Sessions |
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Keynotes |
Invited |
Contributed |
Keynotes |
statistical methods PoS(Big3)001 |
future of the supercomputing PoS(Big3)002 |
Cosmic Microwave Background PoS(Big3)003 |
Invited |
From mean Euler characteristics to the Gaussian kinematic formula PoS(Big3)004 |
Shrinking the quadratic estimator PoS(Big3)005 |
Compressed sensing in astrophysics and beyond PoS(Big3)006 |
High level programming languages and hybrid programming in the context of high performance scientific applications PoS(Big3)007 |
Secondary CMB anisotropies and their simulations PoS(Big3)008 |
Component separation techniques for CMB maps PoS(Big3)009 |
CMB power spectrum estimation techniques PoS(Big3)010 |
sampling algorithms, Markov and non-Markov chains PoS(Big3)011 |
Making maps for CMB experiments PoS(Big3)012 pdf |
needlets/wavelets nonGaussianity estimators PoS(Big3)013 |
Hunting for relics from the early universe in the CMB PoS(Big3)014 |
Discrete Aspects of High-Performance Iterative Linear Solvers PoS(Big3)015 |
non-Gaussianity tests PoS(Big3)016 pdf |
on recent developments in numerical linear algebra PoS(Big3)037 |
Contributed |
Sparse component separation for accurate CMB map estimation PoS(Big3)017 |
CMB lensing reconstruction in the presence of diffuse polarized foregrounds PoS(Big3)018 pdf |
A robust constraint on cosmic textures from the cosmic microwave background PoS(Big3)019 |
Deriving bounds for trispectrum estimators for Planck PoS(Big3)020 |
Power spectrum estimation on the sphere using wavelets PoS(Big3)021 pdf |
Nets and nests: accelerated Bayesian inference in astrophysics PoS(Big3)022 |
Restoration of a whole-sky CMB map PoS(Big3)023 pdf |
Searching for the Unexpected PoS(Big3)024 |
Simple foreground cleaning algorithm for detecting primordial B-mode polarization of the cosmic microwave background PoS(Big3)025 |
Spherical wavelet-Bayesian cosmic string tension estimation PoS(Big3)026 |
Methodology and lessons from the QUIET Maximum Likelihood map-maker PoS(Big3)027 |
True CMB Power Spectrum Estimation PoS(Big3)028 |
Removal of two large scale Cosmic Microwave Background anomalies after subtraction of the Integrated Sachs Wolfe effect PoS(Big3)029 |
Reconstruction of high-resolution SZ maps from heterogeneous datasets using needlets PoS(Big3)030 pdf |
Primordial non-Gaussianity and diffuse Galactic emissions PoS(Big3)031 pdf |
Detection of Point Sources Using Internal Templates and Needlets PoS(Big3)032 |
Avoiding Communication in Generalized Least Square Problems PoS(Big3)033 |
Accelerating convolutions on the sphere with hybid GPU/CPU kernel splitting PoS(Big3)034 pdf |
Component Separation for Full-Sky Cosmic Microwave Background Recovery using Sparsity PoS(Big3)035 |
Accelerating maximum likelihood Cosmic Microwave Background map-making PoS(Big3)036 |