Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-06T22:52:12.354831Z
Paper Citation Record · LEDGER
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
As of 7 August 2026, this Paper Citation Record lists 100 of 149 outbound references and 12 inbound Pith citation observations for arXiv:2506.20731.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T22:42:34.620826Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
100 of 149 outbound references displayed
- verified exact3
- verified fuzzy0
- unresolved97
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
Observation c923c578-246b-4494-b5c3-1a7f693a11ae · outbound
This paper cites Advanced LIGO.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Advanced LIGO
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.088241Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6f8d39dd-0f74-4b8e-a9e1-f5eb669abf03 · outbound
This paper cites Advanced Virgo: a 2nd generation interferometric gravitational wave detector.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Advanced Virgo: a 2nd generation interferometric gravitational wave detector
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.091378Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e5d55a39-ce3c-42c9-b6d5-b14a6d90f14e · outbound
This paper cites Akutsuet al.(KAGRA), PTEP2021, 05A101 (2021), arXiv:2005.05574 [physics.ins-det].
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Akutsuet al.(KAGRA), PTEP2021, 05A101 (2021), arXiv:2005.05574 [physics.ins-det]
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.094496Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f815e926-85a4-4480-8f37-a1ba5f38c00c · outbound
This paper cites GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.097568Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation dc08cad7-bd51-49bc-938c-937685a43748 · outbound
This paper cites Vitale, D.
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.100404Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d12fe6ed-c079-4720-8b40-17e89a5cb62e · outbound
This paper cites An introduction to Bayesian inference in gravitational-wave astronomy: parameter estimation, model selection, and hierarchical models.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop An introduction to Bayesian inference in gravitational-wave astronomy: parameter estimation, model selection, and hierarchical models
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.103029Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0ee1bc48-2fa4-4200-80f2-429e889d37d8 · outbound
This paper cites Observed Gravitational-Wave Populations.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Observed Gravitational-Wave Populations
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.105793Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b0bedd8d-9daf-491c-8641-b4c7ab0c88a2 · outbound
This paper cites Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.108901Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation aa26fc62-e4b6-4f53-97d2-39015d66b2f0 · outbound
This paper cites Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.111610Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bb253c3e-67d6-4dbe-9db7-dda474e72df5 · outbound
This paper cites The population of merging compact binaries inferred using gravitational waves through GWTC-3.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop The population of merging compact binaries inferred using gravitational waves through GWTC-3
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.114291Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 47d0f09b-c321-49bb-9fe0-ae04e0873802 · outbound
This paper cites Binary black hole mergers: formation and populations.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Binary black hole mergers: formation and populations
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.116971Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d6b49082-ade2-42d1-8c12-8a21f0019f64 · outbound
This paper cites Common Envelope Evolution: Where we stand and how we can move forward.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Common Envelope Evolution: Where we stand and how we can move forward
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.120175Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ed555f5b-b560-4dbd-a342-8c9f51dd1aa6 · outbound
This paper cites The impact of mass-transfer physics on the observable properties of field binary black hole populations.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop The impact of mass-transfer physics on the observable properties of field binary black hole populations
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.123246Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 21abbd4e-6407-48ea-b3db-21116af3ba7c · outbound
This paper cites Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.125764Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a130269a-3398-4386-8268-3dcb078a542c · outbound
This paper cites The properties of merging black holes and neutron stars across cosmic time.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop The properties of merging black holes and neutron stars across cosmic time
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.128326Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 165272e4-a735-482a-b83c-494275820563 · outbound
This paper cites Rates of Compact Object Coalescences.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Rates of Compact Object Coalescences
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.130894Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 524f2574-1af0-4923-b5c0-46d4db0db491 · outbound
This paper cites Forming short-period Wolf-Rayet X-ray binaries and double black holes through stable mass transfer.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Forming short-period Wolf-Rayet X-ray binaries and double black holes through stable mass transfer
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.133453Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a3e4dc25-6a72-4232-a26d-532fe8c211af · outbound
This paper cites The effect of the metallicity-specific star formation history on double compact object mergers.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop The effect of the metallicity-specific star formation history on double compact object mergers
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.136240Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b1439881-a536-4aac-8dc0-bdb69ae19922 · outbound
This paper cites Binary Black Hole Formation with Detailed Modeling: Stable Mass Transfer Leads to Lower Merger Rates.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Binary Black Hole Formation with Detailed Modeling: Stable Mass Transfer Leads to Lower Merger Rates
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.138849Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4e22ab87-bf94-4582-b5c7-d4274eabaa15 · outbound
This paper cites Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.141662Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bc32c372-ea4d-489d-a09e-35470c4ca960 · outbound
This paper cites Eggleton, S.
