D. L. Harrison

TL;DR: In this article, the authors present an analysis of Planck satellite data on the Coma Cluster observed via the Sunyaev-Zeldovich effect, and they find that the Arnaud et al. universal pressure profile does not fit Coma, and that their pressure profile for merging systems provides a good fit of the data only at r R_500 than the mean pressure profile predicted by the simulations.

TL;DR: In this paper, the authors used WMAP and Planck maps, combined with ancillary radio and IR data, to construct a sample of 98 candidate AME sources, assembling SEDs for each source using aperture photometry on 1deg-smoothed maps from 0.408 GHz up to 3000 GHz.

TL;DR: In this paper, the authors performed observations at 37 GHz for a sample of 78 radio-loud and radio-quiet narrow-line Seyfert 1 (NLS1) galaxies, together with additional lower and higher frequency radio data from RATAN-600, Owens Valley Radio Observatory, and the Planck satellite.

TL;DR: In this article, the authors evaluate the construction methodology of an all-sky catalogue of galaxy clusters detected through the Sunyaev-Zel'dovich (SZ) effect, and provide a comparison of a representative sample of SZ detection algorithms and highlight important issues in their application.

TL;DR: In this paper, the spectral energy distributions (SEDs) of a sample of Galactic planetary nebulae (PNe) in the important and relatively unexplored observational band between 30 and 857GHz were derived.