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Paper Citation Record · LEDGER

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions

As of 22 August 2026, this Paper Citation Record lists 22 of 22 outbound references and 0 inbound Pith citation observations for arXiv:1908.05909.

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

pith.paper-citation-record.v1
1908.05909 v1

Coverage vector

measured 22 of 22 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:05:59.597764Z

measured 22 of 22 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

22 of 22 outbound references displayed

  • verified exact1
  • verified fuzzy12
  • unresolved9
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  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation ce36113d-3762-4d69-b7fb-a832f4086765 · outbound

This paper cites Kodama1,2, H.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Kodama1,2, H

Reference 1

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verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation a625d70a-1445-4848-8486-a8eb99d675c9 · outbound

This paper cites an unresolved cited work.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Unresolved cited work

Reference 2

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unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation a840d87b-f7ea-4fee-bfe2-898fe2083493 · outbound

This paper cites an unresolved cited work.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Unresolved cited work

Reference 3

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 6abc263f-9cef-4044-8c78-832f93f0adcb · outbound

This paper cites Thus, it is necessary to carefully consider the relationship between the runaway threshold and the water distribution on more realistic planets with oceans.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Thus, it is necessary to carefully consider the relationship between the runaway threshold and the water distribution on more realistic planets with oceans

Reference 4

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 7802e068-6959-4e73-9097-41470e484641 · outbound

This paper cites In Section 6, we summarize our findings.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions In Section 6, we summarize our findings

Reference 5

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verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation db7b36e5-ecf8-4373-9ae5-dfdd03816fba · outbound

This paper cites This GCM was developed for the modeling of the present Earth’s climate [Numaguchi, 1999] and was applied to the paleoclimate of Earth [Abe-Ouchi et al., 2013].

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions This GCM was developed for the modeling of the present Earth’s climate [Numaguchi, 1999] and was applied to the paleoclimate of Earth [Abe-Ouchi et al., 2013]

Reference 6

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation b0b9b5fd-1c80-42db-840d-1dff775fd1a7 · outbound

This paper cites the dispersed case.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions the dispersed case

Reference 7

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation fe0e127d-2702-4342-87ae-648095605eb1 · outbound

This paper cites Climate in this case is still stable.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Climate in this case is still stable

Reference 9

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verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 01367c28-6a6e-46e4-b3e9-17450ac45c46 · outbound

This paper cites an unresolved cited work.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Unresolved cited work

Reference 10

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 381eafc6-7ea8-441f-aa0d-684c65787113 · outbound

This paper cites The runaway threshold decreases with the increase in the number of grids of the water pool region.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions The runaway threshold decreases with the increase in the number of grids of the water pool region

Reference 11

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 64dec1b5-5580-446f-a7b2-3a8ce38bbd27 · outbound

This paper cites The runaway thresholds for the meridionally uniform surface water distribution is quite a lot lower than that for the zonally uniform case.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions The runaway thresholds for the meridionally uniform surface water distribution is quite a lot lower than that for the zonally uniform case

Reference 12

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 9b47cfd3-06aa-4b3f-a9c3-063c39b2c50e · outbound

This paper cites an unresolved cited work.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Unresolved cited work

Reference 15

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 50513cd7-08f7-4816-b455-a6f97ae56bb1 · outbound

This paper cites 43 0-3 C.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions 43 0-3 C

Reference 16

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No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 51d7f948-92fe-433b-8944-3269131d3b38 · outbound

This paper cites an unresolved cited work.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Unresolved cited work

Reference 17

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unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation e069b3e0-b6a0-45af-b688-6aca0484f653 · outbound

This paper cites MCFEP 1ʷ 1ʷ 1ʷ.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions MCFEP 1ʷ 1ʷ 1ʷ

Reference 18

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verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 16004523-abe0-4fc1-898b-b02eb78fa98f · outbound

This paper cites Therefore, we showed a range of possible runaway thresholds depending on the surface water distribution.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Therefore, we showed a range of possible runaway thresholds depending on the surface water distribution

Reference 20

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation c05444e6-af47-4a33-b150-4c498d5ad25e · outbound

This paper cites an unresolved cited work.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Unresolved cited work

Reference 24

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unresolved
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No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 488f1588-fb2a-4f11-820b-8b85b3be578c · outbound

This paper cites an unresolved cited work.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Unresolved cited work

Reference 84

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unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 5a67d2ce-81e3-4446-a660-7121cb4a4327 · outbound

This paper cites an unresolved cited work.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Unresolved cited work

Reference 1992

Resolution
unresolved
raw_fallback, observed 2026-08-14T13:06:00.032167Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 61731549-ca6d-448c-b8be-251bd9dc3f20 · outbound

This paper cites an unresolved cited work.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions Unresolved cited work

Reference 2006

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 34d76ee7-b567-4695-bd6c-98a366d929ac · outbound

This paper cites They assumed the typical amount of water on the surface of a land planet to be 5% of VOCE based on a result from Abe et al.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions They assumed the typical amount of water on the surface of a land planet to be 5% of VOCE based on a result from Abe et al

Reference 2015

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Observation 0c05dce3-2cfa-4c9d-b6cd-96445fd2b67f · outbound

This paper cites an aqua planet.

Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions an aqua planet

Reference 2018

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T13:06:00.004983Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

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Pith citing papers

No inbound Pith citation observations are available.