Paper Citation Record · LEDGER

Turning a negative neutrino mass into a positive optical depth

As of 20 August 2026, this Paper Citation Record lists 67 of 67 outbound references and 34 inbound Pith citation observations for arXiv:2504.21813.

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pith.paper-citation-record.v1
2504.21813 v1

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measured 67 of 67 reference resolution

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Outbound references

Observation 5cd322df-9694-4bcc-a31f-518edf3b91aa · outbound

This paper cites Navas et al.

Turning a negative neutrino mass into a positive optical depth Navas et al

Reference 1

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Observation 137249c9-ffc7-4e71-a162-8fe9adb41ed4 · outbound

This paper cites Neutrinos in Cosmology.

Turning a negative neutrino mass into a positive optical depth Neutrinos in Cosmology

Reference 2

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Observation c4141ebe-58a2-4242-b5af-01edd61e3c2b · outbound

This paper cites an unresolved cited work.

Turning a negative neutrino mass into a positive optical depth Unresolved cited work

Reference 3

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Observation d9884458-027a-4218-bbe6-c4ce5010ba28 · outbound

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

Turning a negative neutrino mass into a positive optical depth DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 4

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Observation 53917a81-7c5c-432b-b113-bbc47e4e5a2a · outbound

This paper cites No $\nu$s is Good News.

Turning a negative neutrino mass into a positive optical depth No $\nu$s is Good News

Reference 5

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Observation fde351c7-76b5-4504-8303-81ff5fd4eb03 · outbound

This paper cites NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations.

Turning a negative neutrino mass into a positive optical depth NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations

Reference 6

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Observation 9d07a8e7-3df8-4dfb-a5c2-e3e319dd6d2e · outbound

This paper cites Massive neutrinos and cosmic composition.

Turning a negative neutrino mass into a positive optical depth Massive neutrinos and cosmic composition

Reference 7

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Observation 6cdba87e-fe6f-4e06-b980-21b591ba7e0c · outbound

This paper cites Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape.

Turning a negative neutrino mass into a positive optical depth Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape

Reference 8

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Observation af8a80e1-1081-4e60-83b4-5a960b84dd46 · outbound

This paper cites The Cosmological Preference for Negative Neutrino Mass.

Turning a negative neutrino mass into a positive optical depth The Cosmological Preference for Negative Neutrino Mass

Reference 9

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Observation 5b4bcae1-6df7-4b2a-86f8-793a08d3ef19 · outbound

This paper cites Living at the Edge: A Critical Look at the Cosmological Neutrino Mass Bound.

Turning a negative neutrino mass into a positive optical depth Living at the Edge: A Critical Look at the Cosmological Neutrino Mass Bound

Reference 10

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Observation dfe236f4-8bb8-4da3-ac39-ef5233e4ce57 · outbound

This paper cites Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension.

Turning a negative neutrino mass into a positive optical depth Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension

Reference 11

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Observation b5cac60b-2530-4a94-a04c-1d193bffe4e3 · outbound

This paper cites What's the matter with $\Sigma m_{\nu}$?.

Turning a negative neutrino mass into a positive optical depth What's the matter with $\Sigma m_{\nu}$?

Reference 12

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Observation cd628d71-77fa-4011-b621-93523ded920e · outbound

This paper cites Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations.

Turning a negative neutrino mass into a positive optical depth Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 13

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Observation a8098b7f-609b-4643-80c2-de67a673962c · outbound

This paper cites Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes.

Turning a negative neutrino mass into a positive optical depth Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 14

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Observation 7801e092-c965-4714-8d77-594fed1bbdef · outbound

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Turning a negative neutrino mass into a positive optical depth Unresolved cited work

Reference 15

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Observation 41c66a83-b2d3-4bbf-beb9-aa93d45ae944 · outbound

This paper cites Investigating Late-Time Dark Energy and Massive Neutrinos in Light of DESI Y1 BAO.

