paper cites Advanced Virgo: a 2nd generation interferometric gravitational wave detector.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Advanced Virgo: a 2nd generation interferometric gravitational wave detector

Reference 9

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Observation 133d0ba1-1bd3-4db5-9db2-c59c32060fe9 · outbound

This paper cites PTEP2021(5), 05–101 (2021) https://doi.org/10.1093/ptep/ptaa125 arXiv:2005.05574 [physics.ins-det].

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap PTEP2021(5), 05–101 (2021) https://doi.org/10.1093/ptep/ptaa125 arXiv:2005.05574 [physics.ins-det]

Reference 10

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Observation ddecd91e-53bb-4fc2-ae01-b9ad765d4cff · 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.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

Reference 11

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Observation 743c0019-f5ae-453e-a8ca-356fae33e711 · outbound

This paper cites Observation of Gravitational Waves from a Binary Black Hole Merger.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Observation of Gravitational Waves from a Binary Black Hole Merger

Reference 12

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Observation 43d48c64-2cc6-4970-a163-7b1f24273f86 · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The population of merging compact binaries inferred using gravitational waves through GWTC-3

Reference 13

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Observation 1955e853-4536-4459-ac40-5370ea35d730 · outbound

This paper cites New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries

Reference 14

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Observation a53dfbd7-4ce6-4c57-93d3-1606370e6aee · outbound

This paper cites Searching for a subpopulation of primordial black holes in LIGO/Virgo gravitational-wave data.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Searching for a subpopulation of primordial black holes in LIGO/Virgo gravitational-wave data

Reference 15

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Observation a6fcba2f-7d1e-4dfa-89a2-acef8c57b698 · outbound

This paper cites What You Don't Know Can Hurt You: Use and Abuse of Astrophysical Models in Gravitational-wave Population Analyses.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap What You Don't Know Can Hurt You: Use and Abuse of Astrophysical Models in Gravitational-wave Population Analyses

Reference 16

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Observation fdff9618-92bc-4846-934d-73ec7071d021 · outbound

This paper cites Classifying the generation and formation channels of individual LIGO-Virgo-KAGRA observations from dynamically formed binaries.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Classifying the generation and formation channels of individual LIGO-Virgo-KAGRA observations from dynamically formed binaries

Reference 17

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Observation 0a42f1ab-e358-477c-b207-a305d3e9a39b · outbound

This paper cites Backward Population Synthesis: Mapping the Evolutionary History of Gravitational-Wave Progenitors.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Backward Population Synthesis: Mapping the Evolutionary History of Gravitational-Wave Progenitors

Reference 18

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Observation 27cd234e-fc0b-495f-9701-89e8425ca3ca · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The Emergence of Structure in the Binary Black Hole Mass Distribution

Reference 19

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Observation 4676daa4-60d8-4b0b-a146-c456b6a2af84 · outbound

This paper cites Exploring Features in the Binary Black Hole Population.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Exploring Features in the Binary Black Hole Population

Reference 20

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Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Unresolved cited work

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Observation 53937df6-a3c1-43fa-8e05-1c176822f0c4 · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Black hole genealogy: Identifying hierarchical mergers with gravitational waves

Reference 22

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Observation a56216ea-d4cf-46b1-aa3d-07fab2c6b5b5 · outbound

This paper cites Evidence for hierarchical black hole mergers in the second LIGO--Virgo gravitational-wave catalog.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Evidence for hierarchical black hole mergers in the second LIGO--Virgo gravitational-wave catalog

Reference 23

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This paper cites Phase Space of Binary Black Holes from Gravitational Wave Observations to Unveil its Formation History.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Phase Space of Binary Black Holes from Gravitational Wave Observations to Unveil its Formation History

Reference 24

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Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Unresolved cited work

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This paper cites Mergers of Stellar-Mass Black Holes in Nuclear Star Clusters.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Mergers of Stellar-Mass Black Holes in Nuclear Star Clusters

