Paper Citation Record · LEDGER

Early SPI/INTEGRAL contraints on the morphology of the 511 keV line emission in the 4th galactic quadrant

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0309442.

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

pith.paper-citation-record.v1
astro-ph/0309442 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T12:04:37.639070Z

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

171
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 5c6cfe93-be2e-4083-9150-ed387c986c2a · inbound

Updated Constraints on the Injection Energy of Positrons Generating the Galactic 511 keV $\gamma$-ray line cites this paper.

Updated Constraints on the Injection Energy of Positrons Generating the Galactic 511 keV $\gamma$-ray line Early SPI/INTEGRAL contraints on the morphology of the 511 keV line emission in the 4th galactic quadrant

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T12:04:37.639070Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a3897e0d-93eb-4d5b-ae37-3834a228a46c · inbound

A new model of quasar mass evolution cites this paper.

A new model of quasar mass evolution Early SPI/INTEGRAL contraints on the morphology of the 511 keV line emission in the 4th galactic quadrant

Reference 50

Resolution: verified exact; local_arxiv, observed 2026-07-11T14:58:04.315186Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.