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most citedPlanck 2015 results. XIII. Cosmological parameters

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astro-ph.CO2015★ 18 cited

Planck intermediate results. XLI. A map of lensing-induced B-modes

Planck Collaboration, P. A. R. Ade, N. Aghanim +178

The secondary cosmic microwave background (CMB) -modes stem from the post-decoupling distortion of the polarization -modes due to the gravitational lensing effect of large-sc…

astro-ph.CO2015★ 38 cited

Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster

Planck Collaboration, P. A. R. Ade, N. Aghanim +202

The Virgo cluster is the largest Sunyaev-Zeldovich (SZ) source in the sky, both in terms of angular size and total integrated flux. Planck's wide angular scale and frequency covera…

astro-ph.CO2015★ 9 cited

HI intensity mapping with FAST

Marie-Anne Bigot-Sazy, Yin-Zhe Ma, Richard A. Battye +7

We discuss the detectability of large-scale HI intensity fluctuations using the FAST telescope. We present forecasts for the accuracy of measuring the Baryonic Acoustic Oscillation…

astro-ph.GA2015★ 9 cited

Anomalous Microwave Emission in HII regions: is it really anomalous? The case of RCW 49

Roberta Paladini, Adriano Ingallinera, Claudia Agliozzo +5

The detection of an excess of emission at microwave frequencies with respect to the predicted free-free emission has been reported for several Galactic HII regions. Here, we invest…

astro-ph.CO2015★ 140 cited

Planck 2015 results. XXIII. The thermal Sunyaev-Zeldovich effect--cosmic infrared background correlation

Planck Collaboration, P. A. R. Ade, N. Aghanim +199

We use Planck data to detect the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) effect and the infrared emission from the galaxies that make up the the cosmic infrar…

astro-ph.GA2015★ 26 cited

Planck intermediate results. XXXIX. The Planck list of high-redshift source candidates

Planck Collaboration, P. A. R. Ade, N. Aghanim +186

The Planck mission, thanks to its large frequency range and all-sky coverage, has a unique potential for systematically detecting the brightest, and rarest, submillimetre sources o…