Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Evolution of the optical emission lines and the X-ray emission during the super-active stage of T CrB
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2406.01971.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T10:34:59.607072Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, 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
3
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation d4da5fe5-49d4-4670-bd29-c1f5329af28b · inbound
Modeling the high-brightness state of the recurrent nova T CrB as an enhanced mass-transfer event cites this paper.
Modeling the high-brightness state of the recurrent nova T CrB as an enhanced mass-transfer event Evolution of the optical emission lines and the X-ray emission during the super-active stage of T CrB
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T10:34:59.607072Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c6ca3bfb-4931-4522-9ab0-98246d986bc4 · inbound
The accretion-driven eruption of the recurrent nova T Corona Borealis cites this paper.
The accretion-driven eruption of the recurrent nova T Corona Borealis Evolution of the optical emission lines and the X-ray emission during the super-active stage of T CrB
Reference 30
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T18:58:08.605488Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 0c9eba71-e7ef-4ebc-8054-c1a1b457db66 · inbound
The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review cites this paper.
The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review Evolution of the optical emission lines and the X-ray emission during the super-active stage of T CrB
Reference 122
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T05:31:07.323495Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation f121ffec-cca3-457e-904e-2084b5efb29d · inbound
When will T Coronae Borealis next erupt as a nova? Constraints from recurrence, orbital phase, and accretion-state evolution cites this paper.
When will T Coronae Borealis next erupt as a nova? Constraints from recurrence, orbital phase, and accretion-state evolution Evolution of the optical emission lines and the X-ray emission during the super-active stage of T CrB
Reference 85
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:48:00.579152Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.