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Paper Citation Record · LEDGER

An Empirical Determination of the Dust Mass Absorption Coefficient, $\kappa_{d}$, Using the Herschel Reference Survey

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1603.04860.

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

pith.paper-citation-record.v1
1603.04860 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T15:21:47.535906Z

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

52
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation fdfdef16-ee84-4c48-91ea-7a76832e7b50 · inbound

Interstellar dust production, destruction and effects of dust depletion in galaxies cites this paper.

Interstellar dust production, destruction and effects of dust depletion in galaxies An Empirical Determination of the Dust Mass Absorption Coefficient, $\kappa_{d}$, Using the Herschel Reference Survey

Reference 177

Resolution
verified exact
local_arxiv, observed 2026-05-19T09:02:13.667938Z

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=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:84a45d879f5680a047150ae194e65e973f0e9afd459725178d4b9c5c5241c4f5

Observation d7340de1-620f-496b-92be-2974cfa7add6 · inbound

COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 cites this paper.

COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 An Empirical Determination of the Dust Mass Absorption Coefficient, $\kappa_{d}$, Using the Herschel Reference Survey

Reference 149

Resolution
verified exact
local_arxiv, observed 2026-05-20T03:58:01.749633Z

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=sha256:33e190f3df506b0d2e825f68cba4c7eea67a1ea377697b959b9091be56d1d902

Observation 06fbad5b-88f3-439d-a985-17b7a003bb98 · inbound

COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 cites this paper.

COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12 An Empirical Determination of the Dust Mass Absorption Coefficient, $\kappa_{d}$, Using the Herschel Reference Survey

Reference 149

Resolution
verified exact
local_arxiv, observed 2026-05-21T07:49:49.352418Z

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=sha256:737b756f3581bd91ff1776eddf3f42bbe65810a41d1b2ef04b7ebc972dbea009

Observation 54c1f071-c8e2-4061-b3ca-46155a9d4724 · 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 An Empirical Determination of the Dust Mass Absorption Coefficient, $\kappa_{d}$, Using the Herschel Reference Survey

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-08T15:21:47.535906Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T15:21:47.535906Z digest=sha256:ab711759395f81c8d3775733d3ab8d777e23368483921678d068f7d42be1f75b