Paper Citation Record · LEDGER

The contribution of AGNs to the X-ray background

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/9409067.

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

pith.paper-citation-record.v1
astro-ph/9409067 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T22:40:00.189753Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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External citation measurements

54
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 6a9e50ae-6827-4365-b4da-bdc96aa24a17 · inbound

Chandra Follow-up Observations of Swift-BAT-selected AGNs III cites this paper.

Chandra Follow-up Observations of Swift-BAT-selected AGNs III The contribution of AGNs to the X-ray background

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-09T22:40:00.189753Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ca372120-11b0-4545-a5c7-f5703da9e20f · inbound

X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population cites this paper.

X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population The contribution of AGNs to the X-ray background

Reference 29

Resolution: metadata mismatch; local_arxiv, observed 2026-07-03T11:28:04.898363Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation f6bd306c-b63d-4e1d-99e9-e552e4403616 · inbound

An intrinsic decline of accretion activity in GRS 1915+105 cites this paper.

An intrinsic decline of accretion activity in GRS 1915+105 The contribution of AGNs to the X-ray background

Reference 60

Resolution: verified exact; local_arxiv, observed 2026-07-08T13:54:58.369397Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 758c861d-3241-4e36-975e-30a8db39be8a · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ The contribution of AGNs to the X-ray background

Reference 275

Resolution: unresolved; no resolver link, observed 2026-08-01T06:58:59.773837Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a3753418-02c2-479b-a050-c93a85cd0b99 · 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 The contribution of AGNs to the X-ray background

Reference 135

Resolution: unresolved; no resolver link, observed 2026-07-31T05:23:38.527343Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.