Pith. sign in

Paper Citation Record · LEDGER

On the Physical Origin of OVI Absorption-Line Systems

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0205556.

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

pith.paper-citation-record.v1
astro-ph/0205556 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T10:19:02.451272Z

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
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

129
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation aaca919d-dd48-4b61-ad0c-5ecb148300ac · inbound

CRexit observed: probing cosmic ray transport in the circumgalactic medium with absorption line spectra cites this paper.

CRexit observed: probing cosmic ray transport in the circumgalactic medium with absorption line spectra On the Physical Origin of OVI Absorption-Line Systems

Reference 266

Resolution
verified exact
local_arxiv, observed 2026-07-10T22:17:37.339462Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7bb3231276ea2842c9c264757050c015305b0e6df8f80e8315c608ee3efd52ab

Observation 8becab21-0bac-451a-9105-739ab8cc523f · inbound

On the Origin of the Ly$\alpha$ Damping Wing in Galaxies at $8\le z \le 10$: Explorations using the NINJA Simulations cites this paper.

On the Origin of the Ly$\alpha$ Damping Wing in Galaxies at $8\le z \le 10$: Explorations using the NINJA Simulations On the Physical Origin of OVI Absorption-Line Systems

Reference 216

Resolution
unresolved
no resolver link, observed 2026-08-08T16:24:48.168698Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T16:24:48.168698Z digest=sha256:d171b859e8e7c19974014732118fce2403af8791a4c1619f51cc1a0a9efd0541

Observation 1d889473-030e-4b1d-80fc-e734049bfb53 · inbound

An emerging baryon cycle in a galaxy 500 million years after the Big Bang cites this paper.

An emerging baryon cycle in a galaxy 500 million years after the Big Bang On the Physical Origin of OVI Absorption-Line Systems

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-11T10:19:02.451272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T10:19:02.451272Z digest=sha256:2279ca2f5c1ae655a1c084a77d5c6b941b94661d47c26c2b0ef37e7c908751d4