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20072023
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 15.4k across the 73 of their papers we have counts for

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astro-ph.GA2013★ 827 cited

Planck 2013 results. XI. All-sky model of thermal dust emission

Planck Collaboration, A. Abergel, P. A. R. Ade +244

This paper presents an all-sky model of dust emission from the Planck 857, 545 and 353 GHz, and IRAS 100 micron data. Using a modified black-body fit to the data we present all-sky…

astro-ph.CO2013★ 305 cited

Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation

Planck Collaboration, P. A. R. Ade, N. Aghanim +238

We present new measurements of CIB anisotropies using Planck. Combining HFI data with IRAS, the angular auto- and cross frequency power spectrum is measured from 143 to 3000 GHz, a…

astro-ph.GA2013★ 5 cited

Planck intermediate results. XV. A study of anomalous microwave emission in Galactic clouds

Planck Collaboration, P. A. R. Ade, N. Aghanim +180

Anomalous microwave emission (AME) is believed to be due to electric dipole radiation from small spinning dust grains. The aim of this paper is a statistical study of the basic pro…

stat.ML2013★ 35 cited

Sparse and Non-Negative BSS for Noisy Data

Jérémy Rapin, Jérôme Bobin, Anthony Larue +1

Non-negative blind source separation (BSS) has raised interest in various fields of research, as testified by the wide literature on the topic of non-negative matrix factorization…

cs.IT2013

Hyperspectral fluorescence microscopy based on Compressive Sampling

Makhlad Chahid, Jerome Bobin, Hamed Shams Mousavi +3

The mathematical theory of compressed sensing (CS) asserts that one can acquire signals from measurements whose rate is much lower than the total bandwidth. Whereas the CS theory i…

astro-ph.GA2013★ 80 cited

Planck intermediate results. XIV. Dust emission at millimetre wavelengths in the Galactic plane

Planck Collaboration, P. A. R. Ade, N. Aghanim +190

We use Planck HFI data combined with ancillary radio data to study the emissivity index of the interstellar dust emission in the frequency range 10 - 353 GHz, or 3 - 0.8 mm, in the…