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Paper Citation Record · LEDGER

Constraining hydrostatic mass bias of galaxy clusters with high-resolution X-ray spectroscopy

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1507.02730.

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

pith.paper-citation-record.v1
1507.02730 v3

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

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:11:32.710249Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T00:45:48.993834Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 954f0b92-d352-473e-a3c4-1416248d910c · inbound

Voyage through the Hidden Physics of the Cosmic Web cites this paper.

Voyage through the Hidden Physics of the Cosmic Web Constraining hydrostatic mass bias of galaxy clusters with high-resolution X-ray spectroscopy

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-14T15:11:32.710249Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T15:11:32.710249Z digest=sha256:824a05fe5cffd78c1e2bfc944bd264031d54a8eb26daf29830f8ec128d2d4dd5

Observation a40fdf05-ab24-473b-9145-356478afe0fc · inbound

Correcting the hydrostatic mass for non-thermal gas motions: a comparison of two approaches cites this paper.

Correcting the hydrostatic mass for non-thermal gas motions: a comparison of two approaches Constraining hydrostatic mass bias of galaxy clusters with high-resolution X-ray spectroscopy

Reference 240

Resolution
verified exact
local_arxiv, observed 2026-07-02T07:26:45.044165Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8ee5e19cb86fd0e93fc0fcc2ba7a95f1dddf217d2f7aeab9bf61905f1788eb02

Observation df20bda0-96b7-4d53-b4f9-3ce16cb8a276 · inbound

XRISM Reveals a Kinematically Coherent Core System of the Nearby Cool-Core Cluster Abell 2199 cites this paper.

XRISM Reveals a Kinematically Coherent Core System of the Nearby Cool-Core Cluster Abell 2199 Constraining hydrostatic mass bias of galaxy clusters with high-resolution X-ray spectroscopy

Reference 24

Resolution
verified exact
local_arxiv, observed 2026-07-09T00:45:48.995140Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:814e2375a5a6e1e7871b4accb236c65d1a1a584dfcfa4162675d475e50aac714