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20052018
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 42.1k across the 114 of their papers we have counts for

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astro-ph.IM2015★ 96 cited

Planck 2015 results. V. LFI calibration

Planck Collaboration, P. A. R. Ade, N. Aghanim +206

We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, cov…

astro-ph.IM2015★ 74 cited

Planck 2015 results. VII. HFI TOI and beam processing

Planck Collaboration, R. Adam, P. A. R. Ade +225

The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polari…

astro-ph.IM2015★ 62 cited

Planck 2015 results. II. Low Frequency Instrument data processing

Planck Collaboration, P. A. R. Ade, N. Aghanim +213

We present an updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline, associated with the 2015 data release. We point out the places where our re…

astro-ph.IM2013★ 188 cited

Planck 2013 results. IX. HFI spectral response

Planck Collaboration, P. A. R. Ade, N. Aghanim +217

The Planck High Frequency Instrument (HFI) spectral response was determined through a series of ground based tests conducted with the HFI focal plane in a cryogenic environment pri…

astro-ph.IM2013★ 111 cited

Planck 2013 results. VII. HFI time response and beams

Planck Collaboration, P. A. R. Ade, N. Aghanim +220

This paper characterizes the effective beams,the effective beam window functions and the associated errors for the Planck HFI detectors. The effective beam is the angular response…

astro-ph.IM2013★ 78 cited

Planck 2013 results. V. LFI calibration

Planck Collaboration, N. Aghanim, C. Armitage-Caplan +217

We discuss the methods employed to photometrically calibrate the data acquired by the Low Frequency Instrument on Planck. Our calibration is based on a combination of the Orbital D…

astro-ph.IM2012★ 23 cited

A coherent polarimeter array for the Large Scale Polarization Explorer balloon experiment

M. Bersanelli, A. Mennella, G. Morgante +43

We discuss the design and expected performance of STRIP (STRatospheric Italian Polarimeter), an array of coherent receivers designed to fly on board the LSPE (Large Scale Polarizat…

astro-ph.IM2011★ 88 cited

Planck Early Results. V. The Low Frequency Instrument data processing

A. Zacchei, D. Maino, C. Baccigalupi +146

We describe the processing of data from the Low Frequency Instrument (LFI) used in production of the Planck Early Release Compact Source Catalogue (ERCSC). In particular, we discus…

astro-ph.IM2011★ 143 cited

Planck Early Results. II. The thermal performance of Planck

Planck Collaboration, P. A. R. Ade, N. Aghanim +225

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…

astro-ph.IM2011★ 525 cited

Planck Early Results: The Planck mission

Planck Collaboration, P. A. R. Ade, N. Aghanim +272

The European Space Agency's Planck satellite was launched on 14 May 2009, and has been surveying the sky stably and continuously since 13 August 2009. Its performance is well in li…