Paper Citation Record · LEDGER

Observations of a Possible Transient Magnetically Arrested Accretion State in a Nearby Quasar: OQ208

As of 14 August 2026, this Paper Citation Record lists 7 of 7 outbound references and 0 inbound Pith citation observations for arXiv:2606.22845.

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

pith.paper-citation-record.v1
2606.22845 v1

Coverage vector

measured 7 of 7 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-06-26T08:34:10.052190Z

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

7 of 7 outbound references displayed

verified exact0
verified fuzzy0
unresolved5
parse uncertain0
malformed identifier2
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation bdc546db-a705-4f9a-9802-86737a8921e4 · outbound

This paper cites Uncertainty is 0.1 beam FWHM for both RA and Dec coordinates (Lister et al.

Observations of a Possible Transient Magnetically Arrested Accretion State in a Nearby Quasar: OQ208 Uncertainty is 0.1 beam FWHM for both RA and Dec coordinates (Lister et al

Reference 1

Resolution: unresolved; no resolver link, observed 2026-06-26T08:34:10.052190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 63a2fe94-b0b9-49a8-96db-921f7f52c2cd · outbound

This paper cites Uncertainty is 0.2 beam FWHM for both RA and Dec coordinates (Lister et al.

Observations of a Possible Transient Magnetically Arrested Accretion State in a Nearby Quasar: OQ208 Uncertainty is 0.2 beam FWHM for both RA and Dec coordinates (Lister et al

Reference 2

Resolution: unresolved; no resolver link, observed 2026-06-26T08:34:10.052190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation afbbcc1b-cd6a-4b0c-871e-b1da1ff89e0a · outbound

This paper cites J1 in early 1995) or low contrast with the rms noise (SW2), we add 0.1 of the FWHM of component in quadrature with the uncertainty in 2) for both RA and DEC.

Observations of a Possible Transient Magnetically Arrested Accretion State in a Nearby Quasar: OQ208 J1 in early 1995) or low contrast with the rms noise (SW2), we add 0.1 of the FWHM of component in quadrature with the uncertainty in 2) for both RA and DEC

Reference 3

Resolution: unresolved; no resolver link, observed 2026-06-26T08:34:10.052190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6f798e1-a7ad-4c6d-a510-028ef71b578c · outbound

This paper cites Our VLBA observations have an absolute ﬂux density uncertainty of 5%.

Observations of a Possible Transient Magnetically Arrested Accretion State in a Nearby Quasar: OQ208 Our VLBA observations have an absolute ﬂux density uncertainty of 5%

Reference 4

Resolution: malformed identifier; no resolver link, observed 2026-06-26T08:34:10.052190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a649888e-8bd1-433f-a54b-774ead77d4dc · outbound

This paper cites an unresolved cited work.

Observations of a Possible Transient Magnetically Arrested Accretion State in a Nearby Quasar: OQ208 Unresolved cited work

Reference 5

Resolution: unresolved; no resolver link, observed 2026-06-26T08:34:10.052190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ceb24ff0-99c8-43e9-8876-55347fd0dfeb · outbound

This paper cites The 22 GHz image is then reﬁt with one elliptical Gaussian for NE1b+NE1c.

Observations of a Possible Transient Magnetically Arrested Accretion State in a Nearby Quasar: OQ208 The 22 GHz image is then reﬁt with one elliptical Gaussian for NE1b+NE1c

Reference 6

Resolution: malformed identifier; no resolver link, observed 2026-06-26T08:34:10.052190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 17b2d437-098c-439c-8ccc-6203ac43f470 · outbound

This paper cites The 1997 VSOP data at 1.66 GHz is fromKameno et al.(2000).

Observations of a Possible Transient Magnetically Arrested Accretion State in a Nearby Quasar: OQ208 The 1997 VSOP data at 1.66 GHz is fromKameno et al.(2000)

Reference 7

Resolution: unresolved; no resolver link, observed 2026-06-26T08:34:10.052190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

No inbound Pith citation observations are available.