Pith. sign in

Paper Citation Record · LEDGER

The Chemical Evolution of the Draco Dwarf Spheroidal Galaxy

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0906.1006.

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

pith.paper-citation-record.v1
0906.1006 v1

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 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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

measured 1 of 1 external citation measurements

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

Source: pith, 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

212
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 18a94cff-49e3-43c4-90bc-85e0b6125e37 · inbound

The Pristine Dwarf Galaxy Survey -- VII. The metallicity distributions of 12 Milky Way faint satellites cites this paper.

The Pristine Dwarf Galaxy Survey -- VII. The metallicity distributions of 12 Milky Way faint satellites The Chemical Evolution of the Draco Dwarf Spheroidal Galaxy

Reference 86

Resolution
verified exact
local_arxiv, observed 2026-06-28T00:11:25.436132Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d9417d86f75974c752427e253d76c0ea8c13b8d42ab648bd23eb0411b0489a0e

Observation a5f5d798-b733-4a5d-97cf-132411a349e1 · inbound

The Sc, Ti, and V Abundance Discrepancy: Testing High-Mass IMF Variation and Massive-Star Rotation cites this paper.

The Sc, Ti, and V Abundance Discrepancy: Testing High-Mass IMF Variation and Massive-Star Rotation The Chemical Evolution of the Draco Dwarf Spheroidal Galaxy

Reference 20

Resolution
verified exact
local_arxiv, observed 2026-07-01T05:15:24.872029Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:fadde3f870a32e419869bd780e2d34eaeb7df2a8f69d26efb31cdde152119a4f