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.144278Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c62600bc-3653-4a9f-ade0-71e94a4b9eb2 · outbound
This paper cites Paczynski, Symposium - International Astronomical Union73, 75–80 (1976).
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Paczynski, Symposium - International Astronomical Union73, 75–80 (1976)
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.146907Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0bc66f9f-4ff1-410c-be01-544484c6e4e0 · outbound
This paper cites an unresolved cited work.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Unresolved cited work
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.149295Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 80b33c75-ee7b-4499-9222-ddbba14ebfbd · outbound
This paper cites Evolution of Binary Compact Objects Which Merge.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Evolution of Binary Compact Objects Which Merge
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.151691Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c1ee661a-51ca-4e02-88c1-be4f9ce27499 · outbound
This paper cites A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.154376Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 255f0475-cf5c-437f-b450-569847648d4c · outbound
This paper cites Formation of the first three gravitational-wave observations through isolated binary evolution.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Formation of the first three gravitational-wave observations through isolated binary evolution
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.156969Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2ac29e63-71da-4aeb-a0a5-c7225a02a8a4 · outbound
This paper cites The progenitors of compact-object binaries: impact of metallicity, common envelope and natal kicks.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop The progenitors of compact-object binaries: impact of metallicity, common envelope and natal kicks
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.159647Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3932d427-dd89-4760-bd60-24b3fcef4530 · outbound
This paper cites Double Compact Objects I: The Significance Of The Common Envelope On Merger Rates.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Double Compact Objects I: The Significance Of The Common Envelope On Merger Rates
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.162657Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ca9a66e8-7cd5-48f4-b1cd-2fa0f5e70c2c · outbound
This paper cites an unresolved cited work.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Unresolved cited work
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.165346Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bd7d972a-a8d9-49f6-a137-e66c284630b4 · outbound
This paper cites I: SMT and CHE.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop I: SMT and CHE
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.084112Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ac4d53b1-7ac5-41fa-bf8f-a01966bdf5fd · outbound
This paper cites One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.167997Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0f53dfa7-6f84-4b46-96bb-de3e04f70090 · outbound
This paper cites Rotational mixing in massive binaries: detached short-period systems.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Rotational mixing in massive binaries: detached short-period systems
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.170725Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ab328555-73ad-43e4-9100-65e1135443f7 · outbound
This paper cites Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.173647Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bf889166-2126-479c-b7b8-78c9a7099821 · outbound
This paper cites The chemically homogeneous evolutionary channel for binary black hole mergers: rates and properties of gravitational-wave events detectable by advanced LIGO.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop The chemically homogeneous evolutionary channel for binary black hole mergers: rates and properties of gravitational-wave events detectable by advanced LIGO
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.176221Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2b79c0d1-6511-496a-8050-373b4f76a602 · outbound
This paper cites A new route towards merging massive black holes.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop A new route towards merging massive black holes
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.178729Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ae186cc1-5746-4c1c-81f8-fa955ddfa355 · outbound
This paper cites Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.181264Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a5eee19e-6565-483d-a7d7-5d3705208b34 · outbound
This paper cites Sigurdsson and L.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Sigurdsson and L
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.184088Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6d56c4b1-1c53-4150-b0e2-ae1e7803c636 · outbound
This paper cites Sigurdsson and E.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Sigurdsson and E
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.186461Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9d64a025-9247-4780-9081-1b35c4b6ef3a · outbound
This paper cites Black hole mergers in the universe.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Black hole mergers in the universe
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.188773Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5a3c1fef-f69a-41b5-9ef7-965e46a8b181 · outbound
This paper cites Four-Body Effects in Globular Cluster Black Hole Coalescence.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Four-Body Effects in Globular Cluster Black Hole Coalescence
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.191590Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c65b811b-5d7e-41af-aedf-8adc096a6550 · outbound
This paper cites an unresolved cited work.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Unresolved cited work
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.195019Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a820a2e7-9824-4b7a-93dd-9717da194248 · outbound
This paper cites an unresolved cited work.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Unresolved cited work
Reference 42
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.197623Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8fc80058-63d6-4c4d-ac8f-dcd9d15fc61b · outbound
This paper cites Monte Carlo Simulations of Globular Cluster Evolution. IV. Direct Integration of Strong Interactions.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Monte Carlo Simulations of Globular Cluster Evolution. IV. Direct Integration of Strong Interactions
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.200001Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6a57879f-7a08-402a-9143-e0f9f74774de · outbound
This paper cites Binary Mergers and Growth of Black Holes in Dense Star Clusters.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Binary Mergers and Growth of Black Holes in Dense Star Clusters
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.202470Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a8933030-5d4c-4f99-bc53-abb83c69d392 · outbound
This paper cites Compact Binaries in Star Clusters I - Black Hole Binaries Inside Globular Clusters.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Compact Binaries in Star Clusters I - Black Hole Binaries Inside Globular Clusters
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.205254Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c1af1427-ad26-4135-8edb-3c2ca07ffa15 · outbound
This paper cites Binary Black Hole Mergers from Globular Clusters: Implications for Advanced LIGO.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Binary Black Hole Mergers from Globular Clusters: Implications for Advanced LIGO
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.207933Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 81c33e20-acdc-48b1-a38f-1a7982af1b5b · outbound
This paper cites Binary Black Hole Mergers from Globular Clusters: Masses, Merger Rates, and the Impact of Stellar Evolution.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Binary Black Hole Mergers from Globular Clusters: Masses, Merger Rates, and the Impact of Stellar Evolution
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.210703Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d8bafa1e-8664-4f6a-9b9a-dfccd17adad5 · outbound
This paper cites Black Holes: The Next Generation -- Repeated Mergers in Dense Star Clusters and their Gravitational-Wave Properties.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Black Holes: The Next Generation -- Repeated Mergers in Dense Star Clusters and their Gravitational-Wave Properties
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.213349Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3debdabe-8952-4db5-9946-a6b9ccb06684 · outbound
This paper cites MOCCA-SURVEY Database I: Coalescing Binary Black Holes Originating From Globular Clusters.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop MOCCA-SURVEY Database I: Coalescing Binary Black Holes Originating From Globular Clusters
Reference 49
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.216113Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c980094d-96b5-4821-9435-373ebe0edddb · outbound
This paper cites Mergers of Stellar-Mass Black Holes in Nuclear Star Clusters.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Mergers of Stellar-Mass Black Holes in Nuclear Star Clusters
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.218704Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7c7f4c74-2739-4e57-b734-c5c353ef1ce3 · outbound
This paper cites Stellar-mass black holes in star clusters: implications for gravitational wave radiation.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Stellar-mass black holes in star clusters: implications for gravitational wave radiation
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.221203Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 55df74e0-2927-48bc-96b6-0989ead32444 · outbound
This paper cites an unresolved cited work.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Unresolved cited work
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.223939Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d13e1158-68c5-49b4-9a16-afa5d3e0b33d · outbound
This paper cites Merging black hole binaries in galactic nuclei: implications for advanced-LIGO detections.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Merging black hole binaries in galactic nuclei: implications for advanced-LIGO detections
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.226689Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b88127f2-5193-49df-8db1-162df57cd389 · outbound
This paper cites On stellar-mass black hole mergers in AGN disks detectable with LIGO.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop On stellar-mass black hole mergers in AGN disks detectable with LIGO
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.229351Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 183b5bc6-4dd0-43d8-8430-a4fd4150113c · outbound
This paper cites Monte-Carlo simulations of black hole mergers in AGN disks: Low $\chi_{\rm eff}$ mergers and predictions for LIGO.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Monte-Carlo simulations of black hole mergers in AGN disks: Low $\chi_{\rm eff}$ mergers and predictions for LIGO
Reference 55
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.232034Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2ce1d32e-bf85-470c-8781-4eb533167340 · outbound
This paper cites Assisted Inspirals of Stellar Mass Black Holes Embedded in AGN Disks: Solving the "Final AU Problem".
