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Paper Citation Record · LEDGER

HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules. III. The absorption lines of [O I], CH, and OH

As of 6 August 2026, this Paper Citation Record lists 5 of 5 outbound references and 0 inbound Pith citation observations for arXiv:2604.25590.

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

pith.paper-citation-record.v1
2604.25590 v1

Coverage vector

measured 5 of 5 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-07T15:48:40.462414Z

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+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

5 of 5 outbound references displayed

  • verified exact0
  • verified fuzzy2
  • unresolved1
  • parse uncertain0
  • malformed identifier2
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation a6d911ff-be54-4ed8-93a0-5844dc8681fc · outbound

This paper cites an unresolved cited work.

HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules. III. The absorption lines of [O I], CH, and OH Unresolved cited work

Reference 1

Resolution
malformed identifier
raw_fallback, observed 2026-05-27T02:58:26.549482Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

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Observation a7d95178-533e-46e2-8099-02906bb9facc · outbound

This paper cites Another column density table for the velocity interval for VI(M) is available at the CDS via anonymous ftp to cdsarc.cds.unistra.fr (130.79.128.5).

HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules. III. The absorption lines of [O I], CH, and OH Another column density table for the velocity interval for VI(M) is available at the CDS via anonymous ftp to cdsarc.cds.unistra.fr (130.79.128.5)

Reference 2

Resolution
verified fuzzy
raw_fallback, observed 2026-05-27T02:58:26.559653Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-07T15:48:40.462414Z digest=sha256:a8449a773c048a90be2251027e7cf0456f26628fc6745ccf3d78cbfb4ce02844

Observation ee258516-d542-459c-85c1-a73fc11ef6dd · outbound

This paper cites an unresolved cited work.

HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules. III. The absorption lines of [O I], CH, and OH Unresolved cited work

Reference 3

Resolution
unresolved
raw_fallback, observed 2026-05-27T02:58:26.556979Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-07T15:48:40.462414Z digest=sha256:530ba6ec7142864ece7ecbe782d8b6132e263813d740ad25b82a8be092b162c9

Observation e4a7ae63-0cea-4ebf-bdf3-183cd0db14ae · outbound

This paper cites C.1: Channel-wise column density spectra (Nd/d3) as a function of velocity.

HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules. III. The absorption lines of [O I], CH, and OH C.1: Channel-wise column density spectra (Nd/d3) as a function of velocity

Reference 4

Resolution
malformed identifier
raw_fallback, observed 2026-05-27T02:58:26.562298Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-07T15:48:40.462414Z digest=sha256:68b88f33271f8a1e865555309f7ec6bdbcf517b0f321dbc8cbb4d2343337ac16

Observation 4baf8e77-6380-4944-aa8f-9895df826190 · outbound

This paper cites The large dispersions in our data points may result from line-of-sight integration through multiple ISM phases with distinct metallicities, particularly between 4 and 8 kpc.

HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules. III. The absorption lines of [O I], CH, and OH The large dispersions in our data points may result from line-of-sight integration through multiple ISM phases with distinct metallicities, particularly between 4 and 8 kpc

Reference 5

Resolution
verified fuzzy
raw_fallback, observed 2026-05-27T02:58:26.554517Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-07T15:48:40.462414Z digest=sha256:58f437d79ab265a159fd5ba985a7ca78c6f022d1c05655734c58efbca4e304d8

Pith citing papers

No inbound Pith citation observations are available.