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I. D. Novikov

Researcher at Russian Academy of Sciences

Publications -  263
Citations -  83503

I. D. Novikov is an academic researcher from Russian Academy of Sciences. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 119, co-authored 260 publications receiving 78911 citations. Previous affiliations of I. D. Novikov include University of Copenhagen & Niels Bohr Institute.

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Planck intermediate results - XXVIII. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck

Peter A. R. Ade, +225 more
TL;DR: In this paper, the authors compare the dust and cosmic rays in the Chamaeleon clouds with the results obtained from the Fermi Large Area Telescope (LAT) and IRAS, and provide average values for the dust properties per gas nucleon in different phases.
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Planck intermediate results - XIII. Constraints on peculiar velocities

Peter A. R. Ade, +228 more
TL;DR: In this article, the authors used Planck data combined with the Meta Catalogue of X-ray detected Clusters of galaxies (MCXC) to address the study of peculiar motions by searching for evidence of the kinetic Sunyaev-Zeldovich effect (kSZ).
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Planck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible

Peter A. R. Ade, +193 more
TL;DR: In this article, the authors measured the sub-millimetre polarized intensity and the optical depth in the V band to the star in the Planck 353 GHz channel, and derived the degree of polarization and optical depth.
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Planck Early Results: The Planck View of Nearby Galaxies

P. A. R. Ade, +193 more
TL;DR: In this paper, the spectral energy distributions (SEDs) of distant submm galaxies are measured using parametric dust models to determine the range of dust temperatures and emissivities.
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Planck Early Results. II. The thermal performance of Planck

Peter A. R. Ade, +226 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.