Pith. sign in

Paper Citation Record · LEDGER

MHD Accretion-Disk Winds as X-ray Absorbers in AGNs

As of 28 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0910.3001.

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

pith.paper-citation-record.v1
0910.3001 v2

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 2026-07-28T06:31:03.373048+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-12T03:29:42.101488Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T00:46:40.210705Z

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 b5118602-6fc7-4830-87d7-6aa06dbeeac4 · inbound

Unification models of Active Galactic Nuclei cites this paper.

Unification models of Active Galactic Nuclei MHD Accretion-Disk Winds as X-ray Absorbers in AGNs

Reference 62

Resolution
verified exact
local_arxiv, observed 2026-06-27T09:20:47.527217Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-28T06:31:03.373048+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:db993ee4940e4fd61544cb52cb34d55fbcc5d22ab15151fdb5ea6ffd3e952da3

Observation 400ef722-2c2a-45db-bfe2-d76361952a46 · inbound

Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference cites this paper.

Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference MHD Accretion-Disk Winds as X-ray Absorbers in AGNs

Reference 171

Resolution
unresolved
no resolver link, observed 2026-07-12T03:29:42.101488Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T03:29:42.101488Z digest=sha256:e9c27301c6756f7f001d3071ad597d1548199a36d408537e78baafdc7266be6c

Observation 337bb1ec-9a20-4eab-8ddf-e8af1c44636b · inbound

First detection of ultra-fast outflows in a quiescent galaxy cites this paper.

First detection of ultra-fast outflows in a quiescent galaxy MHD Accretion-Disk Winds as X-ray Absorbers in AGNs

Reference 67

Resolution
verified exact
local_arxiv, observed 2026-07-10T00:46:40.211985Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-28T06:31:03.373048+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6c6fb8cc31d35612f95830e7a457926e407faad94ed3d507e8cad774cefe9a36