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L. P. L. Colombo

Researcher at University of Milan

Publications -  308
Citations -  100533

L. P. L. Colombo is an academic researcher from University of Milan. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 121, co-authored 291 publications receiving 90215 citations. Previous affiliations of L. P. L. Colombo include University of Southern California & University of Milano-Bicocca.

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Planck 2013 results. III. LFI systematic uncertainties

P. A. R. Ade, +221 more
TL;DR: In this article, the authors present the current accounting of systematic effect uncertainties for the Low Frequency Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results, showing the robustness and consistency of our data set, especially for polarization analysis.
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Planck intermediate results. L. Evidence for spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB $B$-mode analysis

TL;DR: In this article, the authors make use of the Planck-HFI 2015 data release at high frequencies to place new constraints on the properties of the polarized thermal dust emission at high Galactic latitudes.
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Planck intermediate results - XXXIX. The Planck list of high-redshift source candidates

Peter A. R. Ade, +247 more
TL;DR: In this paper, a combination of Planck and IRAS data was used to select the most luminous cold sub-millimetre sources with spectral energy distributions peaking between 353 and 857 GHz at 5′ resolution.
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Planck 2013 results. IV. Low Frequency Instrument beams and window functions

Nabila Aghanim, +260 more
TL;DR: In this paper, the beam normalization and beam window functions for the Planck Low Frequency Instrument (LFI) were characterized and the uncertainties in the beam window function were analyzed.
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Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants

M. Arnaud, +161 more
TL;DR: The all-sky Planck survey in 9 frequency bands was used to search for emission from all 274 known Galactic supernova remnants as mentioned in this paper, of which 16 were detected in at least two Planck frequencies.