On the computational feasibility of Bayesian end-to-end analysis of LiteBIRD simulations within Cosmoglobe
arXiv:2507.05324 · doi:10.1088/1475-7516/2025/11/041
Abstract
We assess the computational feasibility of end-to-end Bayesian analysis of the JAXA-led LiteBIRD experiment by analysing simulated time ordered data (TOD) for a subset of detectors through the Cosmoglobe and Commander3 framework. The data volume for the simulated TOD is 1.55 TB, or 470 GB after Huffman compression. From this we estimate a total data volume of 238 TB for the full three year mission, or 70 TB after Huffman compression. We further estimate the running time for one Gibbs sample, from TOD to cosmological parameters, to be approximately 3000 CPU hours. The current simulations are based on an ideal instrument model, only including correlated 1/f noise. Future work will consider realistic systematics with full end-to-end error propagation. We conclude that these requirements are well within capabilities of future high-performance computing systems.
arXiv comment18 pages, 4 figures, Published in JCAP
References in corpus (38)
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- Planck 2018 results. X. Constraints on inflation
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- Planck 2018 results. I. Overview and the cosmological legacy of Planck
- A 3D Dust Map Based on Gaia, Pan-STARRS 1 and 2MASS
- The Temperature of the Cosmic Microwave Background
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Sky Maps, Systematic Errors, and Basic Results
- Signature of Gravity Waves in Polarization of the Microwave Background
- A Probe of Primordial Gravity Waves and Vorticity
- BICEP2 / Keck Array x: Constraints on Primordial Gravitational Waves using Planck, WMAP, and New BICEP2/Keck Observations through the 2015 Season
- The Quest for B Modes from Inflationary Gravitational Waves
- Improved limits on the tensor-to-scalar ratio using BICEP and Planck
- The Python Sky Model: software for simulating the Galactic microwave sky
- The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths
- Towards a free-free template for CMB foregrounds
- Planck 2013 results. XIII. Galactic CO emission
- Separation of anomalous and synchrotron emissions using WMAP polarization data
- The LiteBIRD Satellite Mission - Sub-Kelvin Instrument
- The Websky Extragalactic CMB Simulations
- Planck 2018 results. II. Low Frequency Instrument data processing
- Modeling Thermal Dust Emission with Two Components: Application to the Planck HFI Maps
- Updated design of the CMB polarization experiment satellite LiteBIRD
- Results from the Wilkinson Microwave Anisotropy Probe
- Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
- BeyondPlanck III. Commander3
- Forecasting Polarized Radio Sources for CMB observations
- BeyondPlanck XIII. Intensity foreground sampling, degeneracies, and priors
- Gravitational waves and large field inflation
- Simulated catalogs and maps of radio galaxies at millimeter wavelengths in Websky
- A 3D model for CO molecular line emission as a potential CMB polarization contaminant
- Cosmoglobe DR1 results. I. Improved Wilkinson Microwave Anisotropy Probe maps through Bayesian end-to-end analysis
- BeyondPlanck VI. Noise characterization and modelling
- Concept Design of Low Frequency Telescope for CMB B-mode Polarization satellite LiteBIRD
- How bad could it be? Modelling the 3D complexity of the polarised dust signal using moment expansion
- Overview of the Medium and High Frequency Telescopes of the LiteBIRD satellite mission
- BeyondPlanck IV. On end-to-end simulations in CMB analysis -- Bayesian versus frequentist statistics
- Evaluation of the single-component thermal dust emission model in CMB experiments
- Multi-dimensional optimisation of the scanning strategy for the LiteBIRD space mission