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Paper Citation Record · LEDGER

A new estimate of the Galactic interstellar radiation field between 0.1 microns and 1000 microns

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0507119.

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

pith.paper-citation-record.v1
astro-ph/0507119 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 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T05:32:01.616450Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-13T00:16:21.800782Z

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 7c923f66-b211-4931-aae4-12025da174a6 · inbound

Deciphering the AMS cosmic-ray positron flux cites this paper.

Deciphering the AMS cosmic-ray positron flux A new estimate of the Galactic interstellar radiation field between 0.1 microns and 1000 microns

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-14T05:32:01.616450Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T05:32:01.616450Z digest=sha256:ddab86e95b76a972aa6fb23e0dc67d7fbb82f8f98afb7ec2b83e158a46381f72

Observation 514eb0a1-0101-4dd1-8b53-96f18dcd5581 · inbound

Modeling the X-ray emission of the Boomerang nebula and implication for its potential ultrahigh-energy gamma-ray emission cites this paper.

Modeling the X-ray emission of the Boomerang nebula and implication for its potential ultrahigh-energy gamma-ray emission A new estimate of the Galactic interstellar radiation field between 0.1 microns and 1000 microns

Reference 48

Resolution
verified exact
local_arxiv, observed 2026-08-12T20:17:03.267117Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-12T20:17:03.026312Z digest=sha256:a5d7e3134aa91a200a131d6957e432ec1873167cb12b90f68c0b69ce9dc4c9e6