Paper Citation Record · LEDGER

First Constraints on a Pixelated Universe in Light of DESI

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2406.04408.

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

pith.paper-citation-record.v1
2406.04408 v2

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 2026-08-19T06:32:44.657259+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T13:41:23.839657Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T15:55:04.897181Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

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 43bf9113-af94-4d88-8bd1-cc747652fc31 · inbound

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? First Constraints on a Pixelated Universe in Light of DESI

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.839657Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4d7a9478-54de-4a9a-a8e8-763822843684 · inbound

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? cites this paper.

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? First Constraints on a Pixelated Universe in Light of DESI

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-10T22:00:59.801338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bd3b7e8e-9d19-4032-a23b-0f3b7487def3 · inbound

Dark energy and lensing anomaly in Planck CMB data cites this paper.

Dark energy and lensing anomaly in Planck CMB data First Constraints on a Pixelated Universe in Light of DESI

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-08T22:04:59.474616Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 615bbf73-17bd-4abb-8c67-d8e9d4768851 · inbound

Can the universe experience an AdS landscape since matter-radiation equality? cites this paper.

Can the universe experience an AdS landscape since matter-radiation equality? First Constraints on a Pixelated Universe in Light of DESI

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:56.220816Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation be538fd5-ea24-4367-92d9-8a0145082f9a · inbound

Imprint of swampland-inspired coupled early dark energy cites this paper.

Imprint of swampland-inspired coupled early dark energy First Constraints on a Pixelated Universe in Light of DESI

Reference 23

Resolution: verified exact; local_arxiv, observed 2026-07-08T15:55:04.898490Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.