activity
20062026
most citedThe non-Gaussian Cold Spot in the 3-year WMAP data

220 citations · 976 across the 12 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

6 papers · 1 filter

astro-ph.CO2026

Validation of harmonic-space likelihood methods for LiteBIRD B-mode polarisation analysis

G. Galloni, P. Campeti, C. Gimeno-Amo +112

The LiteBIRD satellite mission aims to measure the tensor-to-scalar ratio with unprecedented sensitivity through observations of the cosmic microwave background (CMB) -mode…

astro-ph.CO2013★ 6 cited

Using CMB polarization to constrain the anomalous nature of the Cold Spot with an incomplete sky-coverage

R. Fernández-Cobos, P. Vielva, E. Martínez-González +2

Recent results of the ESA Planck satellite have confirmed the existence of some anomalies in the statistical distribution of the cosmic microwave background (CMB) anisotropies. One…

astro-ph.CO2011★ 136 cited

Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance

A. Mennella, M. Bersanelli, R. C. Butler +158

The scientific performance of the Planck Low Frequency Instrument (LFI) after one year of in-orbit operation is presented. We describe the main optical parameters and discuss photo…

astro-ph.CO2010★ 43 cited

Anomalous variance in the WMAP data and Galactic Foreground residuals

M. Cruz, P. Vielva, E. Martínez-González +1

A previous work (Monteserín et al. 2008) estimated the CMB variance from the three-year WMAP data, finding a lower value than expected from Gaussian simulations using the WMAP best…

astro-ph.CO2009★ 17 cited

WMAP anomalous signal in the ecliptic plane

J. M Diego, M. Cruz, J. Gonzalez-Nuevo +3

We report the detection of a high Galactic latitude, large scale, 7-sigma signal in WMAP 5yr and spatially correlated with the ecliptic plane. Two possible candidates are studied,…

astro-ph.CO2009★ 6 cited

The WMAP cold spot

M. Cruz, E. Martinez-Gonzalez, P. Vielva

The WMAP cold spot was found by applying spherical wavelets to the first year WMAP data. An excess of kurtosis of the wavelet coefficient was observed at angular scales of around 5…