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S. Galeotta

Researcher at INAF

Publications -  411
Citations -  113794

S. Galeotta is an academic researcher from INAF. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 140, co-authored 377 publications receiving 101132 citations. Previous affiliations of S. Galeotta include Trieste Astronomical Observatory & ASTRON.

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Planck early results. II. The thermal performance of Planck

Peter A. R. Ade, +249 more
TL;DR: In this paper, the performance of the Planck instruments in space is enabled by their low operating temperatures, 20K for LFI and 0.1K for HFI, achieved through a combination of passive radiative cooling and three active mechanical coolers.
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Planck Early Results: Statistical properties of extragalactic radio sources in the Planck Early Release Compact Source Catalogue

P. A. R. Ade, +201 more
TL;DR: The data reported in Planck's Early Release Compact Source Catalogue (ERCSC) are exploited to measure the number counts (dN/dS) of extragalactic radio sources at 30, 44, 70, 100, 143 and 217 GHz as mentioned in this paper.
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Planck 2015 results - VII. High Frequency Instrument data processing: Time-ordered information and beams

R. Adam, +239 more
TL;DR: The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polarization as mentioned in this paper.
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Planck intermediate results: XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect

Peter A. R. Ade, +247 more
TL;DR: In this article, the authors estimate the pairwise momentum of the kSZ temperature fluctuations at the positions of the Central Galaxy Catalogu e (CGC) samples extracted from Sloan Digital Sky Survey (SDSS-DR7) data.
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Planck intermediate results. XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect

Peter A. R. Ade, +190 more
TL;DR: In this paper, the kinetic Sunyaev-Zeldovich effect (kSZ) in Planck nominal mission data was used to detect baryons participating in large-scale bulk flows around central galaxies.