Pith. sign in

Paper Citation Record · LEDGER

The Origin of the soft excess in AGN

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0703449.

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

pith.paper-citation-record.v1
astro-ph/0703449 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T01:57:42.447995Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

2
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation f7fd5cce-7168-49c4-80d1-89206495a860 · inbound

An X-ray and optical spectral study of the changing-look narrow-line Seyfert 1 2MASX J0413-0050 cites this paper.

An X-ray and optical spectral study of the changing-look narrow-line Seyfert 1 2MASX J0413-0050 The Origin of the soft excess in AGN

Reference 234

Resolution
verified exact
arxiv_id, observed 2026-07-04T15:00:13.099449Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-05-08T15:53:31.107603Z digest=sha256:1768c56d960c0ba3b3c45247e413d42a94b68bb474495d53027bef006942eae7

Observation 3b7338c1-c007-4420-b6fc-6f281e266954 · inbound

Comprehensive X-ray Study of Giant Radio Galaxies with XMM-Newton and Chandra cites this paper.

Comprehensive X-ray Study of Giant Radio Galaxies with XMM-Newton and Chandra The Origin of the soft excess in AGN

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-01T01:57:42.447995Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T01:57:42.447995Z digest=sha256:db30835a6040998269a8d2e625567d40e24f613d7484e8b7d8739cf8c9e3b304