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Paper Citation Record · LEDGER

The Aemulus Project III: Emulation of the Galaxy Correlation Function

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1804.05867.

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

pith.paper-citation-record.v1
1804.05867 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T04:48:07.696829Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T04:53:06.731030Z

Reference resolution

0 of 0 outbound references displayed

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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 3fa19058-5e4b-42c9-88d3-232b836365da · inbound

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation cites this paper.

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation The Aemulus Project III: Emulation of the Galaxy Correlation Function

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-07T04:48:07.696829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T04:48:07.696829Z digest=sha256:2ff6afa6336143a7847896596ef8ea8cd686544ad12dc38d5c62cb9e49ca2535

Observation 9a328b01-5abc-4554-8df6-4244062298cc · inbound

Modeling nonlinear scales for dynamical dark energy cosmologies with COLA cites this paper.

Modeling nonlinear scales for dynamical dark energy cosmologies with COLA The Aemulus Project III: Emulation of the Galaxy Correlation Function

Reference 95

Resolution
verified exact
local_arxiv, observed 2026-05-18T06:15:58.735362Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-18T06:13:13.345307Z digest=sha256:107f370489b1bc416d6aba73d88136ca14065a17a0d99dfbcae4fc873f2a51a8

Observation eaf8d7f0-e7a8-4130-8606-630bff555b17 · inbound

Analytical and fitting formulae for solutions to Lyman-alpha radiative transfer equations: the effects of geometry, recoil, and velocity gradients cites this paper.

Analytical and fitting formulae for solutions to Lyman-alpha radiative transfer equations: the effects of geometry, recoil, and velocity gradients The Aemulus Project III: Emulation of the Galaxy Correlation Function

Reference 164

Resolution
verified exact
local_arxiv, observed 2026-06-29T04:53:06.732538Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:55a679bc2a6a728b5a9bd92e11b0d01c7df8d776f6bb11107067811fb5ddea3e