activity
20002017
most citedPlanck 2013 results. XV. CMB power spectra and likelihood

577 citations · 1.2k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2017★ 28 cited

Recovering galaxy cluster gas density profiles with XMM-Newton and Chandra

I. Bartalucci, M. Arnaud, G. W. Pratt +6

We examine the reconstruction of galaxy cluster radial density profiles obtained from Chandra and XMM X-ray observations, using high quality data for a sample of twelve objects cov…

astro-ph.HE2014★ 38 cited

Planck intermediate results. XXVIII. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck

Planck, Fermi Collaborations, : +197

Shortened abstract: Observations of the nearby Chamaeleon clouds in gamma rays with the Fermi Large Area Telescope and in thermal dust emission with Planck and IRAS have been used…

astro-ph.CO2013★ 577 cited

Planck 2013 results. XV. CMB power spectra and likelihood

Planck collaboration, P. A. R. Ade, N. Aghanim +257

We present the Planck likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations. We use this likelihood to derive the…

astro-ph2000★ 60 cited

A Mosaic of the Coma Cluster of Galaxies with XMM-Newton

Ulrich G. Briel, J. Patrick Henry, David H. Lumb +7

The Coma cluster of galaxies was observed with XMM-Newton in 12 partially overlapping pointings. We present here the resulting X-ray map in different energy bands and discuss the l…

astro-ph2000★ 374 cited

XMM-Newton observation of the Lockman Hole; I. The X-ray Data

G. Hasinger, B. Altieri, M. Arnaud +25

We report on the first deep X-ray survey with the XMM-Newton observatory during the performance verification phase. The field of the Lockman Hole, one of the best studied sky areas…

astro-ph2000★ 117 cited

Temperature and Heavy Element Abundance Profiles of Cool Clusters of Galaxies from ASCA

A. Finoguenov, M. Arnaud, L. P. David

We perform a spatially resolved X-ray spectroscopic study of a set of 18 relaxed clusters of galaxies with gas temperatures below 4 keV. Spectral analysis was done using ASCA/SIS d…