Pith. sign in

Paper Citation Record · LEDGER

Unraveling the collision scenario of the dissociative galaxy cluster Abell 56 through hydrodynamic simulations

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2401.15044.

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

pith.paper-citation-record.v1
2401.15044 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:51:54.298723Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T23:57:44.098622Z

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 a143d583-5711-4e37-a092-0715380382b5 · inbound

The Treble Clef radio phoenix and its old nonthermal filaments cites this paper.

The Treble Clef radio phoenix and its old nonthermal filaments Unraveling the collision scenario of the dissociative galaxy cluster Abell 56 through hydrodynamic simulations

Reference 84

Resolution
metadata mismatch
local_arxiv, observed 2026-07-10T23:57:44.114890Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:cf76c725a8f7b652ab3b69d1a7d99859651bb9d7a8f7a28dcc1f6952c9e8d362

Observation d592fa2a-c7a7-4956-900a-9401c11c6382 · inbound

The topology of the magnetic field in Abell 2255 out to its virial radius. Results from the LOFAR Galaxy Cluster Ultra-Deep Field cites this paper.

The topology of the magnetic field in Abell 2255 out to its virial radius. Results from the LOFAR Galaxy Cluster Ultra-Deep Field Unraveling the collision scenario of the dissociative galaxy cluster Abell 56 through hydrodynamic simulations

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-02T02:51:54.298723Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:51:54.298723Z digest=sha256:294ac8f03f338e3cc2a70d356eedb90ba3ad31f1f9c8817773c2f745c9a9a89c