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Paper Citation Record · LEDGER

Implications of different stellar spectra for the climate of tidally-locked Earth-like exoplanets

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2005.13002.

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

pith.paper-citation-record.v1
2005.13002 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 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T00:58:41.945493Z

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

27
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 47ffb903-0a92-4c3a-b613-b44de5c3ec25 · inbound

A generalised microbial cell model for methane biosignature predictions cites this paper.

A generalised microbial cell model for methane biosignature predictions Implications of different stellar spectra for the climate of tidally-locked Earth-like exoplanets

Reference 160

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T08:34:48.467361Z

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=sha256:1f61d671aebe6124e3422da249139c04323412be6aad86d431dfaeaed6f59e28

Observation fa7a1b4a-7a37-4fbb-ab60-56d2097143a7 · 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 Implications of different stellar spectra for the climate of tidally-locked Earth-like exoplanets

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-02T00:58:41.945493Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T00:58:41.945493Z digest=sha256:75d5a24cdc67948af60053e652e5074a34c2d272d326b1287cd3a283d1e40ad6