No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization | Paper Citation Record

Observation 6ca4f7c3-06c7-4763-9f51-09ffa5b0ff35 · outbound

This paper cites Into the Gompverse: A robust Gompertzian reionization model for CMB analyses.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Into the Gompverse: A robust Gompertzian reionization model for CMB analyses

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Observation 8e02a8ae-7ed5-4e01-9686-7420d3714e44 · outbound

This paper cites Five parameters are all you need (in $\Lambda$CDM).

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Five parameters are all you need (in $\Lambda$CDM)

Reference 2

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Observation 1038992c-50c9-4497-8bd0-5b8919024ec3 · outbound

This paper cites Neural network emulation of reionization to constrain new physics with early- and late-time probes.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Neural network emulation of reionization to constrain new physics with early- and late-time probes

Reference 3

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Observation 931e9e33-359f-4c18-865d-3d898b127d45 · outbound

This paper cites Planck intermediate results. XLVII. Planck constraints on reionization history.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Planck intermediate results. XLVII. Planck constraints on reionization history

Reference 4

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Observation d20a6cee-b6d3-4448-b449-52e257cff4fc · outbound

This paper cites A new parameterization of the reionisation history.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization A new parameterization of the reionisation history

Reference 5

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Observation 009ffab0-ec8b-47a8-a0b9-88155da26313 · outbound

This paper cites Parametrizing the Reionization History with the Redshift Midpoint, Duration, and Asymmetry.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Parametrizing the Reionization History with the Redshift Midpoint, Duration, and Asymmetry

Reference 6

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Observation 8fd1c5d8-77b9-4aca-8aa0-f0ed2287f874 · outbound

This paper cites , keywords =.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization , keywords =

Reference 7

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

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

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

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Observation 4fed44a3-6c62-4e3e-9406-45a3d145bb04 · outbound

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

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 9

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Observation e12ba933-1940-465a-9dc3-68032eb2a815 · outbound

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

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 10

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Observation 4028cd96-4559-4af4-8cd4-eda2881f7e78 · outbound

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

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Planck 2018 results. V. CMB power spectra and likelihoods

Reference 11

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Observation 8d2abe81-1915-4122-81fa-934a18ea913b · outbound

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

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters

Reference 12

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Observation 4ac662a2-66dd-400b-b9bb-0fe4484bc113 · outbound

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

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape

Reference 13

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Observation e5413535-526a-46d5-9abd-f1cdeb3ea210 · outbound

This paper cites The Cosmological Preference for Negative Neutrino Mass.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization The Cosmological Preference for Negative Neutrino Mass

Reference 14

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Observation 494b5279-59de-4800-80da-caaebb8565d2 · outbound

This paper cites Planck 2018 results. I. Overview and the cosmological legacy of Planck.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Planck 2018 results. I. Overview and the cosmological legacy of Planck

Reference 15

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Observation 7ebe6e2f-ba3c-4894-9202-40a4b740bfd9 · outbound

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

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization SRoll2: an improved mapmaking approach to reduce large-scale systematic effects in the Planck High Frequency Instrument legacy maps

Reference 16

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Observation a19603b5-8ad9-46d7-87f8-f8feddadaaf9 · outbound

This paper cites SRoll3: A neural network approach to reduce large-scale systematic effects in the Planck High Frequency Instrument maps.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization SRoll3: A neural network approach to reduce large-scale systematic effects in the Planck High Frequency Instrument maps

Reference 17

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Observation 1b05b1b6-6be1-4477-bc76-44e3c2247a97 · outbound

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

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Reionization optical depth determination from Planck HFI data with ten percent accuracy

Reference 18

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Observation 1e3a3f5f-e0d8-447d-a1e7-18b39e7a301a · outbound

This paper cites arXiv e-prints , keywords =.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization arXiv e-prints , keywords =

Reference 19

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Observation ceb5c0f6-7b54-4b5a-860a-9b19cbf35cda · outbound

This paper cites Cosmological constraints from the DESI DR1 Bispectrum Full-Shape and DR2 BAO.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Cosmological constraints from the DESI DR1 Bispectrum Full-Shape and DR2 BAO

Reference 20

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Observation 4a238745-6bcb-4672-982b-22a1cfb42be1 · outbound

This paper cites Introducing the THESAN project: radiation-magnetohydrodynamic simulations of the epoch of reionization.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Introducing the THESAN project: radiation-magnetohydrodynamic simulations of the epoch of reionization

Reference 21

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Observation 9d29bb8c-65ed-44bb-a94f-05379260eed3 · outbound

This paper cites , keywords =.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization , keywords =

Reference 22

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Observation 0ee1b0ed-54b1-47bc-9ced-8f4d1ff00278 · outbound

This paper cites The Sherwood-Relics simulations: overview and impact of patchy reionization and pressure smoothing on the intergalactic medium.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization The Sherwood-Relics simulations: overview and impact of patchy reionization and pressure smoothing on the intergalactic medium

Reference 23

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Observation 4e0d9718-1d1d-47a7-b92f-9c7c667efdf5 · outbound

This paper cites Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization

Reference 24

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Observation 2619fcf6-7dbb-43d4-afc8-df63ed0504d0 · outbound

This paper cites Raising the reionization optical depth with inflationary CMB features.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Raising the reionization optical depth with inflationary CMB features

Reference 25

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Observation 7871bf4d-fdfb-4ce1-a480-9cccacdcf8d5 · outbound

This paper cites Fireworks at Cosmic Dawn: relieving BAO-CMB tensions with the Pop III.1 Flash.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Fireworks at Cosmic Dawn: relieving BAO-CMB tensions with the Pop III.1 Flash

Reference 26

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Observation 82d18987-ba09-4604-866a-9e3dfc62f35c · outbound

This paper cites Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument

Reference 27

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Observation 45aaae81-4c62-4d33-97a7-b3ca749d4f55 · outbound

This paper cites A Detailed Description of the CamSpec Likelihood Pipeline and a Reanalysis of the Planck High Frequency Maps.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization A Detailed Description of the CamSpec Likelihood Pipeline and a Reanalysis of the Planck High Frequency Maps

Reference 28

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Observation 533659dc-4bb7-4665-ae71-2b5c9563ead8 · outbound

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

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth

Reference 29

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Observation 209669dc-0796-4983-bccf-b862ebef3a49 · outbound

This paper cites CMB lensing from Planck PR4 maps.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization CMB lensing from Planck PR4 maps

Reference 30

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Observation eedfa553-e7f2-4878-aaa0-f9b6843d2265 · outbound

This paper cites , keywords =.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization , keywords =

Reference 31

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Observation 3b496aa5-b061-4abf-9290-93f5a517cfe0 · outbound

This paper cites IGM damping wing constraints on reionisation from covariance reconstruction of two $z\gtrsim7$ QSOs.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization IGM damping wing constraints on reionisation from covariance reconstruction of two $z\gtrsim7$ QSOs

Reference 32

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Observation a3d28855-2aab-432e-9406-2053d1564eb3 · outbound

This paper cites IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample

Reference 33

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Observation c72654a6-9a3c-4c04-833e-990b1e361e21 · outbound

This paper cites Damping wings in the Lyman-{\alpha} forest: a model-independent measurement of the neutral fraction at 5.4<z<6.1.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Damping wings in the Lyman-{\alpha} forest: a model-independent measurement of the neutral fraction at 5.4<z<6.1

Reference 34

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Observation 9e830d8c-8d49-4106-964f-0d1105761bd2 · outbound

This paper cites Chronicling the reionization history at $6\lesssim z \lesssim 7$ with emergent quasar damping wings.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Chronicling the reionization history at $6\lesssim z \lesssim 7$ with emergent quasar damping wings

Reference 35

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Observation 86e8a959-94c2-49e9-8fa9-12bb27820200 · outbound

This paper cites Rapid late-time reionization: constraints and cosmological implications.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Rapid late-time reionization: constraints and cosmological implications

Reference 36

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Observation 8dddaa93-2c6c-4c30-9dd3-b2b1a5b1a419 · outbound

This paper cites A New Constraint on the Optical Depth from the Reionization History Independent of CMB Large-Scale E-Mode Polarization.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization A New Constraint on the Optical Depth from the Reionization History Independent of CMB Large-Scale E-Mode Polarization

Reference 37

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Observation 99b8df1e-1e05-4fa8-9041-11475a5465d6 · outbound