Reference 26

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This paper cites Monthly Notices of the Royal Astro- nomical Society402(1), 371–380 (2010) https://doi.org/10.1111/j.1365-2966.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Monthly Notices of the Royal Astro- nomical Society402(1), 371–380 (2010) https://doi.org/10.1111/j.1365-2966

Reference 27

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This paper cites Physical Review D89(6), 064007 (2014) https://doi.org/10.1103/PhysRevD.89.064007.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Physical Review D89(6), 064007 (2014) https://doi.org/10.1103/PhysRevD.89.064007

Reference 28

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This paper cites Demographics of Hierarchical Black Hole Mergers in Dense Star Clusters.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Demographics of Hierarchical Black Hole Mergers in Dense Star Clusters

Reference 29

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This paper cites Physical Review D93(8), 084029 (2016) https://doi.org/10.1103/PhysRevD.93.084029.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Physical Review D93(8), 084029 (2016) https://doi.org/10.1103/PhysRevD.93.084029

Reference 30

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This paper cites The Astrophysical Journal910(2), 14 (2021) https://doi.org/10.3847/2041-8213/ac0ea7.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The Astrophysical Journal910(2), 14 (2021) https://doi.org/10.3847/2041-8213/ac0ea7

Reference 31

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This paper cites Did LIGO detect dark matter?.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Did LIGO detect dark matter?

Reference 32

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This paper cites The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO

Reference 33

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This paper cites Primordial Black Hole Scenario for the Gravitational-Wave Event GW150914.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Primordial Black Hole Scenario for the Gravitational-Wave Event GW150914

Reference 34

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This paper cites Popular Astronomy22, 275–294 (1914).

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Popular Astronomy22, 275–294 (1914)

Reference 35

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source=pdf_text observed=2026-08-04T19:47:51.922194Z digest=sha256:b10e1d5e3d80c9a59bd375378d81accf593f5903c2af60c4c9ed0cf8b636af41

Observation 05f3159d-4e69-40f0-ae39-3eb47e08d938 · outbound

This paper cites The slope of the black-hole mass versus velocity dispersion correlation.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The slope of the black-hole mass versus velocity dispersion correlation

Reference 36

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source=pdf_text observed=2026-08-04T19:47:51.926010Z digest=sha256:89f97ae7a6c29067c5a231dc61585ddf137776500756d6d8b1ec926abea9bea1

Observation 1d4c2289-4bf8-4bec-9932-a2920aa614dd · outbound

This paper cites Phase transitions in neutron stars and their links to gravitational waves.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Phase transitions in neutron stars and their links to gravitational waves

Reference 37

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source=pdf_text observed=2026-08-04T19:47:51.929990Z digest=sha256:6684df3318fd3b5dc94d9fedfc9994144295f41d9efcc8b530bf0f0035a71482

Observation f49406c4-40f0-4b44-8a8a-95b851f88fb4 · outbound

This paper cites GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run

Reference 38

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source=pdf_text observed=2026-08-04T19:47:51.934118Z digest=sha256:942da2c33b3d54a568f449421b738a50d6e89e5a6539c9523044de60c1e2d899

Observation c9f21c4e-3bd8-4453-b9c7-b24dcfcddfc2 · outbound

This paper cites GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Reference 39

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source=pdf_text observed=2026-08-04T19:47:51.937961Z digest=sha256:295012841e4b6ff4e14b4854092869d5e3cce68cd3409a8693eeecfd8bb2e289

Observation 9e8cc2e5-7837-4a8d-b64b-34ef487fdd37 · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Is GW190521 the merger of black holes from the first stellar generations?

