Publications related to Cosmic neutrino background

This paper presents the Planck 2013 likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations that accounts for all known relevant uncertainties, both instrumental and astrophysical in nature. ...

Edp Sciences S A2014

Search for a diffuse flux of astrophysical muon neutrinos with the IceCube 59-string configuration

Matthias Wolf, Shirit Cohen, Sofia Vallecorsa, Mark Tobin, Mathieu Ribordy, Xiaoxia Bai

A search for high-energy neutrinos was performed using data collected by the IceCube Neutrino Observatory from May 2009 to May 2010, when the array was running in its 59-string configuration. The data sample was optimized to contain muon neutrino induced e ...

Amer Physical Soc2014

Conservative constraints on early cosmology with MONTE PYTHON

Julien Lesgourgues, Benjamin Audren

Models for the latest stages of the cosmological evolution rely on a less solid theoretical and observational ground than the description of earlier stages like BBN and recombination. As suggested in a previous work by Vonlanthen et al., it is possible to ...

Iop Publishing Ltd2013

Sparsity and the Bayesian perspective

Jean-Luc Starck, Anaïs Marie Rassat

Sparsity has recently been introduced in cosmology for weak-lensing and cosmic microwave background (CMB) data analysis for different applications such as denoising, component separation, or inpainting (i.e., filling the missing data or the mask). Although ...

Edp Sciences S A2013

On preferred axes in WMAP cosmic microwave background data after subtraction of the integrated Sachs-Wolfe effect

Jean-Luc Starck, Anaïs Marie Rassat

There is currently a debate over the existence of claimed statistical anomalies in the cosmic microwave background (CMB), recently confirmed in Planck data. Recent work has focussed on methods for measuring statistical significance, on masks and on seconda ...

Edp Sciences S A2013

Low-l CMB analysis and inpainting

Jean-Luc Starck, Anaïs Marie Rassat

Reconstructing the cosmic microwave background (CMB) in the Galactic plane is extremely difficult due to the dominant foreground emissions such as dust, free-free or synchrotron. For cosmological studies, the standard approach consists in masking this area ...

Edp Sciences S A2013

Searches For High-Energy Neutrino Emission In The Galaxy With The Combined Icecube-Amanda Detector

Matthias Wolf, Shirit Cohen, Mathieu Ribordy, Xiaoxia Bai

We report on searches for neutrino sources at energies above 200 GeV in the Northern sky of the Galactic plane, using the data collected by the South Pole neutrino telescope, IceCube, and AMANDA. The Galactic region considered in this work includes the loc ...

Iop Publishing Ltd2013

Removal of two large-scale cosmic microwave background anomalies after subtraction of the integrated Sachs-Wolfe effect

Jean-Luc Starck, Anaïs Marie Rassat

Context. Although there is currently a debate over the significance of the claimed large-scale anomalies in the cosmic microwave background (CMB), their existence is not totally dismissed. In parallel to the debate over their statistical significance, rece ...

Edp Sciences S A2013

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Cosmic neutrino background

CMB power spectra and likelihood

Search for a diffuse flux of astrophysical muon neutrinos with the IceCube 59-string configuration

Conservative constraints on early cosmology with MONTE PYTHON

Sparsity and the Bayesian perspective

On preferred axes in WMAP cosmic microwave background data after subtraction of the integrated Sachs-Wolfe effect

The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths

Graceful exit from Higgs G inflation

Low-l CMB analysis and inpainting

Searches For High-Energy Neutrino Emission In The Galaxy With The Combined Icecube-Amanda Detector

Removal of two large-scale cosmic microwave background anomalies after subtraction of the integrated Sachs-Wolfe effect

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Conservative constraints on early cosmology with MONTE PYTHON

Low-l CMB analysis and inpainting

On preferred axes in WMAP cosmic microwave background data after subtraction of the integrated Sachs-Wolfe effect

Sparsity and the Bayesian perspective

Search for a diffuse flux of astrophysical muon neutrinos with the IceCube 59-string configuration

Removal of two large-scale cosmic microwave background anomalies after subtraction of the integrated Sachs-Wolfe effect

Graceful exit from Higgs G inflation

CMB power spectra and likelihood

Searches For High-Energy Neutrino Emission In The Galaxy With The Combined Icecube-Amanda Detector

The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths