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Paper Citation Record · LEDGER

On the environmental dependence of halo formation

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0402237.

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

pith.paper-citation-record.v1
astro-ph/0402237 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T07:53:18.912461Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T15:14:47.236956Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • parse uncertain0
  • malformed identifier0
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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 ec0234e4-1166-4a17-a0cb-15a0fab9849f · inbound

Tomographic Alcock-Paczynski Test with Marked Correlation Functions cites this paper.

Tomographic Alcock-Paczynski Test with Marked Correlation Functions On the environmental dependence of halo formation

Reference 33

Resolution
verified exact
local_arxiv, observed 2026-05-22T18:56:57.834842Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-05-22T18:56:46.117021Z digest=sha256:0d44cc4ca6fbbd2e6838efa9c43096b657f53bab083b4b7a8e13977b47938c3d

Observation b3b1da0f-8cb9-470c-b8d1-a76463508d08 · inbound

Cosmological constraints from neighbor-density-weighted marked correlation functions cites this paper.

Cosmological constraints from neighbor-density-weighted marked correlation functions On the environmental dependence of halo formation

Reference 53

Resolution
verified exact
local_arxiv, observed 2026-05-25T03:30:17.397013Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-05-25T03:27:13.896349Z digest=sha256:20018c1e4b629ab26be98960613b5fa111ac8d9cd91ea523afb7f9aadc34fb83

Observation b43f010b-0eba-4c54-8ddc-420141e2a12e · inbound

Cosmological constraints from neighbor-density-weighted marked correlation functions cites this paper.

Cosmological constraints from neighbor-density-weighted marked correlation functions On the environmental dependence of halo formation

Reference 53

Resolution
verified exact
local_arxiv, observed 2026-06-30T15:14:47.238177Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-06-30T15:08:32.960489Z digest=sha256:7845a69a1aa3f9590f05b12db79da004fbb83530dab70a55401857c24ebdb283

Observation 68ee2ecb-66ae-4310-aaae-32d526c3cab5 · inbound

The Environmental Dependence of Halo Intrinsic Alignments: Stronger Signals in Underdense Regions cites this paper.

The Environmental Dependence of Halo Intrinsic Alignments: Stronger Signals in Underdense Regions On the environmental dependence of halo formation

Reference 45

Resolution
unresolved
no resolver link, observed 2026-07-14T06:58:47.359702Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:58:47.359702Z digest=sha256:a1178695288101b67c84b1b24a16a201056edf587a4dde1d808f244b10e8a33a

Observation f4ca4794-8942-48df-8734-992b8bfda37a · inbound

Web-Halo Model Peak-Background Split (WHM-PBS): halo bias as a distribution, not a number cites this paper.

Web-Halo Model Peak-Background Split (WHM-PBS): halo bias as a distribution, not a number On the environmental dependence of halo formation

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-01T07:53:18.912461Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T07:53:18.912461Z digest=sha256:f0c17f91839d443ed2808a7d9df3ed11be481e464d96d1543fd553a3f96bd62f