Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
ATLASGAL - Kinematic distances and the dense gas mass distribution of the inner Galaxy
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1503.00007.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:56.875805Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
101
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation f12a3792-809d-494a-8be6-fccde45d5817 · 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 ATLASGAL - Kinematic distances and the dense gas mass distribution of the inner Galaxy
Reference 259
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T09:41:51.034164Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 7ca1c674-18ab-4f40-a88b-783b64bc1773 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry ATLASGAL - Kinematic distances and the dense gas mass distribution of the inner Galaxy
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:56.875805Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.