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Paper Citation Record · LEDGER

Magnetized Gas Clouds can Survive Acceleration by a Hot Wind

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1409.6719.

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

pith.paper-citation-record.v1
1409.6719 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 2026-08-07T06:34:17.273281+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T19:42:53.258001Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-04T18:20:03.961547Z

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 0cd2148f-371d-4c62-bf98-fc0ace50bbb6 · inbound

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 cites this paper.

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 Magnetized Gas Clouds can Survive Acceleration by a Hot Wind

Reference 57

Resolution
metadata mismatch
local_arxiv, observed 2026-07-04T18:20:03.964423Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-06-25T22:58:21.809334Z digest=sha256:2faa04ced30ec864473bfba309a48c10dc8cc319511a092aadb7b4e2a59fd897

Observation 8b7c9dd1-c031-46d3-922a-58f3a0d60ed1 · inbound

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 cites this paper.

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 Magnetized Gas Clouds can Survive Acceleration by a Hot Wind

Reference 57

Resolution
metadata mismatch
local_arxiv, observed 2026-07-04T13:19:50.174660Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-06-26T05:24:52.713752Z digest=sha256:455173f54e6a0a2ad25c3bb627ef93d23d5580fa57636d5445dfe457a1998ecd

Observation eb56a1ab-6293-4780-a881-f4d3f843f9e2 · inbound

MIGHTEE-HI: Environmental effects of cosmic filaments on extragalactic HI detections in the COSMOS and XMM-LSS fields cites this paper.

MIGHTEE-HI: Environmental effects of cosmic filaments on extragalactic HI detections in the COSMOS and XMM-LSS fields Magnetized Gas Clouds can Survive Acceleration by a Hot Wind

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-06T19:42:53.258001Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T19:42:53.258001Z digest=sha256:929fd3e4d77a8c169e0c270465aa77b2aab844600db3f27178e37883bac49fc3