Turning a negative neutrino mass into a positive optical depth Investigating Late-Time Dark Energy and Massive Neutrinos in Light of DESI Y1 BAO

Reference 16

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Observation 8de492bb-93df-4980-b628-c6882efc4839 · outbound

This paper cites Cosmological Information from Lensed CMB Power Spectra.

Turning a negative neutrino mass into a positive optical depth Cosmological Information from Lensed CMB Power Spectra

Reference 17

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Observation 65371f70-66d0-4310-aa71-42abc48f38ca · outbound

This paper cites Cosmic Microwave Weak lensing data as a test for the dark universe.

Turning a negative neutrino mass into a positive optical depth Cosmic Microwave Weak lensing data as a test for the dark universe

Reference 18

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Observation 21fe1a8c-a790-49ef-aa7a-034626d8f5f7 · outbound

This paper cites Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data.

Turning a negative neutrino mass into a positive optical depth Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data

Reference 19

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Observation 9ee6a1fa-79a1-48c7-bef3-205733c25bf9 · outbound

This paper cites Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results.

Turning a negative neutrino mass into a positive optical depth Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results

Reference 20

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Observation ae186ce4-5ada-45e9-855d-22ccda89392d · outbound

This paper cites Towards a cosmological neutrino mass detection.

Turning a negative neutrino mass into a positive optical depth Towards a cosmological neutrino mass detection

Reference 21

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Observation 6824109f-6a00-479d-906f-1ab74d7a3a6d · outbound

This paper cites Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization.

Turning a negative neutrino mass into a positive optical depth Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization

Reference 22

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Observation 725f0f71-62be-4cf9-b8f0-d0919064806b · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Turning a negative neutrino mass into a positive optical depth Planck 2018 results. VI. Cosmological parameters

Reference 23

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This paper cites Planck 2013 results. XVI. Cosmological parameters.

Turning a negative neutrino mass into a positive optical depth Planck 2013 results. XVI. Cosmological parameters

Reference 24

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Observation 53533d51-3d54-43ef-9f4f-1f836a225f3f · outbound

This paper cites Planck 2015 results. XIII. Cosmological parameters.

Turning a negative neutrino mass into a positive optical depth Planck 2015 results. XIII. Cosmological parameters

Reference 25

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Observation db4ca2f5-b1f3-4ee0-9abb-6ccb3b38885f · outbound

This paper cites Turning a negative neutrino mass into a positive optical depth.

Turning a negative neutrino mass into a positive optical depth Turning a negative neutrino mass into a positive optical depth

Reference 26

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Observation 5e8f432d-2d52-4a4b-a3b4-74b7c60ae784 · outbound

This paper cites Model-Independent Reionization Observables in the CMB.

Turning a negative neutrino mass into a positive optical depth Model-Independent Reionization Observables in the CMB

Reference 27

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Observation 7d489f79-16d9-464e-8c5a-fb840a334985 · outbound

This paper cites Complete Reionization Constraints from Planck 2015 Polarization.

Turning a negative neutrino mass into a positive optical depth Complete Reionization Constraints from Planck 2015 Polarization

Reference 28

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This paper cites SRoll2: an improved mapmaking approach to reduce large-scale systematic effects in the Planck High Frequency Instrument legacy maps.

Turning a negative neutrino mass into a positive optical depth SRoll2: an improved mapmaking approach to reduce large-scale systematic effects in the Planck High Frequency Instrument legacy maps

Reference 29

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Observation 347ec533-7304-4bbb-b76d-99c7e28bc5ce · outbound

This paper cites RELIKE: Reionization Effective Likelihood from Planck 2018 Data.

Turning a negative neutrino mass into a positive optical depth RELIKE: Reionization Effective Likelihood from Planck 2018 Data

Reference 30

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This paper cites Inflationary vs. Reionization Features from Planck 2015 Data.

