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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. XXIII. Galactic plane emission components derived from Planck with ancillary data

Peter A. R. Ade, +190 more
TL;DR: In this article, the spectral energy distributions (SEDs) at positions along the Galactic plane using the wide frequency coverage of Planck (28.4-857GHz) in combination with low-frequency radio data at 0.408-2.3GHz plus WMAP data at 23-94GHz, along with far-infrared (FIR) data from DIRBE and IRAS.
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Planck intermediate results: XLIII. Spectral energy distribution of dust in clusters of galaxies

R. Adam, +249 more
TL;DR: In this article, the spectral energy distribution (SED) of the infrared spectrum of thermal dust emission in clusters of galaxies was obtained by using a stacking approach for a sample of several hundred objects from the Planck cluster sample; this procedure averaged out fluctuations from the IR sky, allowing to reach a significant detection of the faint cluster contribution.
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Planck intermediate results. XXXIX. The Planck list of high-redshift source candidates

Peter A. R. Ade, +187 more
TL;DR: In this article, a combination of Planck and IRAS data was used to select the most luminous cold submm sources with spectral energy distributions peaking between 353 and 857GHz at 5' resolution.
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Planck intermediate results. XLIII. The spectral energy distribution of dust in clusters of galaxies

R. Adam, +178 more
TL;DR: In this paper, the spectral energy distribution (SED) of the infrared spectrum of thermal dust emission in clusters of galaxies was obtained by using a stacking approach for a sample of several hundred objects from the Planck cluster sample; this procedure averaged out fluctuations from the IR sky, allowing to reach a significant detection of the faint cluster contribution.
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Planck intermediate results. XXV. The Andromeda Galaxy as seen by Planck

Peter A. R. Ade, +203 more
TL;DR: In this paper, the authors examined the morphology of the Andromeda galaxy's outermost spiral arms and investigated the dust heating mechanism across M31, finding that dust dominating the longer wavelength emission is heated by the diffuse stellar population.