Populations behind the source-subtracted cosmic infrared background anisotropies
by Alexander Kashlinsky, R. G. Arendt, M. Ashby, F. Atrio-Barandela, V. Bromm, N. Cappelluti, S. Clesse, A. Comastri, G. Fazio, S. Driver, A. Ferrara, A. Finoguenov, J. Garcia-Bellido, D. Fixsen, G. Hasinger, K. Helgason, R. J. Hill, R. Jansen, J. Kruk, J. Mather, P. Natarajan, N. Odegard, M. Ricotti, M. Sahlen, E. Switzer, R. Windhorst, E. Wollack, and Bin Yue
Published onMay 31, 2019
Populations behind the source-subtracted cosmic infrared background anisotropies
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Abstract
Source-subtracted CIB fluctuations cannot be explained by known galaxy populations and appear highly coherent with unresolved CXB from significantly abundant accreting BHs. Characterizing the CIB with high accuracy, and constraining the nature of the new populations would produce critically important cosmological information in the next decade.
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