Reference 40

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source=pdf_text observed=2026-08-04T19:47:51.942047Z digest=sha256:5edb2edd0e6cde0eb1f3445296bcdec2fceab5c0752ff929e05587f1f45fae83

Observation de08c87d-415e-43e6-88d5-67e5b9b2966b · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The Formation of a 70 Msun Black Hole at High Metallicity

Reference 41

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source=pdf_text observed=2026-08-04T19:47:51.946146Z digest=sha256:b242e6dd85f2f84c144d8e53c806442cef8b3a70a2364dfe219885d4a0913c6b

Observation 386856c0-a73c-4b4d-a436-eaf3e6974182 · outbound

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

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

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source=pdf_text observed=2026-08-04T19:47:51.950204Z digest=sha256:e58f1c010f8ae67f3f8d217769aeeaac8866db19a3277a523e5640aaf9768ef0

Observation 75c9e55f-6115-4981-98a5-d75a798f124e · 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.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Constraints from gravitational wave detections of binary black hole mergers on the $^{12}\rm{C}\left(\alpha,\gamma\right)^{16}\!\rm{O}$ rate

Reference 43

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source=pdf_text observed=2026-08-04T19:47:51.954177Z digest=sha256:74282c27189216ec7b0dd5d427b1aeead214520f23402f1aa5e51899a662d7c4

Observation ef145909-eeb7-429d-8861-2cb35d01bd0c · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Pulsational pair-instability supernovae in gravitational-wave and electromagnetic transients

Reference 44

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source=pdf_text observed=2026-08-04T19:47:51.958065Z digest=sha256:144cb898469bcbc96a5b02683e7f7a861ba18839e5fc7ad164a12196a8a77a8e

Observation 5a64845a-c003-4350-ae14-0fcdd3395a7b · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap

Reference 45

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source=pdf_text observed=2026-08-04T19:47:51.961931Z digest=sha256:f2807cc53e61c014160a91e98f6bf56747d455a89cca9b2506e12c0cbfe165ad

Observation 45ea2100-eab5-42ed-8e4d-efd8f8a53eb5 · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Pulsational Pair-instability Supernovae. I. Pre-collapse Evolution and Pulsational Mass Ejection

Reference 46

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source=pdf_text observed=2026-08-04T19:47:51.965507Z digest=sha256:1dd83175b7cf9c3af70eb1dbc2c8b6f6a68cc509b18f584394bbafb4bfe47e80

Observation 25d88274-dec9-4876-bc5e-c39a0ddc300a · outbound

This paper cites The Maximum Black Hole Mass at Solar Metallicity.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The Maximum Black Hole Mass at Solar Metallicity

Reference 47

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source=pdf_text observed=2026-08-04T19:47:51.969177Z digest=sha256:76888db2a7841de4a1a63debbc5e7bbf5c32d27b4471b685006b91fa9e170a6f

Observation 6eca2ac8-dbd4-4d0f-98fa-f2beb27fd2b2 · outbound

This paper cites an unresolved cited work.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Unresolved cited work

Reference 48

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source=pdf_text observed=2026-08-04T19:47:51.972829Z digest=sha256:885a68b10a45fa6460cccef72dd0a175b4254aff961f836d71f91a316721706b

Observation a3a577ef-81b8-4b5b-b05a-0863cbc7846c · outbound

This paper cites Merging stellar-mass binary black holes.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Merging stellar-mass binary black holes

Reference 49

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source=pdf_text observed=2026-08-04T19:47:51.976540Z digest=sha256:d6751cc5868ca1928777976b7cbd069f33df5b2e014f4a705710fa59b0caa586

Observation 7aea52e8-ec14-46cb-9cd3-3decf13a319d · outbound

This paper cites The role of mass transfer and common envelope evolution in the formation of merging binary black holes.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The role of mass transfer and common envelope evolution in the formation of merging binary black holes

Reference 50

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source=pdf_text observed=2026-08-04T19:47:51.980255Z digest=sha256:d613983d1d0771841e5cdf1314da1bd55098152f7d644cbc4635f1d534c72b53

Observation 6ee59522-d896-4b3a-a96d-c3566affb1e2 · outbound

This paper cites The impact of mass-transfer physics on the observable properties of field binary black hole populations.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The impact of mass-transfer physics on the observable properties of field binary black hole populations

