Paper Citation Record · LEDGER

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter

As of 9 August 2026, this Paper Citation Record lists 100 of 120 outbound references and 5 inbound Pith citation observations for arXiv:2506.23029.

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pith.paper-citation-record.v1
2506.23029 v1

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Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

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Outbound references

Observation c2ae387a-4e21-4418-a617-34b76c133a85 · outbound

This paper cites an unresolved cited work.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

Reference 1

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Observation 7b571711-8636-4347-ae62-9cb5e4effd80 · outbound

This paper cites Cosmic Black-Body Radiation,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Cosmic Black-Body Radiation,

Reference 2

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Observation 3f7ae64d-6c51-4c6e-9930-4f834a76f6d6 · outbound

This paper cites A Measurement of excess antenna temperature at 4080-Mc/s,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter A Measurement of excess antenna temperature at 4080-Mc/s,

Reference 3

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Observation 8fd5b667-2ffa-48ca-8157-50c2057ea465 · outbound

This paper cites Observa- tional evidence from supernovae for an accelerating uni- verse and a cosmological constant,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Observa- tional evidence from supernovae for an accelerating uni- verse and a cosmological constant,

Reference 4

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Observation 55aa7919-abe2-4574-9520-29a83bff6e07 · outbound

This paper cites Structure in the COBE differential microwave radiometer first year maps,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Structure in the COBE differential microwave radiometer first year maps,

Reference 5

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Observation 91619bd9-8147-4f0a-b33c-e3a7bfdd66ed · outbound

This paper cites Cosmic Microwave Background Anisotropies,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Cosmic Microwave Background Anisotropies,

Reference 6

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Observation 8e130446-35dc-4078-ad26-5f0b93ab2cd0 · outbound

This paper cites Measurements of Ω and Λ from 42 high redshift super- novae,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Measurements of Ω and Λ from 42 high redshift super- novae,

Reference 7

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This paper cites an unresolved cited work.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

Reference 8

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Observation e9351b56-11f3-433a-897c-255bcc39d588 · outbound

This paper cites Observational Probes of Cosmic Acceleration,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Observational Probes of Cosmic Acceleration,

Reference 9

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Observation 32a6b5d9-59cb-4649-9b80-342aa08d8293 · outbound

This paper cites an unresolved cited work.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

Reference 10

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Observation 1f5e6be5-3788-4c38-a7da-d5811c7c148f · outbound

This paper cites Nine-Year Wilkinson Mi- crowave Anisotropy Probe (WMAP) Observations: Final Maps and Results,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Nine-Year Wilkinson Mi- crowave Anisotropy Probe (WMAP) Observations: Final Maps and Results,

Reference 11

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Observation 9af785e7-e67c-45ed-bd41-94e35f150141 · outbound

This paper cites ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter

Reference 12

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Observation 00393b40-f758-4638-af7a-bcbec4cb66e1 · outbound

This paper cites Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies,

Reference 14

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Observation 577b6b60-f561-4185-9eb2-aa540715d5b8 · outbound

This paper cites The 2dF Galaxy Redshift Sur- vey: Power-spectrum analysis of the final dataset and cosmological implications,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The 2dF Galaxy Redshift Sur- vey: Power-spectrum analysis of the final dataset and cosmological implications,

Reference 15

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Observation 6e8d7ddc-e7ef-4d35-a08d-17cdd35fe6e0 · outbound

This paper cites The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant,

Reference 16

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Observation d62860e2-7a4d-4d48-baee-8189982e4da4 · outbound

This paper cites Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory,

Reference 17

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Observation a8c87035-852d-4f76-ab3e-8237f09df91d · outbound

This paper cites Angular Baryon Acoustic Oscillation measure at z = 2 .225 from the SDSS quasar survey,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Angular Baryon Acoustic Oscillation measure at z = 2 .225 from the SDSS quasar survey,

Reference 18

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Observation 971ba3a0-c930-442b-9a40-f025913597da · outbound

This paper cites The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: first measurement of baryon acoustic os- cillations between redshift 0.8 and 2.2,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: first measurement of baryon acoustic os- cillations between redshift 0.8 and 2.2,

