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Paper Citation Record · LEDGER

The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1102.4618.

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

pith.paper-citation-record.v1
1102.4618 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T15:21:47.739200Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T04:03:05.675371Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 cd9a6bf7-c2c9-433a-9a26-30d641f14456 · inbound

The ${}^{13}\mathrm{CO}(2{-}1)/^{12}\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud cites this paper.

The ${}^{13}\mathrm{CO}(2{-}1)/^{12}\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group

Reference 83

Resolution
verified exact
local_arxiv, observed 2026-05-19T20:17:45.241257Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:01e88e36496c9c800881d644b2ffcff864a687902d23dee7c813c0a702516d4e

Observation 73bc62a9-c025-41e7-9e64-426867c8ee3c · inbound

MSA-3D: Rotation Curves and Dark Matter Fractions at z~0.5-1.7 with JWST/NIRSpec cites this paper.

MSA-3D: Rotation Curves and Dark Matter Fractions at z~0.5-1.7 with JWST/NIRSpec The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group

Reference 228

Resolution
verified exact
local_arxiv, observed 2026-06-29T04:03:05.676745Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:886e396cb5c6a8e76be866d367d99b1cf83bd9567b0d75ba19f5cd93bad7f5d9

Observation cdf830e3-0106-49fa-bfa6-f28a530ca5f5 · inbound

Survival is not Enough: Dust Sputtering, Growth, and H$_2$ Formation in Galactic Winds cites this paper.

Survival is not Enough: Dust Sputtering, Growth, and H$_2$ Formation in Galactic Winds The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group

Reference 181

Resolution
unresolved
no resolver link, observed 2026-07-11T06:21:15.541076Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:21:15.541076Z digest=sha256:81745aaf6c9173bf3195259adef000023bf6f9550db85c311acfbf6320f8da41

Observation a02efe26-de19-4823-9d8b-9c221ab3adff · inbound

Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension cites this paper.

Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group

Reference 233

Resolution
unresolved
no resolver link, observed 2026-08-01T15:30:04.805324Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T15:30:04.805324Z digest=sha256:65b1543d5af330f46534d2aae7321aea2cb629062291edbb58fc79c30c2d9470

Observation eeae77ce-2137-4f29-8dba-9a52e8dfc5b3 · inbound

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud cites this paper.

Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-08T15:21:47.739200Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T15:21:47.739200Z digest=sha256:87c7e09a9f774b34e0859a0b4f1aee29c19358cc196b1ceda6abe2c4f721b8aa