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Paper Citation Record · LEDGER

Self-similarity and scaling behavior of IR emission from radiatively heated dust: I. Theory

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/9612164.

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

pith.paper-citation-record.v1
astro-ph/9612164 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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:47:23.700912Z

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

418
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation fbfd32fc-b832-466b-83dd-df9157278e69 · inbound

Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation cites this paper.

Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation Self-similarity and scaling behavior of IR emission from radiatively heated dust: I. Theory

Reference 168

Resolution
verified exact
local_arxiv, observed 2026-06-26T09:59:18.158776Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:849eb8421bc869545e75e6b62dd17183cf9de751f46ae3537e5c9c589bfadb14

Observation c21b1e1b-1341-4914-8d60-e70d08a2bf80 · inbound

JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf cites this paper.

JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf Self-similarity and scaling behavior of IR emission from radiatively heated dust: I. Theory

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-14T13:47:23.700912Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:47:23.700912Z digest=sha256:c0c8801f1d13589331d35451da33dc057da9cd0d37b2c0a6bab85c1a57f4c6cd