Showing 1–20 of 25 results
/ Date/ Name
Nov 11, 2025Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distributionOct 20, 2025Euclid preparation: The flat-sky approximation for the clustering of Euclid's photometric galaxiesOct 10, 2025Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and ForecastsJul 30, 2025LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD dataJul 8, 2025First release of LiteBIRD simulations from an end-to-end pipelineJul 7, 2025A Simulation Framework for the LiteBIRD InstrumentsJun 27, 2025Requirements on bandpass resolution and measurement precision for LiteBIRDJun 10, 2025Euclid preparation: The NISP spectroscopy channel, on ground performance and calibrationMay 7, 2025Euclid preparation. The impact of redshift interlopers on the two-point correlation function analysisMar 19, 2025Euclid Quick Data Release (Q1), A first look at the fraction of bars in massive galaxies at $z<1$Mar 19, 2025Euclid Quick Data Release (Q1): First visual morphology catalogueNov 4, 2024Requirements on the gain calibration for LiteBIRD polarisation data with blind component separationAug 6, 2024Multi-dimensional optimisation of the scanning strategy for the LiteBIRD space missionJul 24, 2024LiteBIRD Science Goals and Forecasts. Mapping the Hot Gas in the UniverseJun 4, 2024The LiteBIRD mission to explore cosmic inflationMar 25, 2024LiteBIRD Science Goals and Forecasts: Primordial Magnetic FieldsDec 14, 2023Impact of beam far side-lobe knowledge in the presence of foregrounds for LiteBIRDDec 8, 2023LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer DelensingDec 8, 2023LiteBIRD Science Goals and Forecasts: A full-sky measurement of gravitational lensing of the CMBDec 1, 2023LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization