Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArT\'eMiS
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1605.07434.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-09T08:05:16.230513Z
Reference resolution
0 of 0 outbound references displayed
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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 f530a46e-f5be-4fd1-a0dd-28bcd168b8a5 · inbound
Global and Local Infall in the ASHES Sample (GLASHES). II. Asymmetric Line Profiles around Dense Cores in 70 $\mu$m Dark Massive Clumps cites this paper.
Global and Local Infall in the ASHES Sample (GLASHES). II. Asymmetric Line Profiles around Dense Cores in 70 $\mu$m Dark Massive Clumps Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArT\'eMiS
Reference 195
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-14T20:57:57.455453Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 9256e204-2bae-4ed3-9c25-56bdf6294abf · inbound
Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions cites this paper.
Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArT\'eMiS
Reference 120
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T03:59:32.253592Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation fb621fe8-a3f1-4d86-84a0-398ab34f6ca6 · inbound
Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas cites this paper.
Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArT\'eMiS
Reference 148
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-22T08:11:16.769529Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.