Paper Citation Record · LEDGER

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model

As of 4 August 2026, this Paper Citation Record lists 23 of 23 outbound references and 0 inbound Pith citation observations for arXiv:2606.17749.

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

pith.paper-citation-record.v1
2606.17749 v1

Coverage vector

measured 23 of 23 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-06-26T23:59:35.252096Z

measured 23 of 23 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

23 of 23 outbound references displayed

verified exact3
verified fuzzy0
unresolved20
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 01ea4252-9a05-4d4c-9984-d4f20f3f1363 · outbound

This paper cites an unresolved cited work.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Unresolved cited work

Reference 1

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 632df26b-730b-473b-a8ea-a36c39bb7852 · outbound

This paper cites Perlmutter et al.,Measurements ofΩandΛfrom 42 High Redshift Supernovae, Astrophys.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Perlmutter et al.,Measurements ofΩandΛfrom 42 High Redshift Supernovae, Astrophys

Reference 2

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 737d51ee-ed47-4f13-a231-20ebf427bf97 · outbound

This paper cites an unresolved cited work.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Unresolved cited work

Reference 3

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 002866ff-a141-4811-aaf9-20ad1575359e · outbound

This paper cites Aghanim et al.,Planck 2018 results.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Aghanim et al.,Planck 2018 results

Reference 4

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a7c45691-0c0a-48a7-a267-d710a1e1c63f · outbound

This paper cites an unresolved cited work.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Unresolved cited work

Reference 5

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4fede2ef-41bc-4a11-b7e2-49644095d8ea · outbound

This paper cites an unresolved cited work.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Unresolved cited work

Reference 6

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 753b31eb-6b40-4604-8bad-5185d6ecbe3f · outbound

This paper cites Luongo, and M.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Luongo, and M

Reference 7

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 233cf8f8-f8c4-4263-b799-30909c2d5cd8 · outbound

This paper cites an unresolved cited work.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Unresolved cited work

Reference 8

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85fc4936-b712-40cd-9f3c-a10a0851d03f · outbound

This paper cites Carloni, O.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Carloni, O

Reference 9

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 68490d51-b97a-48af-abb1-011e4871fe5a · outbound

This paper cites an unresolved cited work.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Unresolved cited work

Reference 10

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 43ccd95f-72fe-47be-b98a-c591a57a44d7 · outbound

This paper cites an unresolved cited work.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Unresolved cited work

Reference 11

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 235fd815-ec45-46a5-8dce-c44263846da3 · outbound

This paper cites Carloni, O.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Carloni, O

Reference 12

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7de08435-3775-4b94-a9c6-411fe601611f · outbound

This paper cites Heymans et al.,KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints, Astron.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Heymans et al.,KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints, Astron

Reference 13

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6550c177-11dd-4fa4-9ac4-c633057d5be7 · outbound

This paper cites Di Valentino et al.,Snowmass2021 - Letter of interest cosmology intertwined II: The hubble constant tension, Astropart.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Di Valentino et al.,Snowmass2021 - Letter of interest cosmology intertwined II: The hubble constant tension, Astropart

Reference 14

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ae6ac7cf-a9e4-4c57-80fd-fc8a6453ce6e · outbound

This paper cites an unresolved cited work.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Unresolved cited work

Reference 15

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 196d057d-916f-4464-a014-2cf927dd0e0e · outbound

This paper cites Di Valentino,Can interacting dark energy solve theH 0 tension?, Phys.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Di Valentino,Can interacting dark energy solve theH 0 tension?, Phys

Reference 16

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f4bf178-9b97-4dbb-a3bd-9c8805f91602 · outbound

This paper cites Di Valentino, A.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Di Valentino, A

Reference 17

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 79296cd5-31c7-4b05-be15-b1ca3134218f · outbound

This paper cites Poulin, T.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Poulin, T

Reference 18

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3aba2e48-6d62-4724-a2c2-8cad4eb1b896 · outbound

This paper cites de la Macorra, E.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model de la Macorra, E

Reference 19

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 06456666-6404-466c-80b6-1aef9f7ae1e3 · outbound

This paper cites Resolving the Hubble tension at late times with Dark Energy.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Resolving the Hubble tension at late times with Dark Energy

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-07-03T21:58:58.804738Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation f3862169-179c-4e27-8322-88c2c8d41188 · outbound

This paper cites Solving the Hubble tension at intermediate redshifts with dynamical dark energy.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Solving the Hubble tension at intermediate redshifts with dynamical dark energy

Reference 21

Resolution: verified exact; arxiv_id, observed 2026-07-03T21:58:58.801691Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 47e85219-10b2-4e3f-aaab-06a4cf74c7f9 · outbound

This paper cites Carloni, O.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Carloni, O

Reference 22

Resolution: unresolved; no resolver link, observed 2026-06-26T23:59:35.252096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0e39b4c1-a6e5-4c9b-96cf-3fcc5e51c555 · outbound

This paper cites A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension.

Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension

Reference 23

Resolution: verified exact; local_arxiv, observed 2026-07-03T21:58:58.800009Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Pith citing papers

No inbound Pith citation observations are available.