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20112026
most citedPlanck 2013 results. XI. All-sky model of thermal dust emission

827 citations · 3.5k across the 36 of their papers we have counts for

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Showing 2014Show all

8 papers · 1 filter

astro-ph.GA2014★ 446 cited

The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point

A. P. Jones, L. Fanciullo, M. Koehler +4

Context. The evolution of amorphous hydrocarbon materials, a-C(:H), principally resulting from ultraviolet (UV) photon absorption- induced processing, are likely at the heart of th…

astro-ph.GA2014★ 54 cited

The cycling of carbon into and out of dust

Anthony P. Jones, Nathalie Ysard, Melanie Koehler +5

Observational evidence seems to indicate that the depletion of interstellar carbon into dust shows rather wide variations and that carbon undergoes rather rapid recycling in the in…

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.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…

astro-ph.GA2014★ 42 cited

Shocks in dense clouds. IV. Effects of grain-grain processing on molecular line emission

S. Anderl, V. Guillet, G. Pineau des Forêts +1

Grain-grain processing has been shown to be an indispensable ingredient of shock modelling in high density environments. For densities higher than \sim10^5 cm-3, shattering becomes…

astro-ph.IM2014

Polarization measurements analysis II. Best estimators of polarization fraction and angle

L. Montier, S. Plaszczynski, F. Levrier +5

With the forthcoming release of high precision polarization measurements, such as from the Planck satellite, it becomes critical to evaluate the performance of estimators for the p…

astro-ph.GA2014★ 190 cited

Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization

Planck Collaboration, P. A. R. Ade, M. I. R. Alves +177

Planck has mapped the intensity and polarization of the sky at microwave frequencies with unprecedented sensitivity. We make use of the Planck 353 GHz I, Q, and U Stokes maps as du…

astro-ph.GA2014★ 101 cited

Planck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible

Planck Collaboration, P. A. R. Ade, N. Aghanim +192

The Planck survey provides unprecedented full-sky coverage of the submillimetre polarized emission from Galactic dust, bringing new constraints on the properties of dust. The dust…