Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
H$_2$ formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1711.10568.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T11:37:03.736989Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-30T05:44:18.271690Z
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 017fe272-f50a-4988-bf95-68acab4ec681 · inbound
A HINSA view of cosmic-ray ionization in IC 348 and NGC 1333: evidence for a strong low-energy cosmic-ray disparity cites this paper.
A HINSA view of cosmic-ray ionization in IC 348 and NGC 1333: evidence for a strong low-energy cosmic-ray disparity H$_2$ formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations
Reference 166
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-27T03:50:28.313602Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation e8fa5062-578a-4567-a26c-8b634e71742b · inbound
Pristine composition or size evolution: Can current dust models reproduce emissivities observed in nearby protostars? cites this paper.
Pristine composition or size evolution: Can current dust models reproduce emissivities observed in nearby protostars? H$_2$ formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations
Reference 264
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-30T05:44:18.273343Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation e7abc805-bf15-47a1-98dd-5406c8a85847 · inbound
HI envelope around the carbon star V420 Vul cites this paper.
HI envelope around the carbon star V420 Vul H$_2$ formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T11:37:03.736989Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.