Populations behind the source-subtracted cosmic infrared background anisotropies

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. MatherP. Natarajan, N. Odegard, M. Ricotti, M. Sahlen, E. Switzer, R. Windhorst, E. Wollack, Bin Yue

Research output: Contribution to journalArticlepeer-review


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.
Original languageEnglish
Pages (from-to)37
JournalAmerican Astronomical Society. Bulletin
Issue number3
Publication statusPublished - 2019
EventDecadal Survey on Astronomy and Astrophysics : Division on Engineering and Physical Sciences - , United States
Duration: 8 Oct 2019 → …


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