Reference 51

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source=pdf_text observed=2026-08-04T19:47:51.983838Z digest=sha256:ce278a81afa0003429bf2373f622d4a2d6deeff56d165864dc2d5163ad3a9e4a

Observation 1583047e-68c0-409a-ae61-045289357793 · outbound

This paper cites The origin of spin in binary black holes: Predicting the distributions of the main observables of Advanced LIGO.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The origin of spin in binary black holes: Predicting the distributions of the main observables of Advanced LIGO

Reference 52

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source=pdf_text observed=2026-08-04T19:47:51.987561Z digest=sha256:d5a595bf82590cbd06bf9f8d15c65a8eb4f53e1efe3164bad1dc45d6979c44ea

Observation b36d602c-b8ed-406c-9887-164a50b4b4c0 · outbound

This paper cites Cosmic Star Formation History.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Cosmic Star Formation History

Reference 53

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source=pdf_text observed=2026-08-04T19:47:51.991379Z digest=sha256:9f5374b4947a9419abaa4be9faff3a9a332601d644a2b127d07775bb9c750e14

Observation 4104f915-7741-49c8-ba5c-e726a034f5a5 · outbound

This paper cites Double Compact Objects III: Gravitational Wave Detection Rates.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Double Compact Objects III: Gravitational Wave Detection Rates

Reference 54

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no resolver link, observed 2026-08-04T19:47:51.995115Z

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source=pdf_text observed=2026-08-04T19:47:51.995115Z digest=sha256:d06df1bfaf76b9898e9975a58bd131a916336506b51b6b981c7b9cc149c228ad

Observation e8c5d491-218b-4f34-a753-99665f1a1558 · outbound

This paper cites GWSim: Python package for creating mock GW samples for different astrophysical populations and cosmological models of binary black holes.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap GWSim: Python package for creating mock GW samples for different astrophysical populations and cosmological models of binary black holes

Reference 55

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source=pdf_text observed=2026-08-04T19:47:51.999241Z digest=sha256:748338ce5441917577a2ad3d66812281d43c635fb8412af540c9bb9714733345

Observation 12fc7bc1-2bbf-4acd-90a1-f2f5e1844222 · outbound

This paper cites The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?

Reference 56

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source=pdf_text observed=2026-08-04T19:47:52.003346Z digest=sha256:3c0b68aa9b5d256196a5efd1944ef0b567fd9c0ff85dd85beef88de07b730af1

Observation 14b45dc9-68dc-4ff9-b5c1-c8eebd300560 · outbound

This paper cites Binary black holes population and cosmology in new lights: Signature of PISN mass and formation channel in GWTC-3.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Binary black holes population and cosmology in new lights: Signature of PISN mass and formation channel in GWTC-3

Reference 57

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source=pdf_text observed=2026-08-04T19:47:52.007821Z digest=sha256:4a4b6839888db756e7f3b0e598f4e0b8dba5b1a3a71ba1bc1eb9e314855b31a6

Observation 672521bf-e554-456c-a467-795dd80725c8 · outbound

This paper cites GWTC-4.0: Population Properties of Merging Compact Binaries.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap GWTC-4.0: Population Properties of Merging Compact Binaries

Reference 58

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source=pdf_text observed=2026-08-04T19:47:52.011712Z digest=sha256:3c00814473be8e391380e7a4e1673fd36647b68c5d55622ceae5f671dba747e2

Observation 73e78e84-903d-4af9-93e2-91c34c04eba6 · outbound

This paper cites an unresolved cited work.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Unresolved cited work

Reference 59

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source=pdf_text observed=2026-08-04T19:47:52.015652Z digest=sha256:c6fa0b56ecbd887a6b4fc07530d04b4eff40fd331158a8fab3aedf7c4648f399

Observation 63c1deed-23a7-4c35-ac36-8b1803656a02 · outbound

This paper cites Assessing the Energetics of Spinning Binary Black Hole Systems.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Assessing the Energetics of Spinning Binary Black Hole Systems

Reference 60

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source=pdf_text observed=2026-08-04T19:47:52.019277Z digest=sha256:f9044d59e8acfc7b04a7b0ec542ae9fe2cdba454543109b4c482270e476c6306

Observation 5a3b9cea-e21b-49c0-877e-df53392ceabf · outbound

This paper cites High-accuracy waveforms for binary black hole inspiral, merger, and ringdown.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap High-accuracy waveforms for binary black hole inspiral, merger, and ringdown

Reference 61

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source=pdf_text observed=2026-08-04T19:47:52.023060Z digest=sha256:9606e7ce3df076418f3d90288de329de86e5d1f00bbb82db6f215a590b4dfe69

Observation a2cc6a85-d510-4db0-9b92-ba2e29681330 · outbound

This paper cites Spinning-black-hole binaries: The orbital hang up.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Spinning-black-hole binaries: The orbital hang up

Reference 62

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source=pdf_text observed=2026-08-04T19:47:52.026932Z digest=sha256:25cf43127bd73d80b071f03e9f522e38566e12ec127ecb4e9c5329089c74dc34

Observation f1c593e8-fadc-4955-9402-375c7e89dd8a · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Are LIGO's Black Holes Made From Smaller Black Holes?

Reference 63

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source=pdf_text observed=2026-08-04T19:47:52.030792Z digest=sha256:d5f757ea22225f09c7b5568dfb77bb7bfe49e1202a51ac448d731f4620f28d94

Observation e36f517e-1220-486a-ac5b-371ab3f31daa · outbound

This paper cites Binary black hole mergers from merged stars in the Galactic field.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Binary black hole mergers from merged stars in the Galactic field

Reference 64

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source=pdf_text observed=2026-08-04T19:47:52.034735Z digest=sha256:10e1cd35bb4b0f8b99c6ca3cdd619be4235501f581f689615ec6408d3006c424

Observation 8fe39676-b492-4259-826f-4771953ec459 · outbound

This paper cites Double black hole mergers in nuclear star clusters: eccentricities, spins, masses, and the growth of massive seeds.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Double black hole mergers in nuclear star clusters: eccentricities, spins, masses, and the growth of massive seeds

Reference 65

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source=pdf_text observed=2026-08-04T19:47:52.038795Z digest=sha256:1f89a7ee0102b382ddcd9e8ad3116db634f2e3e927a141ebc4b37bcb83066b91

Observation fc287d18-dc51-4977-ae91-f534807f1664 · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap A Star Cluster Population of High Mass Black Hole Mergers in Gravitational Wave Data

Reference 66

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source=pdf_text observed=2026-08-04T19:47:52.042834Z digest=sha256:eff1ee5d6416613fd920b402c25e60a64401e372dd2fbeee9fcf492b16aea654

Observation d95a77d9-e01b-4d56-a16d-013057158bbb · outbound

This paper cites Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution

Reference 67

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source=pdf_text observed=2026-08-04T19:47:52.046752Z digest=sha256:ae7a2e1c53816fba3eec7c41e1175c22fa619b77f579d28677850ec6b0bd205a

Observation 45e4c0c1-56bd-40fa-a7b6-818a68e48fb1 · outbound

This paper cites an unresolved cited work.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Unresolved cited work

Reference 68

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source=pdf_text observed=2026-08-04T19:47:52.050729Z digest=sha256:81fa4e58afe69f5b9d21df953865510abb1f23d67e3e61d199dfeb50b9c0c681

Observation 292a99e4-97a0-4934-9f4b-1dc8093a11d4 · outbound

This paper cites Merger rate of black hole binaries from globular clusters: theoretical error bars and comparison to gravitational wave data from GWTC-2.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Merger rate of black hole binaries from globular clusters: theoretical error bars and comparison to gravitational wave data from GWTC-2

Reference 69

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source=pdf_text observed=2026-08-04T19:47:52.054290Z digest=sha256:eab07867ef46cd38ddd48fed3cc01c5586d36e961bf3470f5b9b6d76d190a36f

Observation e6f82081-504e-4a6c-bd9a-e91e57129c6f · outbound

This paper cites One to many: comparing single gravitational-wave events to astrophysical populations.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap One to many: comparing single gravitational-wave events to astrophysical populations

Reference 70

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no resolver link, observed 2026-08-04T19:47:52.058162Z

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source=pdf_text observed=2026-08-04T19:47:52.058162Z digest=sha256:a04bc31df896305843cbf2b7015f31a2472e9e251c110466bc2c9da7f97fb5a0

Observation 35b6437f-9175-4d75-b1bd-de1368b00790 · outbound

This paper cites What GW170729's exceptional mass and spin tells us about its family tree.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap What GW170729's exceptional mass and spin tells us about its family tree

Reference 71

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source=pdf_text observed=2026-08-04T19:47:52.062809Z digest=sha256:338d1fbe3faa5f5d5df6436c42cce8e3446adacb70e243b434c11d91f1d0a96d

Observation db68b243-2054-460f-b336-1a98663527c7 · outbound

This paper cites Targeted modeling of GW150914's binary black hole source with dart_board.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Targeted modeling of GW150914's binary black hole source with dart_board

Reference 72

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source=pdf_text observed=2026-08-04T19:47:52.066643Z digest=sha256:423ee442e552ef7d38f0a72acd0f519418d307f82831ea0970702d6fa9fc67dc

Observation c33edb42-4f58-44f6-818d-4f3e3fcc949d · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The Pair-Instability Mass Gap for Black Holes

Reference 73

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source=pdf_text observed=2026-08-04T19:47:52.070913Z digest=sha256:4d017d237b1ee091ad04338f17920ced1cd0cbdfdfc1fc27f5144925b550d443

Observation 5b2571e2-a8b2-4eb2-aabe-b1c9919eee87 · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The impact of stellar rotation on the black hole mass-gap from pair-instability supernovae

Reference 74

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source=pdf_text observed=2026-08-04T19:47:52.074860Z digest=sha256:7d95d09143dba2161861209910232295ecbf4002bcbd3c23d0d8468b8c8108ae

Observation dab4eb0f-18b5-4f23-9672-391759aab971 · outbound

This paper cites Formation of black holes in the pair-instability mass gap: evolution of a post-collision star.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Formation of black holes in the pair-instability mass gap: evolution of a post-collision star

Reference 75

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source=pdf_text observed=2026-08-04T19:47:52.078787Z digest=sha256:463049f1915302adfeed3f770b2cac3ef56dbe3029c2deb8d3f32f58cb8a3d07

Observation 81bf4396-021e-482d-b362-a6fa3ea34c7d · outbound

This paper cites Where are LIGO's Big Black Holes?.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Where are LIGO's Big Black Holes?

Reference 76

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source=pdf_text observed=2026-08-04T19:47:52.083180Z digest=sha256:1d3e465540cf27c4078b67d57d7ad720d6b00be4d9ff52914d547f4211bd28d0

Observation 3974f068-1364-4b9f-bd5e-2fa349a93010 · outbound

This paper cites Measuring the binary black hole mass spectrum with an astrophysically motivated parameterization.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Measuring the binary black hole mass spectrum with an astrophysically motivated parameterization

Reference 77

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source=pdf_text observed=2026-08-04T19:47:52.087783Z digest=sha256:1f2702b27026cc45c4ca93cc2d5450636d813668321d3e5286af7f97d6635880

Observation e410493d-247f-4feb-ab8c-deec4df2f7a5 · outbound

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

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

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source=pdf_text observed=2026-08-04T19:47:52.091394Z digest=sha256:83ba84b549a3dbbd5e5bddfc958bff9cfae34a710c03d4b9eeb85288b5a98a35

Observation dd3f2141-4ce3-42d3-85cd-e4bb729b62c2 · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Resolving the Stellar-Collapse and Hierarchical-Merger origins of the Coalescing Black Holes

Reference 79

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source=pdf_text observed=2026-08-04T19:47:52.095364Z digest=sha256:2ee18624eda392e3c147540279b8f6e32bad29bcad385c4b5a4bfdd151988374

Observation 2b6110ac-7382-42b6-b1e8-d6c9031414c9 · outbound

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

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Evidence of the pair instability gap from black hole masses

Reference 80

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source=pdf_text observed=2026-08-04T19:47:52.099096Z digest=sha256:1ae1111cb29aa2e985f4b2b34d4a1bbdf57e306a1473acf47e7320956a88b2cb

Observation b35ccb6e-3378-416f-bfb4-85b409666589 · outbound

This paper cites Computing in science & engineering13(2), 22–30 (2011).

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Computing in science & engineering13(2), 22–30 (2011)

Reference 81

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source=pdf_text observed=2026-08-04T19:47:52.103167Z digest=sha256:5e696d90b16fead5e8d630287e7e914c57a141dc8c59e4e1e98e2a029d930251

Observation fa221131-837a-40c3-a07d-a5605f71664b · outbound

This paper cites [Online; accessed ¡today¿] (2001–).

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap [Online; accessed ¡today¿] (2001–)

Reference 82

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source=pdf_text observed=2026-08-04T19:47:52.106952Z digest=sha256:96b331eaf9c98d8468a2804d6adb589daeab1a534efd3a86d9b7de9b9b924a92

Observation 2e6d705d-014a-4753-886b-7a40d7b76d11 · outbound

This paper cites Computing in science & engineering9(03), 90–95 (2007).

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Computing in science & engineering9(03), 90–95 (2007)

Reference 83

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source=pdf_text observed=2026-08-04T19:47:52.110587Z digest=sha256:ba42ab7f56042f880e16601faa7a739209a88380c9abab10cc7cd72d599b081e

Observation cacb1718-4aec-4dff-bd3c-ef8ec10de127 · outbound

This paper cites Astronomy & Astrophysics 558, 33 (2013) 29.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Astronomy & Astrophysics 558, 33 (2013) 29

Reference 84

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source=pdf_text observed=2026-08-04T19:47:52.114171Z digest=sha256:44668308e66829bfa698e58afa479ccc5395b842f6decb35d4aecf083bbde6da

Pith citing papers

Observation 2fba1e4b-f7db-4dbc-b613-dc0742319247 · inbound

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Reference 31

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arxiv_id, observed 2026-05-22T12:41:33.051391Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-22T12:40:21.857869Z digest=sha256:8ec0b02e72a3022961a9bf9ae0ba4f3ee56ee10ff0513fc15d344d391e814f38

Observation e2471384-dc0f-4d6c-8580-fbff915ad04f · inbound

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

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Reference 31

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no resolver link, observed 2026-08-04T08:07:40.924944Z

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source=pdf_text observed=2026-08-04T08:07:40.924944Z digest=sha256:c8331bff3ee6ebbe0e02d8d54c6d2a4a9d62d77ff7ae5222acd925e6d576b5e0

Observation bbc740e1-83f8-4c3b-8719-12064ea32383 · inbound

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no resolver link, observed 2026-08-04T07:34:36.703571Z

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source=arxiv_source observed=2026-08-04T07:34:36.703571Z digest=sha256:7e8c1987d56448e53a8083c2ff623ec79121f488ff25f76b14682d96e1c7dc68

Observation 7c789526-4d9c-4d79-8b08-2ddadd348c35 · inbound

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Reference 29

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no resolver link, observed 2026-08-03T14:21:57.775448Z

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source=pdf_text observed=2026-08-03T14:21:57.775448Z digest=sha256:41a841d03d39312a8af24cab2a8146ac1ef0bf705af854a97b7c137bd07c3c62

