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Paper Citation Record · LEDGER

From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2407.18252.

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

pith.paper-citation-record.v1
2407.18252 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T05:47:34.161307Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T21:37:40.091530Z

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 162d0014-b290-48b1-8abf-1bffe892cb37 · inbound

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data cites this paper.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-12T05:47:34.161307Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation a2076bfc-3715-4eb1-90c9-b474cc186de4 · inbound

Neutrino masses from large-scale structures: future sensitivity and theory dependence cites this paper.

Neutrino masses from large-scale structures: future sensitivity and theory dependence From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-11T21:12:37.246374Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T21:12:37.246374Z digest=sha256:64f920648bd755ee0ac224a8ee027a7e84132553954bb73a4b98846b464265d5

Observation 7530b63f-4ba3-4e0d-a971-d8e35e71ec94 · inbound

Probing Long-Range Forces Between Neutrinos with Cosmic Structures cites this paper.

Probing Long-Range Forces Between Neutrinos with Cosmic Structures From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

Reference 121

Resolution
unresolved
no resolver link, observed 2026-08-10T23:18:06.932101Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:18:06.932101Z digest=sha256:e9d37e8569a01d50e7ecf6fc350efe4e75b324427e2eb0141e3166cb7085dc31

Observation e7fa154a-3c7c-4636-9ece-5931975e6fe7 · inbound

Evolving Dark Sector and the Dark Dimension Scenario cites this paper.

Evolving Dark Sector and the Dark Dimension Scenario From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-06T20:31:41.615255Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T20:31:41.615255Z digest=sha256:7d592c38ab517893523c609b01fbbc4638d0eb46341cf560d6e2c139f018775f

Observation 8bc43f28-f76b-4cd2-bd23-3e81fb838f0d · inbound

Multi-species Dark Matter with Warmth and Randomness cites this paper.

Multi-species Dark Matter with Warmth and Randomness From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

Reference 75

Resolution
verified exact
arxiv_id, observed 2026-05-21T21:04:21.724103Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

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Observation aa0e66eb-3dec-4dc3-9daa-da5227ac3234 · inbound

Constraining interacting dark energy models with black hole superradiance cites this paper.

Constraining interacting dark energy models with black hole superradiance From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

Reference 81

Resolution
verified exact
arxiv_id, observed 2026-05-17T21:10:16.839693Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

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Observation 74c0a758-4946-4e2b-ac8e-35356835db71 · inbound

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses cites this paper.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

Reference 40

Resolution
verified exact
arxiv_id, observed 2026-05-17T04:19:01.084362Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

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Observation fe73514d-ac99-4d8e-9060-536ace12a962 · inbound

Disentangling cosmic distance tensions with early and late dark energy cites this paper.

Disentangling cosmic distance tensions with early and late dark energy From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

Reference 45

Resolution
verified exact
arxiv_id, observed 2026-05-11T08:06:00.307794Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-10T16:49:15.994565Z digest=sha256:24f42f8a60266d0317ab9daea5dbd3ea601ce268c5335413c1d24e0fa7cbd435

Observation 57efcada-2a05-499d-990f-bd63d30febd9 · inbound

Natural Phantom Dark Energy from a $\mathbb{Z}_N$--Axion cites this paper.

Natural Phantom Dark Energy from a $\mathbb{Z}_N$--Axion From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

Reference 43

Resolution
verified exact
local_arxiv, observed 2026-07-10T21:37:40.109261Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

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Observation 0ada0a70-eb35-4918-993b-9c721b7c6129 · inbound

Natural Phantom Crossing from Axion-WIMP Interactions cites this paper.

Natural Phantom Crossing from Axion-WIMP Interactions From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-03T00:46:09.949610Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T00:46:09.949610Z digest=sha256:1c16a5f8f335acd141d0a7f99009af982798e717a2373fd65745ed230c1e103f