Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
X-ray Observations of Two Type Ia Supernovae with an H$\alpha$ Line in their Optical Spectrum
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2407.00279.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T21:49:26.670022Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-14T13:47:28.301070Z
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 53c12b79-94cb-4a94-bfdf-0799f2d7d2d3 · inbound
Type Ia supernovae cites this paper.
Type Ia supernovae X-ray Observations of Two Type Ia Supernovae with an H$\alpha$ Line in their Optical Spectrum
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T20:25:19.678199Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eebaf9c1-6736-4db8-95df-ed648fa15d0e · inbound
On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars cites this paper.
On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars X-ray Observations of Two Type Ia Supernovae with an H$\alpha$ Line in their Optical Spectrum
Reference 95
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-15T21:49:26.670022Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0435e6a4-03db-424a-a9ff-0c103948d378 · inbound
JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf cites this paper.
JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf X-ray Observations of Two Type Ia Supernovae with an H$\alpha$ Line in their Optical Spectrum
Reference 193
- Resolution
- verified exact
- local_arxiv, observed 2026-08-14T13:47:28.307574Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.