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Assisted Inspirals of Stellar Mass Black Holes Embedded in AGN Disks: Solving the "Final AU Problem"
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.234688Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d33c8b44-3b95-46b9-bad9-3010143bf1aa · outbound
This paper cites Formation and Evolution of Compact Object Binaries in AGN Disks.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Formation and Evolution of Compact Object Binaries in AGN Disks
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.237534Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cc393266-6cff-41f6-84ed-56192289c36f · outbound
This paper cites Signatures of Hierarchical Mergers in Black Hole Spin and Mass distribution.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Signatures of Hierarchical Mergers in Black Hole Spin and Mass distribution
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.240330Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b79f3048-ed3c-473c-bc16-29016ad91a44 · outbound
This paper cites Bartos, B.
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.243079Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ed65c1ef-701c-4c98-8160-e6b06bcee56d · outbound
This paper cites Cosmic Evolution of Stellar-mass Black Hole Merger Rate in Active Galactic Nuclei.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Cosmic Evolution of Stellar-mass Black Hole Merger Rate in Active Galactic Nuclei
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.245624Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9527d36f-c016-41e4-b807-532578bf6781 · outbound
This paper cites Sana, J.-B.
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.248461Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6573ba76-a6fa-4062-9869-931bfbe25df6 · outbound
This paper cites Lidov-Kozai Cycles with Gravitational Radiation: Merging Black Holes in Isolated Triple Systems.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Lidov-Kozai Cycles with Gravitational Radiation: Merging Black Holes in Isolated Triple Systems
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.250898Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c41c84e0-9cb1-451f-bb26-717b306b2247 · outbound
This paper cites A Triple Origin for the Heavy and Low-Spin Binary Black Holes Detected by LIGO/Virgo.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop A Triple Origin for the Heavy and Low-Spin Binary Black Holes Detected by LIGO/Virgo
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.253473Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 42ea6515-06c0-4cc2-a6b4-ea163b8e6a18 · outbound
This paper cites Gravitational Waves from Hierarchical Triple Systems with Kozai-Lidov Oscillation.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Gravitational Waves from Hierarchical Triple Systems with Kozai-Lidov Oscillation
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.256215Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f4e29895-a6b1-49b1-bc85-2db7b056cd7b · outbound
This paper cites Toonen, S.
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.259012Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3585ca01-4157-4508-904a-9ccf32385360 · outbound
This paper cites Measuring the binary black hole mass spectrum with an astrophysically motivated parameterization.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Measuring the binary black hole mass spectrum with an astrophysically motivated parameterization
Reference 66
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.261442Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6a676319-9aaa-4d95-9543-81bb7c4419f1 · outbound
This paper cites Does the Black Hole Merger Rate Evolve with Redshift?.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Does the Black Hole Merger Rate Evolve with Redshift?
