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most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 40.7k across the 239 of their papers we have counts for

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astro-ph.CO2014★ 66 cited

Pressure distribution of the high-redshift cluster of galaxies CL J1226.9+3332 with NIKA

R. Adam, B. Comis, J. -F. Macías-Pérez +37

The thermal Sunyaev-Zel'dovich (tSZ) effect is expected to provide a low scatter mass proxy for galaxy clusters since it is directly proportional to the cluster thermal energy. The…

astro-ph.CO2014

High resolution SZ observations at the IRAM 30-m telescope with NIKA

R. Adam, A. Adane, P. Ade +36

High resolution observations of the thermal Sunyaev-Zel'dovich (tSZ) effect are necessary to allow the use of clusters of galaxies as a probe for large scale structures at high red…

astro-ph.IM2014★ 2 cited

The NIKA 2012-2014 observing campaigns: control of systematic effects and results

A. Catalano, R. Adam, A. Adane +35

The New IRAM KID Array (NIKA) is a dual-band camera operating with frequency multiplexed arrays of Lumped Element Kinetic Inductance Detectors (LEKIDs) cooled to 100 mK. NIKA is de…

astro-ph.GA2014★ 69 cited

Planck intermediate results. XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust

Planck Collaboration, R. Adam, P. A. R. Ade +199

The role of the magnetic field in the formation of the filamentary structures observed in the interstellar medium (ISM) is a debated topic. The Planck all-sky maps of linearly pola…

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.CO2014★ 222 cited

Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes

Planck Collaboration, R. Adam, P. A. R. Ade +230

The polarized thermal emission from Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background (CMB) at frequencies above 1…