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Paper Citation Record · LEDGER

Treatment of overlapping gaseous absorption with the correlated-k method in hot Jupiter and brown dwarf atmosphere models

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1610.01389.

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

pith.paper-citation-record.v1
1610.01389 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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T00:59:04.109928Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T06:46:51.929279Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 938ca39e-4522-40aa-bd71-45d96f109d62 · inbound

Phase-dependent chemistry of WASP-43 b revealed with a suite of one-, two-, and three-dimensional models cites this paper.

Phase-dependent chemistry of WASP-43 b revealed with a suite of one-, two-, and three-dimensional models Treatment of overlapping gaseous absorption with the correlated-k method in hot Jupiter and brown dwarf atmosphere models

Reference 13

Resolution
verified exact
local_arxiv, observed 2026-07-10T06:46:51.930565Z

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:f1ec2c28792273c712e5c3742de366cc86c86ab03821f30392bade48444b25b0

Observation cab5cbc5-8298-450b-95c7-d3ca25621e24 · inbound

Flow-Driven Limb-Asymmetry of Haze Distribution Part I: An Analytical Framework for Predicting the Size Distribution of Photochemical Hazes Across the Two Limbs of hot-Jupiters cites this paper.

Flow-Driven Limb-Asymmetry of Haze Distribution Part I: An Analytical Framework for Predicting the Size Distribution of Photochemical Hazes Across the Two Limbs of hot-Jupiters Treatment of overlapping gaseous absorption with the correlated-k method in hot Jupiter and brown dwarf atmosphere models

Reference 199

Resolution
unresolved
no resolver link, observed 2026-08-02T00:59:04.109928Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T00:59:04.109928Z digest=sha256:b87650b0fa10bb05f621493d83315f5ef9f57ce8faeb06aa72f8eeb09166ef66