Pith. sign in

Paper Citation Record · LEDGER

Modelling the dust emission from dense interstellar clouds: disentangling the effects of radiative transfer and dust properties

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1202.5966.

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

pith.paper-citation-record.v1
1202.5966 v2

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 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T21:40:32.783789Z

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

65
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation d0f109be-05ce-422a-9a34-0bf17d66392c · inbound

Tracing grain growth in the forming prestellar core L1506C with 3D modeling of Herschel, IRAM, and CFHT observations cites this paper.

Tracing grain growth in the forming prestellar core L1506C with 3D modeling of Herschel, IRAM, and CFHT observations Modelling the dust emission from dense interstellar clouds: disentangling the effects of radiative transfer and dust properties

Reference 28

Resolution
verified exact
local_arxiv, observed 2026-07-03T09:27:47.850436Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:4ec44d3ddc9eca84c1318f32021199a7beda99f8872c900500ccca6c97a3f3c6

Observation ad8154eb-e262-46d8-aa3c-1ab0c4a4be94 · inbound

Infrared spectroscopy of gas-phase hydrogenated and methylated pyrenes: from laboratory spectra to the simulated 3.4 $\mu$m emission band cites this paper.

Infrared spectroscopy of gas-phase hydrogenated and methylated pyrenes: from laboratory spectra to the simulated 3.4 $\mu$m emission band Modelling the dust emission from dense interstellar clouds: disentangling the effects of radiative transfer and dust properties

Reference 232

Resolution
unresolved
no resolver link, observed 2026-08-01T21:40:32.783789Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T21:40:32.783789Z digest=sha256:364f9e385fb529ff9170d103cc05b63dde2dcbbefbac60307cc548ef4c64dac2