Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A 400 solar mass black hole in the Ultraluminous X-ray source M82 X-1 accreting close to its Eddington limit
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1501.03180.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T10:29:38.759074Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-30T19:55:01.772486Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 428caddb-9928-4901-b155-c47be5eadc65 · inbound
Testing loop quantum gravity by quasi-periodic oscillations: rotating blackholes cites this paper.
Testing loop quantum gravity by quasi-periodic oscillations: rotating blackholes A 400 solar mass black hole in the Ultraluminous X-ray source M82 X-1 accreting close to its Eddington limit
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T10:29:38.759074Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4ddca758-188e-43f3-a420-5fa7fdf8671c · inbound
Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers cites this paper.
Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers A 400 solar mass black hole in the Ultraluminous X-ray source M82 X-1 accreting close to its Eddington limit
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T13:27:10.103171Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 81fd7be8-f6d0-4fb2-a964-b9095a9085c1 · inbound
Probing the Strong Gravity Region of Black Holes with eXTP cites this paper.
Probing the Strong Gravity Region of Black Holes with eXTP A 400 solar mass black hole in the Ultraluminous X-ray source M82 X-1 accreting close to its Eddington limit
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T05:24:43.917047Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d3d44c51-b351-4c52-a3d3-daccecbb7855 · inbound
Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts cites this paper.
Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts A 400 solar mass black hole in the Ultraluminous X-ray source M82 X-1 accreting close to its Eddington limit
Reference 68
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T17:28:48.029113Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 455954ba-ce9a-4081-8492-40d3e9119c26 · inbound
Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts cites this paper.
Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts A 400 solar mass black hole in the Ultraluminous X-ray source M82 X-1 accreting close to its Eddington limit
Reference 71
- Resolution
- verified exact
- local_arxiv, observed 2026-06-30T19:55:01.773924Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.