Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 18 inbound Pith citation observations for arXiv:1712.00482.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T16:12:04.898817Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T22:29:00.101508Z
Reference resolution
0 of 0 outbound references displayed
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External citation measurements
No source-named external measurement is stored.
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 8b542fc9-af73-4fe0-8871-5e28b910d38b · inbound
GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run cites this paper.
GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 115
- Resolution
- verified exact
- local_arxiv, observed 2026-05-16T07:45:53.480251Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 8a818472-8a87-4f1f-b7a8-486f89555ab6 · inbound
Detection of GW200105 with a targeted eccentric search cites this paper.
Detection of GW200105 with a targeted eccentric search Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 67
- Resolution
- verified exact
- local_arxiv, observed 2026-05-16T23:08:40.025917Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 4c5d98c4-07c8-41b2-9918-18c073e2f52f · inbound
Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition cites this paper.
Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 65
- Resolution
- verified exact
- local_arxiv, observed 2026-05-16T16:38:06.363944Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation fa524936-2a95-4dbf-9aac-3f8c10f1180b · 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 Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 106
- Resolution
- verified exact
- local_arxiv, observed 2026-05-16T05:37:23.966035Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 0da9b51b-80b4-4fc6-955a-74e195bbd07f · inbound
Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements cites this paper.
Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 155
- Resolution
- verified exact
- arxiv_id, observed 2026-05-10T23:25:49.944850Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 03e8409b-04a5-4ba8-a188-b6c46f1f3947 · inbound
Gravitational-wave astronomy requires population-informed parameter estimation cites this paper.
Gravitational-wave astronomy requires population-informed parameter estimation Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 70
- Resolution
- verified exact
- arxiv_id, observed 2026-05-10T08:22:37.177384Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 89bea301-4a22-4eba-bb91-9d8c6d91c8ed · inbound
Gravitational-wave astronomy requires population-informed parameter estimation cites this paper.
Gravitational-wave astronomy requires population-informed parameter estimation Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T16:12:04.898817Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8d106374-6391-4fb5-83bd-d80283e30eda · inbound
End-to-End Population Inference from Gravitational-Wave Strain using Transformers cites this paper.
End-to-End Population Inference from Gravitational-Wave Strain using Transformers Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 20
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T02:02:06.008591Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation d8586f12-90a0-449a-beb7-27037e8ddcb5 · inbound
Gravitational-wave constraints on $H_0$ are robust to (putative) redshift evolution in the binary black hole mass spectrum at current sensitivity cites this paper.
Gravitational-wave constraints on $H_0$ are robust to (putative) redshift evolution in the binary black hole mass spectrum at current sensitivity Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 41
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T03:48:02.839381Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 849cb3da-7a2d-463b-957e-9705b8dff500 · inbound
Constraining Gravitational Wave Memory with Hierarchical Inference cites this paper.
Constraining Gravitational Wave Memory with Hierarchical Inference Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 141
- Resolution
- verified exact
- local_arxiv, observed 2026-06-29T15:33:32.871327Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 43920172-faac-4692-90c9-d162d0938ae0 · inbound
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors cites this paper.
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 89
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T04:26:36.102570Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 55372506-b18d-479f-b085-dfc167922791 · 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 Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 122
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T12:58:07.916800Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 0f84ae4f-ee59-4a51-a01c-bbff32053f66 · inbound
Fortifying gravitational-wave population inference with normalizing flows cites this paper.
Fortifying gravitational-wave population inference with normalizing flows Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T11:36:00.260053Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d9696a04-d10d-4bcc-8054-728742648c44 · inbound
The Chirp-Mass Ladder: A New Rung Emerges cites this paper.
The Chirp-Mass Ladder: A New Rung Emerges Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 32
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-26T23:10:14.477372Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 201e2a07-f559-41b7-a5cf-00098ac70c67 · 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 Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 53
- Resolution
- verified exact
- local_arxiv, observed 2026-06-30T14:34:45.420648Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation b0ee445f-4993-46bc-bf6e-e952f6cc4a2e · inbound
Establishing Compactness as a Population Observable in Gravitational-Wave Astronomy cites this paper.
Establishing Compactness as a Population Observable in Gravitational-Wave Astronomy Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 88
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T11:35:42.635854Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 8fd2fef3-5148-48f9-8097-83964ae0dbc1 · inbound
Establishing Compactness as a Population Observable in Gravitational-Wave Astronomy cites this paper.
Establishing Compactness as a Population Observable in Gravitational-Wave Astronomy Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 88
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T22:29:00.102918Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 696d0cde-1813-464d-a0c0-19ce0a3da9de · inbound
Establishing Compactness as a Population Observable in Gravitational-Wave Astronomy cites this paper.
Establishing Compactness as a Population Observable in Gravitational-Wave Astronomy Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
Reference 88
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T09:26:37.452079Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.