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Paper Citation Record · LEDGER

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

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 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 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 2026-07-11T11:50:26.030339Z

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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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

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

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:465aea552b6429e64306072299b0cf58df952e485a5367f1fd769a8481b04196

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

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c811d30f770e97c4e6cfcc18b585499ed34695d9ea2b424e8e0cba35c4c3faea