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19992022
most citedPlanck 2013 results. XXII. Constraints on inflation

1.1k citations · 4.3k across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.GA2022★ 36 cited

A new look at local ultraluminous infrared galaxies: the atlas and radiative transfer models of their complex physics

A. Efstathiou, D. Farrah, J. Afonso +11

We present the ultraviolet to submillimetre spectral energy distributions (SEDs) of the HERschel Ultra Luminous Infrared Galaxy Survey (HERUS) sample of 42 local ultraluminous infr…

astro-ph.GA2019★ 39 cited

A LOFAR-IRAS cross-match study: the far-infrared radio correlation and the 150-MHz luminosity as a star-formation rate

L. Wang, F. Gao, K. J. Duncan +15

Aims. We aim to study the far-infrared radio correlation (FIRC) at 150 MHz in the local Universe (at a median redshift z~0:05) and improve the use of the rest-frame 150-MHz luminos…

astro-ph.CO2015★ 146 cited

Planck 2015 results. XXVI. The Second Planck Catalogue of Compact Sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +240

The Second Planck Catalogue of Compact Sources is a catalogue of sources detected in single-frequency maps from the full duration of the Planck mission and supersedes previous vers…

astro-ph.CO2015★ 10 cited

Planck 2015 results. XX. Constraints on inflation

Planck Collaboration, P. A. R. Ade, N. Aghanim +244

We present the implications for cosmic inflation of the Planck measurements of the cosmic microwave background (CMB) anisotropies in both temperature and polarization based on the…

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.CO2013★ 293 cited

Planck 2013 results. XII. Component separation

Planck Collaboration, P. A. R. Ade, N. Aghanim +252

Planck has produced detailed all-sky observations over nine frequency bands between 30 and 857 GHz. These observations allow robust reconstruction of the primordial cosmic microwav…