Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation

In this work we present a new method for probing the star formation history of the Universe, namely tomographic cross-correlation between the cosmic infrared background (CIB) and galaxy samples. The galaxy samples are from the Kilo-Degree Survey (KiDS), while the CIB maps are made from Planck sky ma...

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Bibliographic Details
Published in:Astronomy and astrophysics (Berlin) 2022-09, Vol.665, p.A52
Main Authors: Yan, Ziang, van Waerbeke, Ludovic, Wright, Angus H., Bilicki, Maciej, Gu, Shiming, Hildebrandt, Hendrik, Maniyar, Abhishek S., Tröster, Tilman
Format: Article
Language:English
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Summary:In this work we present a new method for probing the star formation history of the Universe, namely tomographic cross-correlation between the cosmic infrared background (CIB) and galaxy samples. The galaxy samples are from the Kilo-Degree Survey (KiDS), while the CIB maps are made from Planck sky maps at 353, 545, and 857 GHz. We measure the cross-correlation in harmonic space within 100 
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/202243710