Reference 19

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Observation d979f5f6-25a9-4701-be19-bc1ae2918ee7 · outbound

This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 20

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Observation 08fa1d2e-1d4c-4fb0-bc12-d9feef3e6a90 · outbound

This paper cites DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars

Reference 21

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This paper cites DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest

Reference 22

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Observation f1e45aae-f61d-4eba-b295-b120f6e9bcfb · outbound

This paper cites The Cosmological Constant Problem,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The Cosmological Constant Problem,

Reference 23

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This paper cites The Cosmological constant,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The Cosmological constant,

Reference 24

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Observation f971de96-1409-4e88-937a-e39df495ab88 · outbound

This paper cites The Cosmological Con- stant and Dark Energy,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The Cosmological Con- stant and Dark Energy,

Reference 25

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This paper cites Cosmological constant: The Weight of the vacuum,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Cosmological constant: The Weight of the vacuum,

Reference 26

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

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Observation 6fa9308a-8df5-4377-acbd-41dc97ebbfd7 · outbound

This paper cites Quintessence, cosmic coincidence, and the cosmological constant,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Quintessence, cosmic coincidence, and the cosmological constant,

Reference 28

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This paper cites Snowmass2021 - Letter of in- terest cosmology intertwined I: Perspectives for the next decade,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Snowmass2021 - Letter of in- terest cosmology intertwined I: Perspectives for the next decade,

Reference 29

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This paper cites Snowmass2021 - Letter of interest cosmology intertwined II: The hubble constant tension,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Snowmass2021 - Letter of interest cosmology intertwined II: The hubble constant tension,

Reference 30

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Cosmology Intertwined III: f σ8 and S8,

Reference 31

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This paper cites Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology asso- ciated with the cosmological tensions and anomalies,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology asso- ciated with the cosmological tensions and anomalies,

Reference 32

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This paper cites The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Reference 33

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This paper cites Observational and the- oretical constraints on singular dark matter halos,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Observational and the- oretical constraints on singular dark matter halos,

Reference 34

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This paper cites Evidence against dissipationless dark matter from observations of galaxy haloes,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Evidence against dissipationless dark matter from observations of galaxy haloes,

Reference 35

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This paper cites The unexpected diversity of dwarf galaxy rotation curves,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The unexpected diversity of dwarf galaxy rotation curves,

Reference 36

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This paper cites Too big to fail? The puzzling darkness of massive Milky Way subhaloes,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Too big to fail? The puzzling darkness of massive Milky Way subhaloes,

Reference 37

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The Great disk of Milky Way satellites and cosmological sub-structures,

Reference 38

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Die Rotverschiebung von extragalaktischen Nebeln,

Reference 39

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Rotation of the An- dromeda Nebula from a Spectroscopic Survey of Emission Regions,

Reference 40

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Formation of Galaxies and Large Scale Structure with Cold Dark Matter,

Reference 41

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Sterile-neutrinos as dark matter,

Reference 42

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This paper cites CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey,

Reference 43

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This paper cites KiDS-450: Cosmological parameter constraints from tomographic weak gravita- tional lensing,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter KiDS-450: Cosmological parameter constraints from tomographic weak gravita- tional lensing,

Reference 44

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Planck 2018 results. VIII. Gravitational lensing,

Reference 45

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This paper cites Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear,

Reference 46

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Dark Energy Survey year 1 results: Cosmological constraints from galaxy cluster- ing and weak lensing,

Reference 47

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This paper cites Dark Energy Survey Year 3 results: Cosmological constraints from galaxy cluster- ing and weak lensing,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Dark Energy Survey Year 3 results: Cosmological constraints from galaxy cluster- ing and weak lensing,

Reference 48

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This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Clustering.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Dark Energy Survey Year 3 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Clustering

Reference 49

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

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Observation 9295ddab-8f92-4dd3-a4df-dace3aae34e2 · outbound

This paper cites Dark Matter Results from 225 Live Days of XENON100 Data,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Dark Matter Results from 225 Live Days of XENON100 Data,

Reference 51

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

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This paper cites Results from a search for dark matter in the complete LUX exposure,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Results from a search for dark matter in the complete LUX exposure,

Reference 53

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ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

Reference 54

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This paper cites PandaX: A Liquid Xenon Dark Matter Experiment at CJPL,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter PandaX: A Liquid Xenon Dark Matter Experiment at CJPL,

Reference 55

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Observation 9ed902c0-a245-4a67-85ba-a0f4ea5b1c39 · outbound

This paper cites Dark Matter Search Results from a One Ton-Year Exposure of XENON1T,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Dark Matter Search Results from a One Ton-Year Exposure of XENON1T,

Reference 56

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.834834Z

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.