Turning a negative neutrino mass into a positive optical depth Inflationary vs. Reionization Features from Planck 2015 Data

Reference 31

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Observation a2d87e9b-a01b-4ebc-80bc-cf9ab3fb2a94 · outbound

This paper cites CMB lensing from Planck PR4 maps.

Turning a negative neutrino mass into a positive optical depth CMB lensing from Planck PR4 maps

Reference 32

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This paper cites The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth.

Turning a negative neutrino mass into a positive optical depth The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth

Reference 33

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Turning a negative neutrino mass into a positive optical depth Unresolved cited work

Reference 34

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

Turning a negative neutrino mass into a positive optical depth DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 35

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This paper cites The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset.

Turning a negative neutrino mass into a positive optical depth The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset

Reference 36

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Turning a negative neutrino mass into a positive optical depth Cosmology and the neutrino mass ordering

Reference 37

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This paper cites Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data.

Turning a negative neutrino mass into a positive optical depth Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data

Reference 38

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This paper cites Planck 2013 results. XXII. Constraints on inflation.

Turning a negative neutrino mass into a positive optical depth Planck 2013 results. XXII. Constraints on inflation

Reference 39

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This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes.

Turning a negative neutrino mass into a positive optical depth The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

Reference 40

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This paper cites Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code.

Turning a negative neutrino mass into a positive optical depth Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code

Reference 41

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Turning a negative neutrino mass into a positive optical depth MontePython 3: boosted MCMC sampler and other features

Reference 42

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Turning a negative neutrino mass into a positive optical depth Cobaya: Code for Bayesian Analysis of hierarchical physical models

Reference 43

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Turning a negative neutrino mass into a positive optical depth GetDist: a Python package for analysing Monte Carlo samples

Reference 44

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Turning a negative neutrino mass into a positive optical depth Procoli: Profiles of cosmological likelihoods

Reference 45

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Turning a negative neutrino mass into a positive optical depth The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023

Reference 46

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Turning a negative neutrino mass into a positive optical depth Self-interacting neutrinos in light of recent CMB and LSS data

Reference 47

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Turning a negative neutrino mass into a positive optical depth Confronting Cold New Early Dark Energy and its Equation of State with Updated CMB, Supernovae, and BAO Data

Reference 48

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Turning a negative neutrino mass into a positive optical depth A Ratio-Preserving Approach to Cosmological Concordance

Reference 49

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This paper cites Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension.

Turning a negative neutrino mass into a positive optical depth Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension

Reference 50

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Turning a negative neutrino mass into a positive optical depth CMB Observables and Their Cosmological Implications

Reference 51

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Turning a negative neutrino mass into a positive optical depth Concordance and Discordance in Cosmology

Reference 52

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Turning a negative neutrino mass into a positive optical depth Evidence for horizon-scale power from CMB polarization

Reference 53

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Turning a negative neutrino mass into a positive optical depth Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 54

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Turning a negative neutrino mass into a positive optical depth The Cosmology Large Angular Scale Surveyor

Reference 55

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Turning a negative neutrino mass into a positive optical depth A Projected Estimate of the Reionization Optical Depth Using the CLASS Experiment's Sample-Variance Limited E-Mode Measurement

Reference 56

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Turning a negative neutrino mass into a positive optical depth A Measurement of the Largest-Scale CMB E-mode Polarization with CLASS

Reference 57

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Observation 38c522da-f71c-4308-ad51-ce9883c3b0f4 · outbound

This paper cites Hazumi et al.

Turning a negative neutrino mass into a positive optical depth Hazumi et al

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-16T05:00:38.179742Z

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Observation 36fcd097-3529-4997-bb39-9531136aa797 · outbound

This paper cites Probing the Early History of Cosmic Reionization by Future Cosmic Microwave Background Experiments.

