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 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T05:30:09.947740Z
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 b7f2f3fe-e964-451a-9429-161c3d20e1ba · inbound
Is the Symbiotic Recurrent Nova T CrB Late? Recent Photometric Evolution and Comparison with Past Pre-Outburst Behaviour cites this paper.
Is the Symbiotic Recurrent Nova T CrB Late? Recent Photometric Evolution and Comparison with Past Pre-Outburst Behaviour Evolution of the optical emission lines and the X-ray emission during the super-active stage of T CrB
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T05:30:09.947740Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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 bd9ff1c4-b1f5-41dd-a35e-26b0425fff86 · inbound
New symbiotic stars or candidates in LAMOST low resolution spectra cites this paper.
New symbiotic stars or candidates in LAMOST low resolution spectra Evolution of the optical emission lines and the X-ray emission during the super-active stage of T CrB
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T17:55:28.571755Z
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 2026-08-18T06:34:40.430872+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 2026-08-18T06:34:40.430872+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.