31 datasets found

Reproduced with permission. Copyright ESO.

International audience

The search of a clustering signal in the arrival directions of ultra-high-energy cosmic rays (UHECRs) is a standard method to assess the level of anisotropy of the...

We present the results of searches for high-energy muon neutrinos from 41 gamma-ray bursts (GRBs) in the northern sky with the IceCube detector in its 22 string...

The Wilkinson Microwave Anisotropy Probe (WMAP) satellite has provided high-resolution, high signal-to-noise ratio maps of the sky in five main frequency bands ranging...

The 'Internal Linear Combination' (ILC) component separation method has been extensively used to extract a single component, the cosmic microwave background (CMB),...

We present a model-independent investigation of the Wilkinson Microwave Anisotropy Probe (WMAP) data with respect to scale-independent and scale-dependent...

The 'Internal Linear Combination' (ILC) component separation method has been extensively used on the data of the Wilkinson Microwave Anisotropy Probe (WMAP) space...

We estimate cosmic microwave background (CMB) polarization and temperature power spectra using Wilkinson Microwave Anisotropy Probe (WMAP) 5 year foreground...

Context: The WMAP satellite has made available high quality maps of the sky in five frequency bands ranging from 22 to 94 GHz, with the main scientific objective of...

9 pages, 6 figures

Received: 22 March 2013 / Accepted: 01 March 2014

Received: 22 March 2013 / Accepted: 06 January 2014

25 pages, 18 figures, 12 tables, 1 appendix ; Received: 21 March 2013 / Accepted: 22 August 2014

Received: 26 March 2013 / Accepted: 01 July 2014

Submitted to Astronomy and Astrophysics. 25 pages, 25 figures, 14 tables. high resolution version available from the ESA website :...

Received: 21 March 2013 / Accepted: 16 March 2014

56 pages; LaTeX; 42 figures

23 Pages, 23 Figures ; Received: 22 March 2013 / Accepted: 23 February 2014

International audience