Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2201.00607.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T17:08:37.164351Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T21:38:59.310135Z
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
No outbound reference observations are available for this paper version.
Observation b8ceba49-caf1-496f-99ce-3df078490518 · inbound
Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
Reference 67
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation d12853e3-7f67-4f43-9621-a9acfedb1454 · inbound
Two-Dimensional Pulsar Distance Inference from Nanohertz Gravitational Waves Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
Reference 17
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a245c1b4-c2b7-412e-b250-0363e1cdce47 · inbound
Model-independent H0 from GWTC-4 standard sirens and TDCOSMO 2025 strong lensing time delays Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
Reference 74
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 5100321a-d266-4d96-a940-848826670d1e · inbound
Synergy between CSST and future gravitational-wave detectors: Probing primordial black holes by cross-correlating dark sirens with galaxies Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
Reference 57
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.