Turning a negative neutrino mass into a positive optical depth Probing the Early History of Cosmic Reionization by Future Cosmic Microwave Background Experiments

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-16T05:00:38.184162Z

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Observation 4d42f6f5-c3a4-49cb-a93e-b182590ea883 · outbound

This paper cites Eliminating the optical depth nuisance from the CMB with 21 cm cosmology.

Turning a negative neutrino mass into a positive optical depth Eliminating the optical depth nuisance from the CMB with 21 cm cosmology

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-16T05:00:38.188541Z

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Observation f414e523-092f-4bff-8f9a-5e6612bc943f · outbound

This paper cites Mitigating the optical depth degeneracy in the cosmological measurement of neutrino masses using 21-cm observations.

Turning a negative neutrino mass into a positive optical depth Mitigating the optical depth degeneracy in the cosmological measurement of neutrino masses using 21-cm observations

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-16T05:00:38.192912Z

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Observation 6f07f228-2e56-43cc-96f8-d20e7d920b6d · outbound

This paper cites The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5.

Turning a negative neutrino mass into a positive optical depth The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-16T05:00:38.197112Z

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Observation 945da10a-0720-482a-a1d5-a908aaa266c9 · outbound

This paper cites Early results from GLASS-JWST. III: Galaxy candidates at z$\sim$9-15.

Turning a negative neutrino mass into a positive optical depth Early results from GLASS-JWST. III: Galaxy candidates at z$\sim$9-15

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-16T05:00:38.201315Z

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Observation e593f075-46a3-47ca-874f-d3d1421dca92 · outbound

This paper cites Overview of the JWST Advanced Deep Extragalactic Survey (JADES).

Turning a negative neutrino mass into a positive optical depth Overview of the JWST Advanced Deep Extragalactic Survey (JADES)

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-16T05:00:38.205441Z

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Observation 61f784c5-c06f-48d8-a56e-7c40c13bf85d · outbound

This paper cites A Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch.

Turning a negative neutrino mass into a positive optical depth A Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-16T05:00:38.210054Z

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Observation 85d1e8cb-b629-47bc-865c-ebf1cb1dc6c2 · outbound

This paper cites Reionization after JWST: a photon budget crisis?.

Turning a negative neutrino mass into a positive optical depth Reionization after JWST: a photon budget crisis?

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-16T05:00:38.214360Z

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Observation 6bcca286-3a3c-4151-9b36-49168d71d73a · outbound

This paper cites Sailer, G.

Turning a negative neutrino mass into a positive optical depth Sailer, G

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-16T05:00:38.218995Z

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Pith citing papers

Observation db4ca2f5-b1f3-4ee0-9abb-6ccb3b38885f · inbound

Turning a negative neutrino mass into a positive optical depth cites this paper.

Turning a negative neutrino mass into a positive optical depth Turning a negative neutrino mass into a positive optical depth

Reference 26

Resolution: malformed identifier; no resolver link, observed 2026-08-16T05:00:37.940061Z

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Observation 85aded95-7139-4a53-9d64-4115eecdb899 · inbound

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On the tension between DESI DR2 BAO and CMB Turning a negative neutrino mass into a positive optical depth

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-16T01:06:27.361085Z

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Unavailable: canonical work link unavailable.

Observation ad2dd70e-c7e9-4583-be5a-441e9fdc8a98 · inbound

The CMB optical depth constrains the duration of reionization cites this paper.

The CMB optical depth constrains the duration of reionization Turning a negative neutrino mass into a positive optical depth

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T15:15:34.657364Z

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Observation 3e8f1f34-2d4e-4fb6-a049-78f9f56c4632 · inbound

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Flash Ionization of the Early Universe by Pop III.1 Supermassive Stars Turning a negative neutrino mass into a positive optical depth

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-06T23:21:40.948619Z

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Unavailable: canonical work link unavailable.