Observation 23205e17-8062-440b-a1f9-70d264a4c572 · outbound

This paper cites an unresolved cited work.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

Reference 57

Resolution: unresolved; raw_fallback, observed 2026-08-06T22:01:25.819851Z

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.

Observation 8fcc379c-db53-4b30-9d7d-e6a4d043e1c5 · outbound

This paper cites an unresolved cited work.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

Reference 58

Resolution: unresolved; raw_fallback, observed 2026-08-06T22:01:25.801042Z

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.

Observation 6dbb641c-d4e8-421f-a6ee-f689369f8ede · outbound

This paper cites an unresolved cited work.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

Reference 59

Resolution: parse uncertain; raw_fallback, observed 2026-08-06T22:01:25.784313Z

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.

Observation 86c0e06d-4387-462e-83c5-30c0b8156251 · outbound

This paper cites Limits to Dark Matter Annihilation Cross-Section from a Com- bined Analysis of MAGIC and Fermi-LAT Observations of Dwarf Satellite Galaxies,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Limits to Dark Matter Annihilation Cross-Section from a Com- bined Analysis of MAGIC and Fermi-LAT Observations of Dwarf Satellite Galaxies,

Reference 60

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.767367Z

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.

Observation 5f29e5c4-255a-40fc-b6c9-f424a48b9245 · outbound

This paper cites Searching for Secluded Dark Matter with H.E.S.S., Fermi-LAT, and Planck,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Searching for Secluded Dark Matter with H.E.S.S., Fermi-LAT, and Planck,

Reference 61

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.746311Z

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.

Observation e48a0906-6256-4382-b5d7-91868838a327 · outbound

This paper cites Indirect and direct search for dark matter,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Indirect and direct search for dark matter,

Reference 62

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.721501Z

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.

Observation 5396fd07-73fe-4062-9060-915b4ff8df08 · outbound

This paper cites A review of indirect searches for particle dark matter,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter A review of indirect searches for particle dark matter,

Reference 63

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.698766Z

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.

Observation 78d85893-8523-425a-9428-b7e37790e4ba · outbound

This paper cites an unresolved cited work.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

Reference 64

Resolution: unresolved; raw_fallback, observed 2026-08-06T22:01:25.679979Z

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.

Observation dd8cab86-cb3d-426a-9eaa-6c0b55427c97 · outbound

This paper cites Extended Dark Energy analysis using DESI DR2 BAO measurements.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:22.804530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9bb0cbf8-094e-4c1c-99f1-946a70432ed5 · outbound

This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:22.907980Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 98e9e63d-c9d2-4421-9553-949a20dc7442 · outbound

This paper cites DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:23.018866Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0ad45d1e-2c64-4860-996b-675acc0509e6 · outbound

This paper cites Structure formation with generalized dark mat- ter,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Structure formation with generalized dark mat- ter,

Reference 68

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.664838Z

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.

Observation 91ec362a-7b17-430e-95d2-b577c70925ee · outbound

This paper cites Observational constraints on vari- able equation of state parameters of dark matter and dark energy after Planck,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Observational constraints on vari- able equation of state parameters of dark matter and dark energy after Planck,

Reference 69

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.649251Z

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.

Observation efbeb68f-9fab-467d-a8e1-ddbc17cc2c1e · outbound

This paper cites Testing the warmness of dark matter,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Testing the warmness of dark matter,

Reference 70

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.632174Z

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.

