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

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Résumé

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.
langue originaleAnglais
Pages (de - à)37
journalAmerican Astronomical Society. Bulletin
Volume51
Numéro de publication3
Etat de la publicationPublié - 2019
EvénementDecadal Survey on Astronomy and Astrophysics : Division on Engineering and Physical Sciences - , États-Unis
Durée: 8 oct. 2019 → …
https://sites.nationalacademies.org/DEPS/astro2020/

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