Paper Citation Record · LEDGER

The Milky Way Radial Metallicity Gradient as an Equilibrium Phenomenon: Why Old Stars are Metal-Rich

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2410.13256.

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

pith.paper-citation-record.v1
2410.13256 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T10:21:15.903425Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, 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

1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 01788382-a387-46c9-a25c-98a6010bf52c · inbound

Rediscovering the Milky Way with orbit superposition approach and APOGEE data II. Chrono-chemo-kinematics of the disc cites this paper.

Rediscovering the Milky Way with orbit superposition approach and APOGEE data II. Chrono-chemo-kinematics of the disc The Milky Way Radial Metallicity Gradient as an Equilibrium Phenomenon: Why Old Stars are Metal-Rich

Reference 126

Resolution: unresolved; no resolver link, observed 2026-08-12T12:53:26.113005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 06a2a8bd-4b3b-4054-a458-ddb63b361928 · inbound

Local variations of the radial metallicity gradient in a simulated NIHAO-UHD Milky Way analogue and their implications for (extra-)galactic studies cites this paper.

Local variations of the radial metallicity gradient in a simulated NIHAO-UHD Milky Way analogue and their implications for (extra-)galactic studies The Milky Way Radial Metallicity Gradient as an Equilibrium Phenomenon: Why Old Stars are Metal-Rich

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-12T04:43:20.791798Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 13c3adea-f4a3-4fe0-ba6f-91df80302a1e · inbound

Four Elements to Rule Them All: Abundances are Rigidly Coupled in the Milky Way Disk cites this paper.

Four Elements to Rule Them All: Abundances are Rigidly Coupled in the Milky Way Disk The Milky Way Radial Metallicity Gradient as an Equilibrium Phenomenon: Why Old Stars are Metal-Rich

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-16T10:21:15.903425Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e96d2425-41d9-4955-bffb-43a3a3268e06 · inbound

Disentangling Metallicity Effects in Hot Jupiter Occurrence Across Galactic Birth Radius and Phase-Space Density cites this paper.

Disentangling Metallicity Effects in Hot Jupiter Occurrence Across Galactic Birth Radius and Phase-Space Density The Milky Way Radial Metallicity Gradient as an Equilibrium Phenomenon: Why Old Stars are Metal-Rich

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-15T19:29:56.926187Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 07d08b52-3ec6-4e00-9981-0fbfe639e5bf · inbound

The Open Cluster Chemical Abundances and Mapping Survey: VIII. Galactic Chemical Gradient and Azimuthal Analysis from SDSS/MWM DR19 cites this paper.

The Open Cluster Chemical Abundances and Mapping Survey: VIII. Galactic Chemical Gradient and Azimuthal Analysis from SDSS/MWM DR19 The Milky Way Radial Metallicity Gradient as an Equilibrium Phenomenon: Why Old Stars are Metal-Rich

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-06T18:49:48.436182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 17899aa1-e096-4504-ae96-b03a678f90a3 · inbound

Milky Way Mapper decoded abundances -- II: From patterns to paths cites this paper.

Milky Way Mapper decoded abundances -- II: From patterns to paths The Milky Way Radial Metallicity Gradient as an Equilibrium Phenomenon: Why Old Stars are Metal-Rich

Reference 56

Resolution: verified exact; arxiv_id, observed 2026-05-22T08:34:45.022731Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.