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 9 inbound Pith citation observations for arXiv:2002.07251.
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 2026-08-07T13:41:49.943279Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-25T06:40:25.097196Z
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 e2f5d592-71ce-4d08-8641-4671cd1baffc · inbound
Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects Significance of Black Hole Quasinormal Modes: A Closer Look
Reference 56
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 a480c28b-657d-4b97-ad3d-40629b3ffab7 · inbound
Spectrum instability and greybody factor stability for parabolic approximation of Regge-Wheeler potential Significance of Black Hole Quasinormal Modes: A Closer Look
Reference 12
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4f49a3cf-2d26-48b8-b8d1-4228fb90cabc · inbound
Numerical study on the robustness of the stability for stable black holes Significance of Black Hole Quasinormal Modes: A Closer Look
Reference 24
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 34d7204b-8f67-4d10-9c5d-8252fc006090 · inbound
Reflectionless and echo modes in asymmetric Damour-Solodukhin wormholes Significance of Black Hole Quasinormal Modes: A Closer Look
Reference 10
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 8a29d1e2-d467-478b-b372-4ede7245c0bc · inbound
Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors Significance of Black Hole Quasinormal Modes: A Closer Look
Reference 53
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 5e868813-bd74-4933-aa4a-33c4152e512c · inbound
Spectroscopy of analogue black holes using simulation-based inference Significance of Black Hole Quasinormal Modes: A Closer Look
Reference 72
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 83ef247c-f8c7-4976-88d7-a706400eaa10 · inbound
Sensitivity of black hole spectral instability to ultraviolet perturbations Significance of Black Hole Quasinormal Modes: A Closer Look
Reference 6
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 2950bf6e-56db-4011-af7c-fe5f85f5b953 · inbound
Sensitivity of black hole spectral instability to ultraviolet perturbations Significance of Black Hole Quasinormal Modes: A Closer Look
Reference 6
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 96897f70-8248-40c4-a8e3-ddc14c49a040 · inbound
Ringdown Signatures of Dehnen Dark Matter Halos: Fluid Modes and Detectability with Space-Based Detectors Significance of Black Hole Quasinormal Modes: A Closer Look
Reference 35
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.