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Paper Citation Record · LEDGER

Wind Interaction Models for Gamma-Ray Burst Afterglows: The Case for Two Types of Progenitors

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/9908272.

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

pith.paper-citation-record.v1
astro-ph/9908272 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 2026-08-17T06:30:58.91139+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T06:14:07.500870Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T08:07:44.836561Z

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 d3a9eb45-9728-4693-bb1a-a510239d11fe · inbound

Colour evolution in the radio afterglow of GRB 241025A cites this paper.

Colour evolution in the radio afterglow of GRB 241025A Wind Interaction Models for Gamma-Ray Burst Afterglows: The Case for Two Types of Progenitors

Reference 124

Resolution
verified exact
local_arxiv, observed 2026-07-03T08:07:44.838223Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d92180b72f2238d6716914c6d56b18edf91d658c039c41aa74712bb705087f17

Observation af9b3de6-60ff-46bc-9047-788416efaa3a · inbound

Fe K$\alpha$ line from the Broad Line Region of PDS456 with XRISM/Resolve cites this paper.

Fe K$\alpha$ line from the Broad Line Region of PDS456 with XRISM/Resolve Wind Interaction Models for Gamma-Ray Burst Afterglows: The Case for Two Types of Progenitors

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-02T06:14:07.500870Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T06:14:07.500870Z digest=sha256:9aab67ee22342403787cbea1b2a36370aa1e7f7738fe7072b8e8a92b79adbad4

Observation e02af768-a285-45ac-85fd-ada0ddf3a4d0 · inbound

Polarization of impulsive relativistic jets propagating in a stratified medium cites this paper.

Polarization of impulsive relativistic jets propagating in a stratified medium Wind Interaction Models for Gamma-Ray Burst Afterglows: The Case for Two Types of Progenitors

Reference 229

Resolution
unresolved
no resolver link, observed 2026-08-01T09:53:04.420933Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T09:53:04.420933Z digest=sha256:bb6adc4a5d1ada51fb9ee9a572a353be776f461f08e2c87a79dfe2673cd843ce