Pith. sign in

Paper Citation Record · LEDGER

Unveiling the time evolution of chemical abundances across the Milky Way disk with APOGEE

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2305.13378.

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

pith.paper-citation-record.v1
2305.13378 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T19:34:24.262056Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-09T11:39:18.087618Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 30050273-b4dc-4973-af2e-eb10ed4dffc2 · inbound

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? cites this paper.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Unveiling the time evolution of chemical abundances across the Milky Way disk with APOGEE

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-11T19:34:24.262056Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T19:34:24.262056Z digest=sha256:5cdd17761ca2c10c12fbbd09dfc138b9cbdbeed4179d4d65e51f35802444e900

Observation 5d8fa51d-7f52-49cf-8627-56b31b56d444 · inbound

Bar-spiral interaction produces radial migration and star formation bursts cites this paper.

Bar-spiral interaction produces radial migration and star formation bursts Unveiling the time evolution of chemical abundances across the Milky Way disk with APOGEE

Reference 126

Resolution
metadata mismatch
local_arxiv, observed 2026-08-09T11:39:18.092597Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-09T11:39:17.814936Z digest=sha256:82b653314a1b531acf602894cc6676ac0ea06bef6eb5c772b497e8b459d01c92

Observation b1e2215e-27bd-4dd5-b881-0e788b6632fc · 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 Unveiling the time evolution of chemical abundances across the Milky Way disk with APOGEE

Reference 146

Resolution
unresolved
no resolver link, observed 2026-08-01T04:28:46.811462Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T04:28:46.811462Z digest=sha256:311e0cd9805eca90f7056d4f4b60f257ec12f50abaad63d56a0cf81b31ff85ee