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Paper Citation Record · LEDGER

Radiation-Hydrodynamic Simulations of Protostellar Outflows: Synthetic Observations and Data Comparisons

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1110.5640.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1110.5640 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T14:19:20.249424Z

measured 1 of 1 external citation measurements

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

74
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation cda02693-603c-41fc-a361-509c9cc18e49 · inbound

The Accretion Process on Protostars cites this paper.

The Accretion Process on Protostars Radiation-Hydrodynamic Simulations of Protostellar Outflows: Synthetic Observations and Data Comparisons

Reference 183

Resolution
verified exact
local_arxiv, observed 2026-05-14T18:42:35.524013Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7d11dec03e03590a437a9cda53bd93a0de3660464e79d3baf46ba0b8beebccc5

Observation c7f27fe8-9ca8-4062-863e-e9353bdb9938 · 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 Radiation-Hydrodynamic Simulations of Protostellar Outflows: Synthetic Observations and Data Comparisons

Reference 142

Resolution
verified exact
local_arxiv, observed 2026-06-28T09:41:50.633070Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c0a19ed7fc9585faefe040ab86ef9b8a155368dee17b8b9d1f623d29f2bb9d94

Observation c6db6271-2d3e-43c7-a0f1-f35a5ec2b197 · inbound

Asymmetry in the protostellar system HOPS 198: Evidence for the evolution of outflow opening angle driven by density of the surrounding core cites this paper.

Asymmetry in the protostellar system HOPS 198: Evidence for the evolution of outflow opening angle driven by density of the surrounding core Radiation-Hydrodynamic Simulations of Protostellar Outflows: Synthetic Observations and Data Comparisons

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-06T14:19:20.249424Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T14:19:20.249424Z digest=sha256:7de9d1280cc36479322b4d601f1c935c1710e67da37d73fdb639e59b825374c4