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Paper Citation Record · LEDGER

H$_2$O abundances and cloud properties in ten hot giant exoplanets

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1811.00011.

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

pith.paper-citation-record.v1
1811.00011 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 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T00:59:13.276788Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T05:46:40.784541Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 9c4c2e16-819a-4d7c-a7ac-7bb042301874 · inbound

The Mid-Infrared Transmission Spectrum of the Temperate Sub-Neptune TOI-270 d cites this paper.

The Mid-Infrared Transmission Spectrum of the Temperate Sub-Neptune TOI-270 d H$_2$O abundances and cloud properties in ten hot giant exoplanets

Reference 285

Resolution
verified exact
local_arxiv, observed 2026-07-02T05:46:40.786418Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:363a22a525918b4c6ee929bc9fe258db38ad14bd6cedd6585c1d8cffe63dcf60

Observation abcd5afc-9002-49c4-b91b-bcb124ccff2c · 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 H$_2$O abundances and cloud properties in ten hot giant exoplanets

Reference 279

Resolution
unresolved
no resolver link, observed 2026-08-02T00:59:13.276788Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T00:59:13.276788Z digest=sha256:6fc79ee2e4862b0cbdd23c9c291640ac3b4dceb75fa0d35bd3b88d40398dfff8