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Proto-cluster candidates

Proto-cluster candidates

Date: 31 March 2015
Satellite: Planck and Herschel
Copyright: ESA and the Planck Collaboration/ H. Dole, D. Guéry & G. Hurier, IAS/University Paris-Sud/CNRS/CNES

The Planck all-sky map at submillimetre wavelengths (545 GHz). The band running through the middle corresponds to dust in our Milky Way galaxy. The black dots indicate the location of the proto-cluster candidates identified by Planck and subsequently observed by Herschel. The inset images showcase some of the observations made by Herschel's SPIRE instrument; the contours represent the density of galaxies.

Last Update: 1 September 2019
20-Jun-2024 16:25 UT

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