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.264001Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9be2c7bd-f20a-49f6-9d5e-3c5c8b7a90df · outbound
This paper cites When models fail: an introduction to posterior predictive checks and model misspecification in gravitational-wave astronomy.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop When models fail: an introduction to posterior predictive checks and model misspecification in gravitational-wave astronomy
Reference 68
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.266980Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0bc991c9-3431-49c9-8d71-851ca8d3515f · outbound
This paper cites What You Don't Know Can Hurt You: Use and Abuse of Astrophysical Models in Gravitational-wave Population Analyses.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop What You Don't Know Can Hurt You: Use and Abuse of Astrophysical Models in Gravitational-wave Population Analyses
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.269969Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9f40df14-82d4-4660-8840-20098584c8ed · outbound
This paper cites Exploring the Parameter Space of Compact Binary Population Synthesis.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Exploring the Parameter Space of Compact Binary Population Synthesis
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.272655Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation acc3d399-1abb-465c-a8fd-cf03084a2b01 · outbound
This paper cites Mining Gravitational-wave Catalogs To Understand Binary Stellar Evolution: A New Hierarchical Bayesian Framework.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Mining Gravitational-wave Catalogs To Understand Binary Stellar Evolution: A New Hierarchical Bayesian Framework
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.275794Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b7e18e2b-a25b-4eee-9011-c2a42a7f0311 · outbound
This paper cites Joint constraints on the field-cluster mixing fraction, common envelope efficiency, and globular cluster radii from a population of binary hole mergers via deep learning.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Joint constraints on the field-cluster mixing fraction, common envelope efficiency, and globular cluster radii from a population of binary hole mergers via deep learning
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.278646Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 06b5cd28-0706-4978-8400-a7f505db8fbc · outbound
This paper cites Deep learning and Bayesian inference of gravitational-wave populations: Hierarchical black-hole mergers.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Deep learning and Bayesian inference of gravitational-wave populations: Hierarchical black-hole mergers
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.281319Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 95a663b3-8d95-4b64-bc02-979b35f041f1 · outbound
This paper cites Surrogate forward models for population inference on compact binary mergers.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Surrogate forward models for population inference on compact binary mergers
Reference 74
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T22:52:13.357435Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 6fe0c24e-9e93-4de2-8da8-ea71469382a2 · outbound
This paper cites Gravitational wave populations and cosmology with neural posterior estimation.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Gravitational wave populations and cosmology with neural posterior estimation
Reference 75
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.287042Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 13557c2e-fe15-4341-826d-6bfb630754be · outbound
This paper cites Inferring binary black holes stellar progenitors with gravitational wave sources.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Inferring binary black holes stellar progenitors with gravitational wave sources
Reference 76
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.289712Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 025d1b73-1f47-4530-97d9-8b396f142044 · outbound
This paper cites Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows
Reference 77
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.293252Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5d00063a-66dc-492e-b1e6-ba9c82d11db7 · outbound
This paper cites Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes
Reference 78
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.296201Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 00265baf-7844-4a79-b0e4-d5d3c82ae1f7 · outbound
This paper cites Constraining Population III stellar demographics with next-generation gravitational-wave observatories.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Constraining Population III stellar demographics with next-generation gravitational-wave observatories
Reference 79
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.298919Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 84ebe30f-e469-431c-9165-8f4d3b5a874b · outbound
This paper cites PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.301527Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 57df0abf-1300-4588-be53-69c80ab038b1 · outbound
This paper cites Cover Your Basis: Comprehensive Data-Driven Characterization of the Binary Black Hole Population.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Cover Your Basis: Comprehensive Data-Driven Characterization of the Binary Black Hole Population
Reference 81
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.304214Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0ee3915a-5562-49f7-86db-635babbe7a20 · outbound
This paper cites Cosmic Cousins: Identification of a Subpopulation of Binary Black Holes Consistent with Isolated Binary Evolution.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Cosmic Cousins: Identification of a Subpopulation of Binary Black Holes Consistent with Isolated Binary Evolution