This paper cites The Impact of Cosmic Variance on Inferences of Global Neutral Fraction Derived from Ly$\alpha$ Luminosity Functions During Reionization.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization The Impact of Cosmic Variance on Inferences of Global Neutral Fraction Derived from Ly$\alpha$ Luminosity Functions During Reionization

Reference 38

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Observation 08aea471-7943-4c38-b487-96c6522f7e9a · outbound

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

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Cobaya: Code for Bayesian Analysis of hierarchical physical models

Reference 39

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Observation 5ac9fccd-a134-4ad5-a3b0-3a61bc07c808 · outbound

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

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

Reference 40

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Observation a05755bb-4a50-4b4f-a724-04e532685261 · outbound

This paper cites Planck 2018 results. VIII. Gravitational lensing.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Planck 2018 results. VIII. Gravitational lensing

Reference 41

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Observation 0b87d297-1974-45fd-a5d0-3c3e2ea8de73 · outbound

This paper cites Model-independent evidence in favor of an end to reionization by z~6.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Model-independent evidence in favor of an end to reionization by z~6

Reference 42

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Observation 56e6032f-9f74-40df-8871-89d2a6eefb96 · outbound

This paper cites , keywords =.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization , keywords =

Reference 43

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Observation c11d684b-7e4c-4a15-b344-0317862e3530 · outbound

This paper cites The Effects of Dark Matter Annihilation and Dark Matter-Baryon Velocity Offsets at Cosmic Dawn.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization The Effects of Dark Matter Annihilation and Dark Matter-Baryon Velocity Offsets at Cosmic Dawn

Reference 44

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Observation 3767a489-f913-48f5-9b14-0d01517b3345 · outbound

This paper cites CMB limits on decaying dark matter beyond the ionization threshold.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization CMB limits on decaying dark matter beyond the ionization threshold

Reference 45

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No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization , keywords =

Reference 46

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This paper cites , keywords =.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization , keywords =

Reference 47

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Observation c92e5de0-b8f1-4e98-84f6-7c4b422fd1e8 · outbound

This paper cites The Evolution of the Lyman-Alpha Luminosity Function During Reionization.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization The Evolution of the Lyman-Alpha Luminosity Function During Reionization

Reference 48

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Observation 7d24f780-b41b-4f5c-a579-1d0f67d7c7ef · outbound

This paper cites Census of Ly$\alpha$ Emission from $\sim 600$ Galaxies at $z=5-14$: Evolution of the Ly$\alpha$ Luminosity Function and a Late Sharp Cosmic Reionization.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Census of Ly$\alpha$ Emission from $\sim 600$ Galaxies at $z=5-14$: Evolution of the Ly$\alpha$ Luminosity Function and a Late Sharp Cosmic Reionization

Reference 49

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No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization , keywords =

Reference 50

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No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization , keywords =

Reference 51

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Observation e7824bfa-8e83-48a0-957c-f50bb672789c · outbound

This paper cites Reionization and the Hubble Constant: Correlations in the Cosmic Microwave Background.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Reionization and the Hubble Constant: Correlations in the Cosmic Microwave Background

Reference 52

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Observation 9f7450e9-b457-452d-961b-dd4ab842a6d4 · outbound

This paper cites Cosmic $\tau$ensions Indirectly Correlate with Reionization Optical Depth.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Cosmic $\tau$ensions Indirectly Correlate with Reionization Optical Depth

Reference 53

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Observation aa07dd0a-e21d-423c-960e-c572015ddfb6 · outbound

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

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations

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Observation de05904e-753a-4c47-9a3c-01c8aa105acf · outbound

This paper cites On the nature of the function expressive of the law of human mortality, and on a new mode of determining the value of life contingencies.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization On the nature of the function expressive of the law of human mortality, and on a new mode of determining the value of life contingencies

Reference 55

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Observation 509d4a4c-a992-4dad-9833-e848cddee71d · 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.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization 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 56

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Observation 097ec5a1-c539-4bc6-b751-a99d665fe4f6 · outbound

This paper cites , keywords =.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization , keywords =

Reference 57

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Observation 0bb656a8-02d7-4955-8901-c148b3cb4e82 · outbound

This paper cites , keywords =.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization , keywords =

Reference 58

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Observation 92713a7e-7a25-4c51-a10f-61b2a5a7e837 · outbound

This paper cites , keywords =.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization , keywords =

Reference 59

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