Paper Citation Record · LEDGER

Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2302.02611.

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

pith.paper-citation-record.v1
2302.02611 v3

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T13:19:27.883914Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-13T01:29:14.366046Z

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3aac6f83-1c09-4d81-a9f7-8d413954b3cc · inbound

HD 148797: A bright F-type star with two moderate-period low-density sub-Jovian planets. Compact multi-planet architectures are common in the Neptunian savanna cites this paper.

HD 148797: A bright F-type star with two moderate-period low-density sub-Jovian planets. Compact multi-planet architectures are common in the Neptunian savanna Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra

Reference 147

Resolution: verified exact; local_arxiv, observed 2026-07-13T01:29:14.370238Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 7eb8233e-488e-4abb-895b-fb090b7d6c2e · inbound

Identifying and Determining Atmospheric Parameters of BHB Stars Based on LAMOST DR11 cites this paper.

Identifying and Determining Atmospheric Parameters of BHB Stars Based on LAMOST DR11 Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-01T13:19:27.883914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 93a9d1e9-0729-485e-8913-e9fa4224a388 · inbound

BOSS-CLAM: Utilizing a Constrained Linear Absorption Model to Infer Stellar Parameters from BOSS Spectra cites this paper.

BOSS-CLAM: Utilizing a Constrained Linear Absorption Model to Infer Stellar Parameters from BOSS Spectra Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra

Reference 165

Resolution: unresolved; no resolver link, observed 2026-08-01T04:28:48.992628Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e7547179-9ef8-4c1c-9beb-3125fc95d959 · inbound

Neighbors, Not Kin: Kinematic evidence for tidal tails from NGC 7492 along the Sagittarius stream cites this paper.

Neighbors, Not Kin: Kinematic evidence for tidal tails from NGC 7492 along the Sagittarius stream Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra

Reference 32

Resolution: unresolved; no resolver link, observed 2026-07-30T11:06:38.820825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3dcbc361-818b-48d8-8fa2-cd6d84147bfe · inbound

PANTERA. I. Hunting for the Most Metal-Rich Stars in the Solar Neighborhood with High-Resolution Spectroscopy cites this paper.

PANTERA. I. Hunting for the Most Metal-Rich Stars in the Solar Neighborhood with High-Resolution Spectroscopy Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-01T09:29:14.776972Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0475b1ab-0972-477d-b0e2-f491c1a4411a · inbound

Detecting Solar-Like Oscillations in the Highest Mass TESS Giants cites this paper.

Detecting Solar-Like Oscillations in the Highest Mass TESS Giants Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra

Reference 56

Resolution: unresolved; no resolver link, observed 2026-07-31T16:17:45.530259Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.