Reference 82
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.306906Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 46eb7957-fd6f-468e-90fc-949af64317d2 · outbound
This paper cites Searching for structure in the binary black hole spin distribution.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Searching for structure in the binary black hole spin distribution
Reference 83
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.309671Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 63dc9027-e173-46e4-8d8d-70f76626d7ce · outbound
This paper cites Probing Correlations in the Binary Black Hole Population with Flexible Models.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Probing Correlations in the Binary Black Hole Population with Flexible Models
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.312259Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c7ebfb07-81aa-41d3-b802-48893fa85f8b · outbound
This paper cites VAMANA: Modeling Binary Black Hole Population with Minimal Assumptions.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop VAMANA: Modeling Binary Black Hole Population with Minimal Assumptions
Reference 85
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.315339Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f7afc156-64ed-47ca-bee6-858e791c4bec · outbound
This paper cites (H)DPGMM: A Hierarchy of Dirichlet Process Gaussian Mixture Models for the inference of the black hole mass function.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop (H)DPGMM: A Hierarchy of Dirichlet Process Gaussian Mixture Models for the inference of the black hole mass function
Reference 86
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.318079Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8d7a8dfd-43fa-4fec-93e7-a391232237c5 · outbound
This paper cites A Parameter-Free Tour of the Binary Black Hole Population.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop A Parameter-Free Tour of the Binary Black Hole Population
Reference 87
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.320752Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 63ba69fb-407e-4a7d-95ee-5f52829945c4 · outbound
This paper cites A flexible Gaussian process reconstruction method and the mass function of the coalescing binary black hole systems.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop A flexible Gaussian process reconstruction method and the mass function of the coalescing binary black hole systems
Reference 88
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.323343Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eb7b7ab4-e324-49ca-8d27-394d24f68f02 · outbound
This paper cites Non-parametric inference of the population of compact binaries from gravitational wave observations using binned Gaussian processes.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Non-parametric inference of the population of compact binaries from gravitational wave observations using binned Gaussian processes
Reference 89
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.325804Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7d513660-7d19-453c-bbd5-558621a862a3 · outbound
This paper cites No need to know: astrophysics-free gravitational-wave cosmology.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop No need to know: astrophysics-free gravitational-wave cosmology
Reference 90
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.328446Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 50c171cc-765f-4935-a35b-2bebfba95aed · outbound
This paper cites Is there an excess of black holes around $20 M_{\odot}$? Optimising the complexity of population models with the use of reversible jump MCMC.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Is there an excess of black holes around $20 M_{\odot}$? Optimising the complexity of population models with the use of reversible jump MCMC
Reference 91
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.331057Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 920c8388-e149-412b-b3e4-e80c15927f3c · outbound
This paper cites Binary vision: The merging black hole binary mass distribution via iterative density estimation.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Binary vision: The merging black hole binary mass distribution via iterative density estimation
Reference 92
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T22:52:13.201858Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation a048f53b-7805-451a-a837-8e738e5b34d9 · outbound
This paper cites Sadiq, T.
Reference 93
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.336784Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 85f6ab9f-fe5f-4574-9ca7-eb21a88efa63 · outbound
This paper cites Sadiq, T.
Reference 94
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.339230Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fa840648-a5a8-484b-be7b-273f06dd389c · outbound
This paper cites Model-independent inference on compact-binary observations.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Model-independent inference on compact-binary observations
Reference 95
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.341572Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 79b991aa-04da-4f78-b468-c61231f90f31 · outbound
This paper cites Reconstructing parametric gravitational-wave population fits from non-parametric results without refitting the data.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Reconstructing parametric gravitational-wave population fits from non-parametric results without refitting the data
Reference 96
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.344196Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0c2bd45b-509a-4c0c-9b38-2ce7375975c7 · outbound
This paper cites Rinaldi, A.
