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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.GA2014★ 30 cited

Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants

Planck Collaboration, M. Arnaud, M. Ashdown +160

The all-sky Planck survey in 9 frequency bands was used to search for emission from all 274 known Galactic supernova remnants. Of these, 16 were detected in at least two Planck fre…

astro-ph.GA2014★ 26 cited

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

Planck Collaboration, P. A. R. Ade, N. Aghanim +189

Planck data when combined with ancillary data provide a unique opportunity to separate the diffuse emission components of the inner Galaxy. The purpose of the paper is to elucidate…

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.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…

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…

astro-ph.GA2013★ 221 cited

Planck 2013 results. XIII. Galactic CO emission

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

Rotational transition lines of CO play a major role in molecular radio astronomy and in particular in the study of star formation and the Galactic structure. Although a wealth of d…