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Reference 6

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arxiv_id, observed 2026-05-13T02:07:06.449335Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-13T02:05:31.143893Z digest=sha256:5ca73fbdfc506d56a1e809f44f09de4bb1810f1bf6bd611653bdb76297b4ec0b

Observation 9b227c03-95bb-45d0-8092-188752352e7f · inbound

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Reference 64

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arxiv_id, observed 2026-05-20T15:48:32.072772Z

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source=pdf_text observed=2026-05-20T15:47:16.201801Z digest=sha256:53e0373a729520e972ee72838c461f420c2c7e5b7d694621ddef9e5bc6913ce4

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Reference 8

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arxiv_id, observed 2026-05-25T05:10:22.128560Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-25T05:08:06.029228Z digest=sha256:11a91354055ce12836cecde5346b2ce7240fe72cbeaa06e947c3b467872350f9

Observation 3a8f273b-e6ce-4b40-b24d-982f3a2171ae · inbound

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Reference 56

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arxiv_id, observed 2026-06-29T22:44:02.258259Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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arxiv_id, observed 2026-06-29T22:44:02.342363Z

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source=pdf_text observed=2026-06-29T20:34:04.639423Z digest=sha256:e342ec577fe0a9284a0f23c2044971fa8d6b613209610eb0b56af889b8ce76e6

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arxiv_id, observed 2026-07-01T20:26:13.206350Z

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source=pdf_text observed=2026-06-28T21:05:31.906236Z digest=sha256:580468b81a82a95b20b73067ab12e5ab35e61e745dca77f41f3a8b69a41a908d

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Reference 281

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arxiv_id, observed 2026-06-28T00:21:28.000547Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-06-28T00:18:26.396766Z digest=sha256:934bd15847cedf68646969d976580ea8b0ab4988e74305914b2d4bbc87cc8059

Observation 0e25982c-4a81-48cc-89ce-9dd05f3ac72e · inbound

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Reference 280

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source=pdf_text observed=2026-08-02T12:20:55.547179Z digest=sha256:03fe510294f068613d7f00e3fa10b7de3fadd2b914c8e908a5aaeaab40475910

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Reference 244

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arxiv_id, observed 2026-06-26T23:10:14.412097Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-06-26T23:08:42.665379Z digest=sha256:be48133e55edccaeaa3394d0d7e3d94c862f215643dfc28dc44f29431067ffe3

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Reference 9

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arxiv_id, observed 2026-07-02T07:56:46.860048Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-02T07:55:37.395171Z digest=sha256:2016c1ad04222b5ce4af6fceed000056a1d59173f2b5b8e7081aa4c6b0ecc3e2

Observation fca7a5b9-7a52-40e5-a9f0-74fbb9224547 · inbound

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Reference 72

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no resolver link, observed 2026-08-01T23:27:58.945083Z

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source=pdf_text observed=2026-08-01T23:27:58.945083Z digest=sha256:0ba56cd742db1a035e39249913e71b2439eb0ee97ca623dee2d2899f048ddc01

Observation d24bf5cf-51de-4725-ac04-2d9967f7ae6b · inbound

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Reference 82

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no resolver link, observed 2026-08-01T23:22:40.759984Z

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source=pdf_text observed=2026-08-01T23:22:40.759984Z digest=sha256:4e841222381ba872c5c08872cdb7f6a7a718bfd7bc6872275a57495cd0c8403e

Observation 658e6205-ff96-4752-8475-68f257eaccb0 · inbound

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unresolved
no resolver link, observed 2026-07-31T22:07:28.371502Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T22:07:28.371502Z digest=sha256:4c35e3f9f18ccb98d39ff0b6f3dbea6fbbaaed3c92e8e4cf641cdcc13d17c4eb

Observation 38bfff6e-5412-4be9-8e4a-98daf10dd0a7 · inbound

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no resolver link, observed 2026-07-31T01:54:12.237885Z

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source=arxiv_source observed=2026-07-31T01:54:12.237885Z digest=sha256:eb72daa07cc4a15fa202b322e2c7c43550244e9ce43ecda11407010744b8909c