Paper Citation Record · LEDGER

Absolute measurement of the unresolved cosmic X-ray background in the 0.5-8 keV band with Chandra

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0512542.

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

pith.paper-citation-record.v1
astro-ph/0512542 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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:15:20.749166Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T04:15:22.678837Z

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 bf9ba3de-a774-4d8f-b3c9-84fc71dede3d · inbound

X-ray Absorption Variability in NGC 1142: Another Constraint on the Nature of the Torus/Broad-Line Region in Active Galactic Nuclei cites this paper.

X-ray Absorption Variability in NGC 1142: Another Constraint on the Nature of the Torus/Broad-Line Region in Active Galactic Nuclei Absolute measurement of the unresolved cosmic X-ray background in the 0.5-8 keV band with Chandra

Reference 127

Resolution: unresolved; no resolver link, observed 2026-07-31T05:23:38.466002Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6dc17e27-5626-4a17-b71b-ed4857d0d343 · inbound

Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations cites this paper.

Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations Absolute measurement of the unresolved cosmic X-ray background in the 0.5-8 keV band with Chandra

Reference 53

Resolution: verified exact; local_arxiv, observed 2026-08-10T04:15:22.683860Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.