Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Dissecting a disk-instability outburst in a symbiotic star: $NuSTAR$, and $Swift$ observations of T Coronae Borealis during the rise to the "super-active" state
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1906.04770.
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 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T12:05:08.607971Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-14T12:05:09.140220Z
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 74dc11d3-b583-4ca6-932c-863643074435 · inbound
XMM-Newton observations of the symbiotic recurrent nova T CrB: evolution of X-ray emission during the active phase cites this paper.
XMM-Newton observations of the symbiotic recurrent nova T CrB: evolution of X-ray emission during the active phase Dissecting a disk-instability outburst in a symbiotic star: $NuSTAR$, and $Swift$ observations of T Coronae Borealis during the rise to the "super-active" state
Reference 20
- Resolution
- verified exact
- local_arxiv, observed 2026-08-14T12:05:09.146064Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 147a9ef7-d818-4c8c-b4d0-69c6385b3393 · 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 Dissecting a disk-instability outburst in a symbiotic star: $NuSTAR$, and $Swift$ observations of T Coronae Borealis during the rise to the "super-active" state
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:47:55.954572Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.