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 originale | Anglais |
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Pages (de - à) | 37 |
journal | American Astronomical Society. Bulletin |
Volume | 51 |
Numéro de publication | 3 |
Etat de la publication | Publié - 31 mai 2019 |
Evénement | Decadal Survey on Astronomy and Astrophysics : Division on Engineering and Physical Sciences - , États-Unis Durée: 8 oct. 2019 → … https://sites.nationalacademies.org/DEPS/astro2020/ |