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Paper Citation Record · LEDGER

Resolving galaxy cluster gas properties at z~1 with XMM-Newton and Chandra

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1610.01899.

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

pith.paper-citation-record.v1
1610.01899 v2

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 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:52:13.948513Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T23:57:43.928627Z

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 ffe24092-ccdd-46b6-83be-0ce161a9e28c · inbound

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

The Treble Clef radio phoenix and its old nonthermal filaments Resolving galaxy cluster gas properties at z~1 with XMM-Newton and Chandra

Reference 263

Resolution
metadata mismatch
local_arxiv, observed 2026-07-10T23:57:43.944650Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:62773b5b30b37d8e9da7a5d2ad974e47cca99b66299e39a5e47ef559722f2c8e

Observation aed1c4ac-3ca6-440a-b744-f127745aa095 · 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 Resolving galaxy cluster gas properties at z~1 with XMM-Newton and Chandra

Reference 263

Resolution
unresolved
no resolver link, observed 2026-08-02T02:52:13.948513Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:52:13.948513Z digest=sha256:716fe86fd4320cfea001215f801b93e84c4a310c1f72d75fa1db8e69f769e56b