Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte-Carlo approach
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2006.13596.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T05:18:38.391862Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-13T14:39:39.560747Z
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 feb2b540-11a2-4391-b7dd-42d1711b5d68 · inbound
Physics of Strong Magnetism with eXTP cites this paper.
Physics of Strong Magnetism with eXTP Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte-Carlo approach
Reference 49
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T05:18:38.391862Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6a6c5fe0-4b92-4a6c-90a2-502e77b1d9ab · inbound
Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared cites this paper.
Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte-Carlo approach
Reference 42
- Resolution
- verified exact
- local_arxiv, observed 2026-07-13T14:39:39.562564Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 22fcb6bc-2dde-49de-8238-0802a18f281c · inbound
Magnetospheric flows in X-ray pulsars II: Heating, cooling and ionization degree at sub-critical accretion cites this paper.
Magnetospheric flows in X-ray pulsars II: Heating, cooling and ionization degree at sub-critical accretion Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte-Carlo approach
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T12:29:39.967082Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.