99 citations · 236 across the 8 of their papers we have counts for
8 papers
Planck 2018 results. II. Low Frequency Instrument data processing
Planck Collaboration, Y. Akrami, F. Argüeso +148
We present a final description of the data-processing pipeline for the Planck, Low Frequency Instrument (LFI), implemented for the 2018 data release. Several improvements have been…
Statistics of the fractional polarisation of compact radio sources in Planck maps
Laura Bonavera, Joaquin González-Nuevo, Francisco Argüeso +1
In this work we apply the stacking technique to estimate the average fractional polarisation from 30 to 353 GHz of a primary sample of 1560 compact sources - essentially all radio…
Extragalactic Compact Sources in the Planck Sky and their Cosmological Implications
Luigi Toffolatti, Carlo Burigana, Francisco Argueso +1
The Planck satellite has proved to be a very successful mission, which has been operating flawlessly for more than 36 months. Its main purpose is to map the anisotropies of the CMB…
Tests of Gaussianity
A. M. Aliaga, E. Martinez-Gonzalez, L. Cayon +4
We review two powerful methods to test the Gaussianity of the cosmic microwave background (CMB): one based on the distribution of spherical wavelet coefficients and the other on sm…
Contributions of point extragalactic sources to the Cosmic Microwave Background bispectrum
F. Argüeso, J. González-Nuevo, L. Toffolatti
All the analyses of Cosmic Microwave Background (CMB) temperature maps up--to--date show that CMB anisotropies follow a Gaussian distribution. On the other hand, astrophysical fore…
Goodness-of-Fit Tests to study the Gaussianity of the MAXIMA data
L. Cayon, F. Argueso, E. Martinez-Gonzalez +1
Goodness-of-Fit tests, including Smooth ones, are introduced and applied to detect non-Gaussianity in Cosmic Microwave Background simulations. We study the power of three different…