Sessions |
---|
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 |