Observation 1dfc6fa1-0450-41c1-b45b-2017c8e4e9b2 · outbound

This paper cites The foundation of the general theory of relativity,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The foundation of the general theory of relativity,

Reference 72

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.613643Z

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.

Observation 8b604c2e-f7e7-46db-a101-2f77e258e686 · outbound

This paper cites On the Curvature of space,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter On the Curvature of space,

Reference 73

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.595360Z

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.

Observation 16113059-2d52-4370-8f19-914785e553ce · outbound

This paper cites Accelerating universes with scaling dark matter,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Accelerating universes with scaling dark matter,

Reference 74

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.577180Z

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.

Observation 9aa7385f-dadc-4a81-a6e2-a77d25b2d26a · outbound

This paper cites Exploring the expansion history of the universe,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Exploring the expansion history of the universe,

Reference 75

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.560089Z

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.

Observation b2bd2657-a29a-4ddd-a6ab-4237aa33c56c · outbound

This paper cites The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:23.448726Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5481c6a2-d4d6-4a7c-b514-1654c26adb6f · outbound

This paper cites Planck 2018 results. V. CMB power spectra and likelihoods,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Planck 2018 results. V. CMB power spectra and likelihoods,

Reference 77

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.543398Z

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.

Observation c04ecb16-8649-410c-b5c6-7bbb13bb4944 · outbound

This paper cites The Atacama Cosmology Tele- scope: A Measurement of the DR6 CMB Lensing Power Spectrum and Its Implications for Structure Growth,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The Atacama Cosmology Tele- scope: A Measurement of the DR6 CMB Lensing Power Spectrum and Its Implications for Structure Growth,

Reference 78

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.523558Z

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.

Observation a8e4a63b-2172-4cb2-b0e3-71de5ed10206 · outbound

This paper cites The Dark Energy Survey: Cosmology Results with ∼1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The Dark Energy Survey: Cosmology Results with ∼1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set,

Reference 79

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.503700Z

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.

Observation cb6d0d25-9a1e-467a-8601-6e4bdf180b18 · outbound

This paper cites The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:23.472647Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 32b8b8b0-ddbd-41d4-a05c-ef259f329d57 · outbound

This paper cites Reionization optical depth determination from Planck HFI data with ten percent accuracy,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Reionization optical depth determination from Planck HFI data with ten percent accuracy,

Reference 81

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.479498Z

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.

Observation 6ee28b08-5264-4258-b5eb-d3069a23a88b · outbound

This paper cites Efficient com- putation of CMB anisotropies in closed FR W models,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Efficient com- putation of CMB anisotropies in closed FR W models,

Reference 82

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.457714Z

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.

Observation 9f0766e5-d2e9-431b-abc1-ed68acd5c049 · outbound

This paper cites Cobaya: Code for Bayesian Analysis of hierarchical physical models,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Cobaya: Code for Bayesian Analysis of hierarchical physical models,

Reference 83

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.437207Z

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.

Observation 0fad7f16-e05e-4523-ae27-532368782e61 · outbound

This paper cites Inference from Iterative Simulation Using Multiple Sequences,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Inference from Iterative Simulation Using Multiple Sequences,

Reference 84

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.416433Z

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.

Observation 29e15b60-18ad-4851-9e0e-13a162ea61a5 · outbound

This paper cites GetDist: a Python package for analysing Monte Carlo samples.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter GetDist: a Python package for analysing Monte Carlo samples

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:23.502705Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 65c97260-eca5-4aee-8344-0706b3669d7d · outbound

This paper cites Quintessence Dark Matter.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Quintessence Dark Matter

Reference 86

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:24.023216Z

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.

Observation fc21414b-5b27-4a84-ab1c-012e1a73ca8e · outbound

This paper cites Evolving Dark Energy or Evolving Dark Matter?.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Evolving Dark Energy or Evolving Dark Matter?

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:23.513743Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e9b5e9b-e591-48eb-9953-a9bf38053d4b · outbound

This paper cites Cosmological bounds on the equation of state of dark matter,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Cosmological bounds on the equation of state of dark matter,

Reference 88

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.397547Z

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.

Observation 30d773a9-73e4-4501-b508-87dee65f16ad · outbound

This paper cites Cosmological constraints on the matter equation of state,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Cosmological constraints on the matter equation of state,

Reference 89

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.379312Z

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.

Observation ef70f96f-2b28-4370-9fa0-a1f6c21f2d45 · outbound

This paper cites Equation of State of Dark Matter after Planck Data,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Equation of State of Dark Matter after Planck Data,

Reference 90

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.360851Z

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.

Observation 69379deb-b9b3-426f-a383-66d63bc177c5 · outbound

This paper cites Constrain- ing the Properties of Dark Matter with Observations of the Cosmic Microwave Background,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Constrain- ing the Properties of Dark Matter with Observations of the Cosmic Microwave Background,

Reference 91

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.343167Z

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.

Observation 686317ad-028f-4b05-aa51-ce6d8c4037bc · outbound

This paper cites Dark Matter Equation of State through Cosmic History,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Dark Matter Equation of State through Cosmic History,

Reference 92

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.322675Z

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.

Observation 06dc648d-d637-471e-a349-e04013f022bb · outbound

This paper cites Evidence for non-cold dark matter from DESI DR2 measurements.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Evidence for non-cold dark matter from DESI DR2 measurements

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:23.545649Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f6c8005-a23a-45be-a4da-d943c7dfbb43 · outbound

This paper cites When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior,

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:23.552658Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 17663d0f-1787-43e3-98c4-3c9b5c89a5c2 · outbound

This paper cites an unresolved cited work.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unresolved cited work

Reference 95

Resolution: unresolved; raw_fallback, observed 2026-08-06T22:01:25.305190Z

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.

Observation 3caf0d03-ac73-4507-8055-7798504d3499 · outbound

This paper cites f(R) Theories Of Grav- ity,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter f(R) Theories Of Grav- ity,

Reference 96

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.286987Z

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.

Observation d2a8dae5-53e6-40da-943a-505497536891 · outbound

This paper cites f(R) theories,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter f(R) theories,

Reference 97

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.269937Z

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.

Observation 47a0c8da-54fb-47a7-950b-853c01f672a8 · outbound

This paper cites Unified cosmic history in modified gravity: from F(R) theory to Lorentz non- invariant models,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Unified cosmic history in modified gravity: from F(R) theory to Lorentz non- invariant models,

Reference 98

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.248698Z

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.

Observation 57b015e3-e6ab-4bb2-8421-59d0324c65eb · outbound

This paper cites Extended Theories of Gravity,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Extended Theories of Gravity,

Reference 99

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.231242Z

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.

Observation 3aff1f13-4ff9-4d1e-b630-64156f60b54e · outbound

This paper cites Modi- fied Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Modi- fied Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution,

Reference 100

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.214241Z

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.

Observation 64312b35-2218-47f5-b3f2-3e93f618b804 · outbound

This paper cites Dark matter in spiral galaxies. II - Galaxies with H I rotation curves,.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter Dark matter in spiral galaxies. II - Galaxies with H I rotation curves,

Reference 101

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.186119Z

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.

Observation 31a23242-60aa-40b3-bf3d-2a60e241c3e3 · outbound

This paper cites On the Use of Galaxy Rotation Curves to Test the Modified Dynamics.

ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter On the Use of Galaxy Rotation Curves to Test the Modified Dynamics

Reference 102

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T22:01:25.165176Z

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.

Pith citing papers

Observation 4d86058f-cb71-4cfc-96f6-78e2e4aa35b2 · inbound

Tsallis-Cirto Hubble parameter: Explaining DESI data and High redshift Supermassive Black Hole cites this paper.

Tsallis-Cirto Hubble parameter: Explaining DESI data and High redshift Supermassive Black Hole ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-05-19T11:57:16.204186Z

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.

Observation 96cc2caa-5c58-41ee-ba0f-acec9507a12c · inbound

Tsallis-Cirto Hubble parameter: Explaining DESI data and High redshift Supermassive Black Hole cites this paper.

Tsallis-Cirto Hubble parameter: Explaining DESI data and High redshift Supermassive Black Hole ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T10:47:12.072300Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9af785e7-e67c-45ed-bd41-94e35f150141 · inbound