Paper Citation Record · LEDGER

Simulating X-ray Clusters with Adaptive Mesh Refinement

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9710186.

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

pith.paper-citation-record.v1
astro-ph/9710186 v1

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 2026-08-19T06:32:44.657259+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T18:45:25.807207Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

10
pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation a1409602-12e5-40a9-8b01-636459fcc00a · inbound

Numerical modeling the mass feeding rates onto accretion-modified stars embedded within AGN disks cites this paper.

Numerical modeling the mass feeding rates onto accretion-modified stars embedded within AGN disks Simulating X-ray Clusters with Adaptive Mesh Refinement

Reference 10

Resolution: verified exact; local_arxiv, observed 2026-08-07T15:31:49.371790Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation fd1d9ac6-6110-4d8f-9295-1dff40ebd0ea · inbound

Direct Collapse Pre-supermassive Black Hole Objects as Ly$\alpha$ Emitters cites this paper.

Direct Collapse Pre-supermassive Black Hole Objects as Ly$\alpha$ Emitters Simulating X-ray Clusters with Adaptive Mesh Refinement

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-15T18:45:25.807207Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.