A. Moneti
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View article: <i>Planck</i> intermediate results
<i>Planck</i> intermediate results Open
We describe an extension of the most recent version of the Planck Catalogue of Compact Sources (PCCS2), produced using a new multi-band Bayesian Extraction and Estimation Package ( BeeP ). BeeP assumes that the compact sources present in P…
View article: Planck intermediate results. LVI. Detection of the CMB dipole through\n modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II
Planck intermediate results. LVI. Detection of the CMB dipole through\n modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II Open
The largest temperature anisotropy in the cosmic microwave background (CMB)\nis the dipole, which has been measured with increasing accuracy for more than\nthree decades, particularly with the Planck satellite. The simplest\ninterpretation…
View article: <i>Planck</i>2018 results
<i>Planck</i>2018 results Open
The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization in the quest for the curl-like B -mode polarization from primordial gravitational waves and the low-multipole …
View article: <i>Planck</i>intermediate results
<i>Planck</i>intermediate results Open
This paper presents the Planck Multi-frequency Catalogue of Non-thermal (i.e. synchrotron-dominated) Sources (PCNT) observed between 30 and 857 GHz by the ESA Planck mission. This catalogue was constructed by selecting objects detected in …
View article: <i>Planck</i> intermediate results
<i>Planck</i> intermediate results Open
Using the Planck full-mission data, we present a detection of the temperature (and therefore velocity) dispersion due to the kinetic Sunyaev-Zeldovich (kSZ) effect from clusters of galaxies. To suppress the primary CMB and instrumental noi…
View article: Planck intermediate results. LIV. Polarized dust foregrounds
Planck intermediate results. LIV. Polarized dust foregrounds Open
The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization. We use new Planck maps to characterize Galactic dust emission as a foreground to the CMB polarization. We pre…
View article: <i>Planck</i>intermediate results
<i>Planck</i>intermediate results Open
The all-sky Planck survey in 9 frequency bands was used to search for emission from all 274 known Galactic supernova remnants. Of these, 16 were detected in at least two Planck frequencies. The radio-through-microwave spectral energy distr…
View article: Planck intermediate results. XVIII. The millimetre and sub-millimetre emission from planetary nebulae
Planck intermediate results. XVIII. The millimetre and sub-millimetre emission from planetary nebulae Open
Late stages of stellar evolution are characterized by copious mass-loss events whose signature is the formation of circumstellar envelopes (CSE). Planck multi-frequency measurements have provided relevant information on a sample of Galacti…