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Paper Citation Record · LEDGER

Gas accretion as the origin of chemical abundance gradients in distant galaxies

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1010.2534.

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

pith.paper-citation-record.v1
1010.2534 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

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

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T01:14:15.558094Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T14:39:32.421851Z

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 aaaed9a3-80f0-4cc3-9492-cf9f3b34df06 · inbound

Resolved Ages and Stellar Metallicities in Progenitors of Milky Way Analogs: A Closer Look at their Star Formation Histories since $z=5$ cites this paper.

Resolved Ages and Stellar Metallicities in Progenitors of Milky Way Analogs: A Closer Look at their Star Formation Histories since $z=5$ Gas accretion as the origin of chemical abundance gradients in distant galaxies

Reference 227

Resolution
verified exact
local_arxiv, observed 2026-06-26T14:39:32.423251Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:472655810ff3847aa0543f41588c2ea7176708eb853d28da325b41ec1a4e986a

Observation 0e807f8e-2a1c-49c2-a5a9-f8891e5c8094 · inbound

The Mysterious Case of Iron in XMPs: Anomalous High log(Fe/O) Observed in Extremely Metal-Poor Galaxies HSCJ1631+4426 and SDSSJ0811+4730 cites this paper.

The Mysterious Case of Iron in XMPs: Anomalous High log(Fe/O) Observed in Extremely Metal-Poor Galaxies HSCJ1631+4426 and SDSSJ0811+4730 Gas accretion as the origin of chemical abundance gradients in distant galaxies

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-02T01:14:15.558094Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T01:14:15.558094Z digest=sha256:dd45102b458fc5efdeaaa672dd58301b680dbf3ab43625547ff7d5a23d74435f