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Paper Citation Record · LEDGER

Testing the origin of ~3.55 keV line in individual galaxy clusters observed with XMM-Newton

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1508.05186.

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

pith.paper-citation-record.v1
1508.05186 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 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T11:51:12.506127Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T11:29:09.202249Z

Reference resolution

0 of 0 outbound references displayed

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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 5f105102-3c9b-4431-96d6-0a02fe4d8d4f · inbound

Revisiting the expected Micro-X signal from the 3.5 keV line cites this paper.

Revisiting the expected Micro-X signal from the 3.5 keV line Testing the origin of ~3.55 keV line in individual galaxy clusters observed with XMM-Newton

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-14T11:51:12.506127Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:51:12.506127Z digest=sha256:551f9a9e19b752be083845c398f046426337278921212e5d86a83c0c811e6173

Observation acdb3d63-1d39-43d3-9fdc-4e2101271286 · inbound

NuSTAR Tests of Sterile-Neutrino Dark Matter: New Galactic Bulge Observations and Combined Impact cites this paper.

NuSTAR Tests of Sterile-Neutrino Dark Matter: New Galactic Bulge Observations and Combined Impact Testing the origin of ~3.55 keV line in individual galaxy clusters observed with XMM-Newton

Reference 64

Resolution
verified exact
local_arxiv, observed 2026-08-14T11:29:09.207799Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-08-14T11:29:07.445769Z digest=sha256:58f6c5a9d95973bcb101686cf9e2410f21685048ff9bc07c6a9ee56e0c4c588d