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Paper Citation Record · LEDGER

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk

As of 12 August 2026, this Paper Citation Record lists 13 of 13 outbound references and 0 inbound Pith citation observations for arXiv:2604.23686.

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

pith.paper-citation-record.v1
2604.23686 v2

Coverage vector

measured 13 of 13 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-07-01T09:46:04.510059Z

measured 13 of 13 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

13 of 13 outbound references displayed

  • verified exact1
  • verified fuzzy3
  • unresolved7
  • parse uncertain0
  • malformed identifier2
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation a94afd5e-3c92-4862-b8b5-df17ac538ecb · outbound

This paper cites an unresolved cited work.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk Unresolved cited work

Reference 1

Resolution
unresolved
raw_fallback, observed 2026-07-06T11:32:22.190344Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 2ea235d2-04f3-4e5c-ac56-1b2de6ffbe7a · outbound

This paper cites an unresolved cited work.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk Unresolved cited work

Reference 2

Resolution
unresolved
raw_fallback, observed 2026-07-06T11:32:22.186639Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 9a3841ef-04fa-4907-91f7-79d4fbab1bc4 · outbound

This paper cites Notably, the detection rate as a function of the equivalent width threshold (Wth) is best characterized by an exponential decay model.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk Notably, the detection rate as a function of the equivalent width threshold (Wth) is best characterized by an exponential decay model

Reference 3

Resolution
verified fuzzy
raw_fallback, observed 2026-07-06T11:32:22.181063Z

Source-reported events for the cited work

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Observation b9f5006b-450f-48e4-a682-661d5fd3072c · outbound

This paper cites an unresolved cited work.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk Unresolved cited work

Reference 4

Resolution
unresolved
raw_fallback, observed 2026-07-06T11:32:22.182829Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-07-01T09:46:04.510059Z digest=sha256:aad4f2f25f3bd47c748d6f29c2e287c82b3200d6967cba36b5110233fd6bbbfb

Observation df384ee0-b3e8-4f71-ad92-b2376074485a · outbound

This paper cites While the south- ern hemisphere has a higher covering fraction (Cf ≈0.90 vs.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk While the south- ern hemisphere has a higher covering fraction (Cf ≈0.90 vs

Reference 5

Resolution
verified fuzzy
raw_fallback, observed 2026-07-06T11:32:22.188486Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 8c525511-2532-4b38-9720-45ce3da22e73 · outbound

This paper cites Rather than a simple uniform depletion law, our results reveal a multi-phase physical picture driven by lo- cal volume density and geometric integration.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk Rather than a simple uniform depletion law, our results reveal a multi-phase physical picture driven by lo- cal volume density and geometric integration

Reference 6

Resolution
verified fuzzy
raw_fallback, observed 2026-07-06T11:32:22.195823Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation c1e0dd28-79e1-48be-997b-1b8dc65d00af · outbound

This paper cites an unresolved cited work.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk Unresolved cited work

Reference 7

Resolution
unresolved
raw_fallback, observed 2026-07-06T11:32:22.197695Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 0f2f0cb8-3a95-4c2a-9065-a03820124bd2 · outbound

This paper cites The chemical composition of the Sun.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk The chemical composition of the Sun

Reference 8

Resolution
malformed identifier
local_arxiv, observed 2026-07-01T09:55:40.090048Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation f9e132eb-b39e-4048-a969-29273ec4a6a7 · outbound

This paper cites an unresolved cited work.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk Unresolved cited work

Reference 9

Resolution
unresolved
raw_fallback, observed 2026-07-06T11:32:22.193850Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-07-01T09:46:04.510059Z digest=sha256:2177e09dc3125598869d31274473ca5544f249fb295977c8aa903db85450399d

Observation e54c5848-7a72-49ce-85c3-3baa46204e82 · outbound

This paper cites an unresolved cited work.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk Unresolved cited work

Reference 10

Resolution
unresolved
raw_fallback, observed 2026-07-06T11:32:22.192132Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation d170cc99-8bd5-44bb-9b4a-4fb986cf75e1 · outbound

This paper cites MAGIICAT I. The MgII Absorber-Galaxy Catalog.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk MAGIICAT I. The MgII Absorber-Galaxy Catalog

Reference 11

Resolution
malformed identifier
local_arxiv, observed 2026-07-01T09:55:40.097022Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 16bd2131-b0a5-4964-a1a6-5223c6ed5767 · outbound

This paper cites an unresolved cited work.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk Unresolved cited work

Reference 12

Resolution
unresolved
raw_fallback, observed 2026-07-06T11:32:22.184551Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-07-01T09:46:04.510059Z digest=sha256:1d7ed047597b5ac57be5957cf63014b3331b1a9443e5be9ea8f4b4a43e8d3412

Observation 0905e9d7-3f9e-4dfd-95e1-cd559e355fa7 · outbound

This paper cites METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. II. Variations of interstellar depletions and dust-to-gas ratio within the LMC.

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. II. Variations of interstellar depletions and dust-to-gas ratio within the LMC

Reference 13

Resolution
verified exact
arxiv_id, observed 2026-07-01T09:55:40.093536Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Pith citing papers

No inbound Pith citation observations are available.