ERD

Multi-resolution Bayesian CMB component separation through Wiener filtering with a pseudo-inverse preconditioner

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

X. Planck Low Frequency Instrument frequency maps with sample-based error propagation

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

BeyondPlanck VII. Bayesian estimation of gain and absolute calibration for CMB experiments

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

XIII. Intensity foreground sampling, degeneracies, and priors

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

Cosmological perturbations engendered by discrete relativistic species

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

IX. Bandpass and beam leakage corrections

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

III. Commander3

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

From BEYONDPLANCK to COSMOGLOBE: Preliminary WMAP Q-band analysis

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

XI. Bayesian CMB analysis with sample-based end-to-end error propagation

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

V. Minimal ADC Corrections for Planck LFI

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

II. CMB mapmaking through Gibbs sampling

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

XIV. Polarized foreground emission between 30 and 70 GHz

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

Evidence for line-of-sight frequency decorrelation of polarized dust emission in Planck data

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

BeyondPlanck IV. On end-to-end simulations in CMB analysis -- Bayesian versus frequentist statistics

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

From BeyondPlanck to Cosmoglobe: Open Science, Reproducibility, and Data Longevity

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

Planck intermediate results

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

COSMOGLOBE: Towards end-to-end CMB cosmological parameter estimation without likelihood approximations

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

XII. Cosmological parameter constraints with end-to-end error propagation

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

VI. Noise characterization and modeling

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

COSMOGLOBE: Simulating zodiacal emission with ZodiPy

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

Constraints on the spectral index of polarized synchrotron emission from WMAP and Faraday-corrected S-PASS data

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

VIII. Efficient sidelobe convolution and corrections through spin harmonics

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

XV. Limits on large-scale polarized anomalous microwave emission from Planck LFI and WMAP

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

Planck 2018 results

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

A Monte Carlo comparison between template-based and Wiener-filter CMB dipole estimators

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

Periodic Reporting for period 3 - Bits2Cosmology (Time-domain Gibbs sampling: From bits to inflationary gravitational wa...

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

Data Management Plan

Project: Bits2Cosmology

Updated at: 27-04-2024

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Project acronym Bits2Cosmology

Resources

Selected filters:

Multi-resolution Bayesian CMB component separation through Wiener filtering with a pseudo-inverse preconditioner

X. <i>Planck</i> Low Frequency Instrument frequency maps with sample-based error propagation

BeyondPlanck VII. Bayesian estimation of gain and absolute calibration for CMB experiments

XIII. Intensity foreground sampling, degeneracies, and priors

Cosmological perturbations engendered by discrete relativistic species

IX. Bandpass and beam leakage corrections

III. Commander3

BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data

From BEYONDPLANCK to COSMOGLOBE: Preliminary WMAP <i>Q</i>-band analysis

XI. Bayesian CMB analysis with sample-based end-to-end error propagation

V. Minimal ADC Corrections for <i>Planck</i> LFI

II. CMB mapmaking through Gibbs sampling

XIV. Polarized foreground emission between 30 and 70 GHz

Evidence for line-of-sight frequency decorrelation of polarized dust emission in Planck data

Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations

BeyondPlanck IV. On end-to-end simulations in CMB analysis -- Bayesian versus frequentist statistics

From BeyondPlanck to Cosmoglobe: Open Science, Reproducibility, and Data Longevity

Planck intermediate results

COSMOGLOBE: Towards end-to-end CMB cosmological parameter estimation without likelihood approximations

XII. Cosmological parameter constraints with end-to-end error propagation

VI. Noise characterization and modeling

COSMOGLOBE: Simulating zodiacal emission with ZodiPy

Constraints on the spectral index of polarized synchrotron emission from WMAP and Faraday-corrected S-PASS data

VIII. Efficient sidelobe convolution and corrections through spin harmonics

XV. Limits on large-scale polarized anomalous microwave emission from <i>Planck</i> LFI and WMAP

Planck 2018 results

A Monte Carlo comparison between template-based and Wiener-filter CMB dipole estimators

Periodic Reporting for period 3 - Bits2Cosmology (Time-domain Gibbs sampling: From bits to inflationary gravitational wa...

Data Management Plan