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Paper Citation Record · LEDGER

How Do Galaxies Get Their Gas?

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0209279.

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

pith.paper-citation-record.v1
astro-ph/0209279 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T21:43:51.647682Z

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

80
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 51369803-21a4-4a0a-89f0-0959f67cb462 · inbound

First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback cites this paper.

First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback How Do Galaxies Get Their Gas?

Reference 256

Resolution
verified exact
local_arxiv, observed 2026-05-16T10:57:46.354447Z

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=2026-05-16T10:56:58.457171Z digest=sha256:95c7d4c7b18298eed4b903e72a507334b3a244e0381e9d56b0a6f8ad6f1f1772

Observation b0b64718-d256-4a65-a708-bee3d3ccc256 · inbound

Gas accretion at high redshift: cold flows all the way cites this paper.

Gas accretion at high redshift: cold flows all the way How Do Galaxies Get Their Gas?

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-09T21:43:51.647682Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-09T21:43:51.647682Z digest=sha256:581622670e5fdaa7e8ad5a4dc7ceecacb697e499e829e5bbfa90124d3b896bc4

Observation df5cfc43-2d49-4a3c-92a7-546206510874 · inbound

Cosmic web stripping and starvation of low-mass filament galaxies in TNG50 cites this paper.

Cosmic web stripping and starvation of low-mass filament galaxies in TNG50 How Do Galaxies Get Their Gas?

Reference 267

Resolution
verified exact
local_arxiv, observed 2026-05-25T04:05:19.706678Z

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=sha256:0004f5bb27edc58e26d961a0de2e233db834d221a7d330739600fa6bceac494c

Observation 1091091d-3be4-4944-bcb1-b18464eb7811 · inbound

MIGHTEE-HI: Environmental effects of cosmic filaments on extragalactic HI detections in the COSMOS and XMM-LSS fields cites this paper.

MIGHTEE-HI: Environmental effects of cosmic filaments on extragalactic HI detections in the COSMOS and XMM-LSS fields How Do Galaxies Get Their Gas?

Reference 191

Resolution
unresolved
no resolver link, observed 2026-08-06T19:42:53.601019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T19:42:53.601019Z digest=sha256:53fb9dab7a8d51d1e3b1a0fbcb113f944474644897b1c7c61dcc64f56c711da6