Reference 97
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.346915Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e106c1f1-212c-4c77-9571-00a06b620f97 · outbound
This paper cites The $\chi_\mathrm{eff}-z$ correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop The $\chi_\mathrm{eff}-z$ correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it
Reference 98
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.349308Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 50c99af0-ad66-43c5-ae8c-7de784e62587 · outbound
This paper cites Black-hole mergers in disklike environments could explain the observed $q$-$\chi_\mathrm{eff}$ correlation.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Black-hole mergers in disklike environments could explain the observed $q$-$\chi_\mathrm{eff}$ correlation
Reference 99
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.352049Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f69d0dc8-5174-4a00-bd65-d1409616b111 · outbound
This paper cites Dropping Anchor: Understanding the Populations of Binary Black Holes with Random and Aligned Spin Orientations.
Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Dropping Anchor: Understanding the Populations of Binary Black Holes with Random and Aligned Spin Orientations
Reference 100
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T22:52:12.883623Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Pith citing papers
Observation 21c486e3-01d2-4573-8056-3f716bcb8eec · inbound
Comparing astrophysical models to gravitational-wave data in the observable space cites this paper.
Comparing astrophysical models to gravitational-wave data in the observable space Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 68
- Resolution
- verified exact
- arxiv_id, observed 2026-07-16T01:22:25.909243Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation c23d0dbe-3c5e-4200-837e-834c1604fd75 · inbound
When (not) to trust Monte Carlo approximations for hierarchical Bayesian inference cites this paper.
When (not) to trust Monte Carlo approximations for hierarchical Bayesian inference Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T22:42:34.620826Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6f7fc3bb-23f4-44ec-933b-fc2b4a6fa562 · inbound
Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot}$ Peak cites this paper.
Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot}$ Peak Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T19:56:39.247533Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 41b3ce3d-576c-4ce6-9167-42066a9abdfe · 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 Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 80
- Resolution
- verified exact
- arxiv_id, observed 2026-07-16T01:22:25.909243Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 2dce1e59-9fa9-49fc-bf18-6f94af8ad5e5 · inbound
Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements cites this paper.
Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 35
- Resolution
- verified exact
- arxiv_id, observed 2026-07-16T01:22:25.909243Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 142487e2-82f7-4a08-ae92-a0a3c82bb38e · 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 Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 75
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-16T01:22:25.909243Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 15076384-51b5-460a-afbc-cbfd93665816 · inbound
Secondary-Mass Features improve Spectral-Siren $H_0$ Constraints cites this paper.
Secondary-Mass Features improve Spectral-Siren $H_0$ Constraints Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 7
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-16T01:22:25.909243Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 1116efdb-2c5e-4e84-a12c-885f2cb7b7b9 · inbound
The first decade of gravitational-wave measurements of black hole spins cites this paper.
The first decade of gravitational-wave measurements of black hole spins Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 269
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-16T01:22:25.909243Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 8556f72c-e947-430b-b025-e2a5c3ee6493 · inbound
The first decade of gravitational-wave measurements of black hole spins cites this paper.
The first decade of gravitational-wave measurements of black hole spins Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 268
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T12:20:55.488055Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation abdcfa2a-9437-4fa2-af51-0e8fadc0ef34 · 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 Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 85
- Resolution
- verified exact
- arxiv_id, observed 2026-07-16T01:22:25.909243Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation b001936d-157c-497a-95bc-4287c7e24d78 · inbound
Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation cites this paper.
Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 74
- Resolution
- verified exact
- arxiv_id, observed 2026-07-16T01:22:25.909243Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation c2f12f5e-1b58-4fcc-ac8d-2892687d1067 · inbound
A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations cites this paper.
A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop
Reference 147
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T01:54:12.543878Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.