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Paper Citation Record · LEDGER

LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1706.07807.

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

pith.paper-citation-record.v1
1706.07807 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T18:48:49.405605Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 61417c07-71e9-4e89-9360-42b777e3b5b4 · inbound

TOI-2147 b and TOI-6019 b: Two eccentric warm Jupiters detected and characterized with TESS and MaHPS cites this paper.

TOI-2147 b and TOI-6019 b: Two eccentric warm Jupiters detected and characterized with TESS and MaHPS LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements

Reference 133

Resolution
metadata mismatch
local_arxiv, observed 2026-06-26T17:29:38.225097Z

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=sha256:458584117c170f1902fc183c5fa11420bb65cb76f6940c7ed92a62cd6ea228a9

Observation 00511c95-2cd0-4f14-857d-fdbbcc5a157d · inbound

The GAPS Programme at TNG LXXIV. A reanalysis of the planetary systems TOI-1272 and TOI-1694 with HARPS-N and retraction of the planetary interpretation of TOI-1272 c cites this paper.

The GAPS Programme at TNG LXXIV. A reanalysis of the planetary systems TOI-1272 and TOI-1694 with HARPS-N and retraction of the planetary interpretation of TOI-1272 c LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements

Reference 62

Resolution
metadata mismatch
local_arxiv, observed 2026-06-26T13:19:29.776116Z

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=sha256:41ec9abc74093fb525642b44ab19d565431a912c48d92295d9ed96d0a82980f9

Observation 6b7a7421-c306-4420-bd1a-ddbb10c4e371 · inbound

The GAPS Programme at TNG LXXIV. A reanalysis of the planetary systems TOI-1272 and TOI-1694 with HARPS-N and retraction of the planetary interpretation of TOI-1272 c cites this paper.

The GAPS Programme at TNG LXXIV. A reanalysis of the planetary systems TOI-1272 and TOI-1694 with HARPS-N and retraction of the planetary interpretation of TOI-1272 c LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements

Reference 62

Resolution
metadata mismatch
local_arxiv, observed 2026-07-02T22:07:25.608859Z

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=sha256:9e78d9e76892caffd27787f2a9879f1d0067fdffe183442d8205dbce5e266fdf

Observation fc580878-12f6-4db8-b2fe-4adc05dfd9df · inbound

Discovery of an Inflated Hot Neptune and Its Formation from Jovian Mass Loss cites this paper.

Discovery of an Inflated Hot Neptune and Its Formation from Jovian Mass Loss LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements

Reference 161

Resolution
metadata mismatch
local_arxiv, observed 2026-07-03T18:48:49.406965Z

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=sha256:3aa7ceb758b0083d0f068a7458d723368debb97c60cdee1717eac9a3e727f61d