Observation ab5e46ce-4e92-4d51-ab44-798531054d5e · inbound

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Type II Seesaw Leptogenesis in a Majoron background Turning a negative neutrino mass into a positive optical depth

Reference 105

Resolution: verified exact; arxiv_id, observed 2026-05-19T07:52:10.254501Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation cc1ddcab-a155-465d-a749-769f31300bdc · inbound

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The BAO-CMB Tension and Implications for Inflation Turning a negative neutrino mass into a positive optical depth

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-06T16:53:13.306507Z

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Observation 109bf04f-4e13-4462-b38f-21ffc2ab080a · inbound

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Probing the ionizing photon output of galaxies near cosmic dawn with the patchy kSZ effect Turning a negative neutrino mass into a positive optical depth

Reference 106

Resolution: unresolved; no resolver link, observed 2026-08-06T14:45:35.935226Z

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Unavailable: canonical work link unavailable.

Observation cbf3f630-9f74-47b4-a372-71d9da4f69e9 · inbound

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Rapid late-time reionization: constraints and cosmological implications Turning a negative neutrino mass into a positive optical depth

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-05T14:41:15.447034Z

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Observation a5880d13-2c7a-4f1b-9a0e-c8554861dcba · inbound

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A New Boundary Condition on Reionization Turning a negative neutrino mass into a positive optical depth

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-04T20:07:40.731068Z

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Observation c31280e4-07cc-419c-b77d-d06427bad678 · inbound

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Cosmic $\tau$ensions Indirectly Correlate with Reionization Optical Depth Turning a negative neutrino mass into a positive optical depth

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-04T18:49:51.397878Z

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Unavailable: canonical work link unavailable.

Observation e3e6fb6b-eeeb-485f-8101-e6e1dec12fd6 · inbound

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Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-04T08:41:21.722083Z

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Unavailable: canonical work link unavailable.

Observation b1a04054-bf04-42ce-a4f6-2203d83328c6 · inbound

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Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-03T17:10:56.033326Z

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Observation e4d09542-e726-46ee-a9c7-e11e3a896471 · inbound

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Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity Turning a negative neutrino mass into a positive optical depth

Reference 111

Resolution: verified exact; arxiv_id, observed 2026-05-16T18:01:09.293872Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation c0f0da9f-bedb-4f94-bdc3-f59edaa3190a · inbound

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Robust Preference for Dark Sector Interactions Turning a negative neutrino mass into a positive optical depth

Reference 154

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:49.005144Z

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Unavailable: canonical work link unavailable.

Observation 8a905910-f047-4563-af50-d9bc7b655697 · inbound

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Disentangling cosmic distance tensions with early and late dark energy Turning a negative neutrino mass into a positive optical depth

Reference 52

Resolution: verified exact; arxiv_id, observed 2026-05-11T08:06:00.702820Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 4ed6ee86-4c88-46e2-ac67-75b3de5e0747 · inbound

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Into the Gompverse: A robust Gompertzian reionization model for CMB analyses Turning a negative neutrino mass into a positive optical depth

Reference 9

Resolution: verified exact; arxiv_id, observed 2026-05-11T11:36:03.085975Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 866068e3-e868-4145-894d-56393a7194ff · inbound

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Faster CMB lensing with control variates Turning a negative neutrino mass into a positive optical depth

Reference 31

Resolution: verified exact; arxiv_id, observed 2026-05-20T09:08:09.686114Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 449d02e0-5184-4e87-aec7-52678156b101 · inbound

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Compressed Gaussian likelihood for the Planck low-$\ell$ data Turning a negative neutrino mass into a positive optical depth

Reference 15

Resolution: verified exact; arxiv_id, observed 2026-07-02T10:56:52.933267Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 9b420002-bff3-46c2-9ba6-55937a6228a7 · inbound

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Reconstructing dark energy with fewer assumptions Turning a negative neutrino mass into a positive optical depth

Reference 86

Resolution: verified exact; arxiv_id, observed 2026-07-02T14:57:04.205190Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 511ae130-c955-4b0b-b58f-eb9050d92150 · inbound

A self-consistent analytical model for both the photoionization rate and reionization history cites this paper.

