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Paper Citation Record · LEDGER

Mass-Radius Relationships for Solid Exoplanets

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:0707.2895.

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

pith.paper-citation-record.v1
0707.2895 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:43:30.290775Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T05:46:40.798063Z

Reference resolution

0 of 0 outbound references displayed

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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 41324d1d-e802-4432-ae53-46bb298a10af · inbound

Revisiting the Exo-Mercury Candidate GJ 367 b with ESPRESSO and a Self-Consistent Tidal Distortion Model cites this paper.

Revisiting the Exo-Mercury Candidate GJ 367 b with ESPRESSO and a Self-Consistent Tidal Distortion Model Mass-Radius Relationships for Solid Exoplanets

Reference 175

Resolution
verified exact
local_arxiv, observed 2026-06-26T22:40:10.484830Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:411b35f807886667a0159025e48aff8c9256334a9ee33f9b8da340bb1a9b40cf

Observation b8147166-8066-421e-b725-3e4607b95340 · inbound

Background-Induced Forces from Quadratically Coupled Ultralight Dark Matter cites this paper.

Background-Induced Forces from Quadratically Coupled Ultralight Dark Matter Mass-Radius Relationships for Solid Exoplanets

Reference 93

Resolution
verified exact
local_arxiv, observed 2026-07-01T15:35:48.274968Z

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.

source=pdf_text observed=2026-06-30T01:20:34.806985Z digest=sha256:47b4dd941aed71f178f30d73d1cc34eeb88012868e20d334a3b14aed7707e881

Observation 466ac1a2-47bc-4cb8-a48b-e2212a340185 · 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 Mass-Radius Relationships for Solid Exoplanets

Reference 291

Resolution
verified exact
local_arxiv, observed 2026-07-02T05:46:40.799312Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:1fd5337915e4d125c5a2bb637e2b281a906918f2858a214cc6b7a4c9bea7c564

Observation 2fc43505-c30c-473f-b8d7-86fb680b87bc · inbound

First planetesimals from DESI DR1: 12 highly metal-rich white dwarfs cites this paper.

First planetesimals from DESI DR1: 12 highly metal-rich white dwarfs Mass-Radius Relationships for Solid Exoplanets

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-02T02:43:30.290775Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:43:30.290775Z digest=sha256:55c62eb0667b4cde297b7ad17974642b5cf8e41e78225f8bfb7b65b5d7b949d9

Observation 5f0bb853-6226-4e85-bfc1-595d384db2f2 · inbound

Dynamically Selected Mass-Radius Relationship for Low Mass Exoplanets cites this paper.

Dynamically Selected Mass-Radius Relationship for Low Mass Exoplanets Mass-Radius Relationships for Solid Exoplanets

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-01T12:14:31.061998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T12:14:31.061998Z digest=sha256:0b67f48798d8649e5417454aab829f86dbfd680f92f74d2e9e272154514e439f