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19952026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2017Show all

556 papers · 1 filter

physics.space-ph2017★ 58 cited

On the statistical properties of turbulent energy transfer rate in the inner Heliosphere

Luca Sorriso-Valvo, Francesco Carbone, Silvia Perri +3

The transfer of energy from large to small scales in solar wind turbulence is an important ingredient of the longstanding question about the mechanism of the interplanetary plasma…

astro-ph.GA2017★ 32 cited

Herschel and SCUBA-2 observations of dust emission in a sample of Planck cold clumps

Mika Juvela, Jinhua He, Katherine Pattle +26

Analysis of all-sky Planck submillimetre observations and the IRAS 100um data has led to the detection of a population of Galactic cold clumps. The clumps can be used to study star…

astro-ph.CO2017★ 41 cited

Galaxy-galaxy weak-lensing measurement from SDSS: II. host halo properties of galaxy groups

Wentao Luo, Xiaohu Yang, Tianhuan Lu +10

As the second paper of a series on studying galaxy-galaxy lensing signals using the Sloan Digital Sky Survey Data Release 7 (SDSS DR7), we present our measurement and modelling of…

astro-ph.GA2017★ 12 cited

Unveiling the inner morphology and gas kinematics of NGC 5135 with ALMA

G. Sabatini, C. Gruppioni, M. Massardi +5

The local Seyfert 2 galaxy NGC5135, thanks to its almost face-on appearance, a bulge overdensity of stars, the presence of a large-scale bar, an AGN and a Supernova Remnant, is an…

astro-ph.SR2017★ 72 cited

Gas and dust from solar metallicity AGB stars

P. Ventura, A. Karakas, F. Dell'Agli +2

We study the asymptotic giant branch (AGB) evolution of stars with masses between . We focus on stars with a solar chemical composition, which allows u…

astro-ph.GA2017★ 28 cited

The VIMOS Public Extragalactic Redshift Survey (VIPERS). AGN feedback in [NeV] emitters

D. Vergani, B. Garilli, M. Polletta +36

Using an unconventional single line diagnostic that unambiguously identifies AGNs in composite galaxies we report statistical differences in the properties (stellar age, [OII] lumi…