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19982026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 31.1k across the 367 of their papers we have counts for

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Showing 2012Show all

9 papers · 1 filter

astro-ph.IM2012★ 43 cited

LOFT: the Large Observatory For X-ray Timing

M. Feroci, J. W. den Herder, E. Bozzo +245

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is curren…

astro-ph.GA2012★ 70 cited

Planck Intermediate Results. IX. Detection of the Galactic haze with Planck

Planck Collaboration, P. A. R. Ade, N. Aghanim +181

Using precise full-sky observations from Planck, and applying several methods of component separation, we identify and characterize the emission from the Galactic "haze" at microwa…

astro-ph.IM2012★ 4 cited

Breadboard model of the LISA phasemeter

Oliver Gerberding, Simon Barke, Ioury Bykov +14

An elegant breadboard model of the LISA phasemeter is currently under development by a Danish-German consortium. The breadboard is build in the frame of an ESA technology developme…

astro-ph.CO2012★ 69 cited

Planck intermediate results. X. Physics of the hot gas in the Coma cluster

Planck Collaboration, P. A. R. Ade, N. Aghanim +207

We present an analysis of Planck satellite data on the Coma Cluster observed via the Sunyaev-Zeldovich effect. Planck is able, for the first time, to detect SZ emission up to r ~ 3…

astro-ph.SR2012★ 22 cited

Microlensig Binaries with Candidate Brown Dwarf Companions

I. -G. Shin, C. Han, A. Gould +152

Brown dwarfs are important objects because they may provide a missing link between stars and planets, two populations that have dramatically different formation history. In this pa…

astro-ph.CO2012★ 26 cited

Planck Intermediate Results. IV. The XMM-Newton validation programme for new Planck galaxy clusters

Planck Collaboration, P. A. R. Ade, N. Aghanim +191

We present the final results from the XMM-Newton validation follow-up of new Planck galaxy cluster candidates. We observed 15 new candidates, detected with signal-to-noise ratios b…