Paper Citation Record · LEDGER

Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2503.03819.

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

pith.paper-citation-record.v1
2503.03819 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T10:20:19.739611Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T12:58:07.783076Z

Reference resolution

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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 1f787ad9-b285-4ab1-8940-42143cc23625 · inbound

Emulating compact binary population synthesis simulations with uncertainty quantification and model comparison using Bayesian normalizing flows cites this paper.

Emulating compact binary population synthesis simulations with uncertainty quantification and model comparison using Bayesian normalizing flows Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-07T10:20:19.739611Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 025d1b73-1f47-4530-97d9-8b396f142044 · inbound

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop cites this paper.

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 fd5021c3-d409-494b-90e3-5b6bfe177ea0 · 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 Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows

Reference 16

Resolution: verified exact; arxiv_id, observed 2026-05-19T04:37:03.839863Z

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 df8196fa-2408-4ecb-a597-1be2f35eff0d · inbound

Exploring the astrophysical origins of binary black holes using normalising flows cites this paper.

Exploring the astrophysical origins of binary black holes using normalising flows Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-05T15:53:35.214375Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation be4c573d-624b-4300-aefc-5cf5a517823b · inbound

Model-Agnostic Population Inference for Gravitational-Wave Astronomy: From LVK to LISA cites this paper.

Model-Agnostic Population Inference for Gravitational-Wave Astronomy: From LVK to LISA Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-03T06:35:05.936171Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b5ea4fd-e8c5-4a17-b888-82175f1c18c0 · inbound

Emergent structure in the binary black hole mass distribution and implications for population-based cosmology cites this paper.

Emergent structure in the binary black hole mass distribution and implications for population-based cosmology Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows

Reference 32

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T11:51:01.229774Z

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 71856644-8374-4c83-83bc-9ec0866a4fff · 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 Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows

Reference 26

Resolution: verified exact; arxiv_id, observed 2026-05-13T02:02:06.026264Z

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 05243865-028d-4020-b7d8-ba467abf530e · 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 Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows

Reference 17

Resolution: verified exact; arxiv_id, observed 2026-07-03T12:58:07.784433Z

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 e0d204fc-4614-466f-b8f6-d767b2c57404 · 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 Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows

Reference 58

Resolution: unresolved; no resolver link, observed 2026-07-31T01:54:12.286507Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.