Complex diffuse emission in the z = 0.52 cluster PLCK G004.5-19.5

The dust reddening is derived either from the Schlegel maps (as given in the GUViCS catalogue), from the Planck E ( B − V ) map, or from our FUV 1 arcmin or 20 arcsec resolution

When using such accessoriesas "Diopter Correction Lens M,,, "Viewfinder Cap," etc., remove the Eyecup p from the camera... Type: Film: Mount: Exposure

Users’ guides to the medical literature, XXIII: Qualitative research in health care, B: What are the results and how do they help me care for my patients. Evidence-Based

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However, A2142 does not host a cool core, its halo has a size typical of giant radio halos, and the difference in the spectral index of the radio emission in the two components is

Using Westerbork Synthesis Radio Telescope (WSRT) observations we find that the cluster hosts a double radio relic system as well as a 1.65 Mpc radio halo covering the region

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