Showing 1–20 of 43 results
/ Date/ Name
Jul 7, 2017Separating CMB Stokes Q and U polarization signals from Non-Gaussian EmissionsApr 28, 2024Accurate and Unbiased Reconstruction of CMB B Mode using Deep LearningFeb 8, 2021An Unbiased Estimator of the Full-sky CMB Angular Power Spectrum at Large Scales using Neural NetworksFeb 12, 2021Application of Genetic Algorithm to Estimate the Large Angular Scale Features of Cosmic Microwave BackgroundDec 11, 2016An Improved Diffuse Foreground Subtraction by ILC method: CMB Map and Angular Power Spectrum using Planck and WMAP ObservationsSep 11, 2015A Perturbative Analysis of Synchrotron Spectral Index Variation over Microwave SkyJun 2, 2025Immunometabolism at the Crossroads of Infection: Mechanistic and Systems-Level Perspectives from Host and PathogenMar 30, 2020An Accurate Reconstruction of CMB E Mode Signal over Large Angular Scales using Prior Information of CMB Covariance Matrix in ILC AlgorithmDec 28, 2017A Global ILC Approach in Pixel Space over Large Angular Scales of the Sky using CMB Covariance MatrixNov 16, 2022Reconstruction of full sky CMB $\bf{E}$ and $\bf{B}$ modes spectra removing $\bf{E}$-to-$\bf{B}$ leakage from partial sky using deep learningOct 21, 2018An Application of Global ILC Algorithm over Large Angular Scales to Estimate CMB Posterior Using Gibbs SamplingDec 27, 2025A Generative Reconstruction of Low-$\ell$ CMB B-Mode Signal using Reverse Diffusion in Deep LearningMay 31, 2011A Foreground Cleaned CMB Map from Non-Gaussianity MeasurementDec 14, 2019Exact Solutions and Constraints on the Dark Energy Model in FRW UniverseJan 12, 2009Model Independent Foreground Power Spectrum Estimation using WMAP 5-year DataApr 14, 2022On Direct Estimation of Density Parameters and Hubble Constant for $Λ$CDM Universe using Hubble MeasurementsMay 5, 2024Foreground removal and angular power spectrum estimation of 21 cm signal using harmonic space ILC methodApr 18, 2020A Foreground Model Independent Estimation of Joint Posterior of CMB E mode Polarization over Large Angular ScalesOct 15, 2021A Partial-Sky Gibbs ILC Approach for the Estimation of CMB Posterior over Large Angular Scales of the SkySep 15, 2022Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions