Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Using Pulsars to Detect Massive Black Hole Binaries via Gravitational Radiation: Sagittarius A* and Nearby Galaxies
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0107470.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
58
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 505507f0-ec71-4d25-b05b-8bed7502c0bb · inbound
Probing Supermassive Black Hole Mergers with Pulsar Timing Arrays cites this paper.
Probing Supermassive Black Hole Mergers with Pulsar Timing Arrays Using Pulsars to Detect Massive Black Hole Binaries via Gravitational Radiation: Sagittarius A* and Nearby Galaxies
Reference 31
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T14:11:04.175746Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 0099d030-c2a6-4557-8a4e-22a6d26868e4 · inbound
Dynamics and detectability of long-lived non-accretion phases for massive black hole binaries in cold, thermally regulating disks cites this paper.
Dynamics and detectability of long-lived non-accretion phases for massive black hole binaries in cold, thermally regulating disks Using Pulsars to Detect Massive Black Hole Binaries via Gravitational Radiation: Sagittarius A* and Nearby Galaxies
Reference 205
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T08:51:49.006232Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.