A self-consistent analytical model for both the photoionization rate and reionization history Turning a negative neutrino mass into a positive optical depth

Reference 109

Resolution: verified exact; arxiv_id, observed 2026-07-04T02:29:23.358510Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation a0d51ddf-30ba-4fb3-a788-e59765a3c5e0 · inbound

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Raising the reionization optical depth with inflationary CMB features Turning a negative neutrino mass into a positive optical depth

Reference 10

Resolution: verified exact; arxiv_id, observed 2026-07-04T05:29:35.779912Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 6c31358c-f312-4af8-a7a6-915a9de37d03 · inbound

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A hidden reionization prior biases cosmological inference Turning a negative neutrino mass into a positive optical depth

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-07-01T17:45:51.538031Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 860eed58-0719-4801-9fd1-329be82a8d32 · inbound

Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM cites this paper.

Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM Turning a negative neutrino mass into a positive optical depth

Reference 53

Resolution: verified exact; arxiv_id, observed 2026-07-01T01:15:13.399169Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 34170e5a-f9e9-4159-8c1e-907e02f5ca51 · inbound

Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM cites this paper.

Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM Turning a negative neutrino mass into a positive optical depth

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-02T09:29:12.750702Z

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Unavailable: canonical work link unavailable.

Observation d0c3380e-0cc6-46bc-b76c-af0f52a8152b · inbound

Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Turning a negative neutrino mass into a positive optical depth

Reference 225

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:15:42.761367Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 3455217d-b0f2-4464-9bf4-c7de9f86248e · inbound

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation Turning a negative neutrino mass into a positive optical depth

Reference 185

Resolution: verified exact; arxiv_id, observed 2026-07-02T06:16:43.329718Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation ff03ab2b-d04d-453d-b006-34c76c5c9e7c · inbound

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Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data Turning a negative neutrino mass into a positive optical depth

Reference 191

Resolution: unresolved; no resolver link, observed 2026-07-12T04:18:55.037825Z

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Unavailable: canonical work link unavailable.

Observation 078b4f8c-06ee-483a-a2ca-67206f2b8a9e · inbound

The Status of Single Scalar Field Dark Energy cites this paper.

The Status of Single Scalar Field Dark Energy Turning a negative neutrino mass into a positive optical depth

Reference 80

Resolution: verified exact; local_arxiv, observed 2026-07-10T18:27:31.592640Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation aef00320-20ec-4dbd-9944-5b7056b3d8f4 · inbound

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The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions Turning a negative neutrino mass into a positive optical depth

Reference 172

Resolution: unresolved; no resolver link, observed 2026-08-02T05:48:21.559462Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 51d70c28-2d6c-4630-843d-1813783bc0d3 · inbound

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization cites this paper.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Turning a negative neutrino mass into a positive optical depth

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-01T17:17:51.197024Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f290ccf-f8da-4450-91fd-586f967673d4 · inbound

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization cites this paper.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Turning a negative neutrino mass into a positive optical depth

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-04T03:21:43.320927Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3a7025f1-c83d-44eb-8e7a-3eb6a92832c7 · inbound

DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints cites this paper.

DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints Turning a negative neutrino mass into a positive optical depth

Reference 137

Resolution: unresolved; no resolver link, observed 2026-08-01T07:53:04.272372Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b95604a-15f1-4452-b87d-870f44599e15 · inbound

DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints cites this paper.

DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints Turning a negative neutrino mass into a positive optical depth

Reference 137

Resolution: unresolved; no resolver link, observed 2026-08-03T01:46:05.859310Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 196c3424-f953-4779-941e-7e306f276163 · inbound

Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift cites this paper.

Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift Turning a negative neutrino mass into a positive optical depth

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-04T18:21:08.142665Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.