Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Chemistry in Infrared Dark Cloud Clumps: a Molecular Line Survey at 3 mm
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1206.6500.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T04:45:22.761165Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-28T09:41:50.701287Z
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 079f5beb-013e-4309-a40b-94c4cd2b7096 · inbound
Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation cites this paper.
Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Chemistry in Infrared Dark Cloud Clumps: a Molecular Line Survey at 3 mm
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T04:45:22.761165Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ac05e155-6f75-4a86-a15d-c2f03684bda3 · inbound
A nine-member protostellar system forming via filament fragmentation in the high mass protocluster NGC 6334-43 cites this paper.
A nine-member protostellar system forming via filament fragmentation in the high mass protocluster NGC 6334-43 Chemistry in Infrared Dark Cloud Clumps: a Molecular Line Survey at 3 mm
Reference 151
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T09:41:50.702963Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.