Corpus ID: 118882620

Populations behind the source-subtracted cosmic infrared background anisotropies

@article{Kashlinsky2019PopulationsBT,
  title={Populations behind the source-subtracted cosmic infrared background anisotropies},
  author={Alexander Kashlinsky and Richard Giles Arendt and Mayor Ashby and Fernando Atrio-Barandela and Volker Bromm and Nico Cappelluti and S'ebastien Clesse and Andrea Comastri and J-G. Cuby and Simon Driver and Giovanni Fazio and Andrea Ferrara and Alexis Finoguenov and Dale J. Fixsen and Juan Garc{\'i}a-Bellido and G. Hasinger and K. Helgason and R Jedd Hill and Ryan Jansen and Jeffrey W. Kruk and Jh Mather and Priyamvada Natarajan and N. P. Odegard and Torsten Reiprich and Massimo Ricotti and Martin Sahl'en and E R Switzer and Rogier Arnold Windhorst and Edward J. Wollack and Bin Yue},
  journal={arXiv: Cosmology and Nongalactic Astrophysics},
  year={2019}
}
  • Alexander Kashlinsky, Richard Giles Arendt, +27 authors Bin Yue
  • Published 2019
  • Physics
  • arXiv: Cosmology and Nongalactic Astrophysics
  • While the upcoming telescopes will reveal correspondingly fainter, more distant galaxies, a question will persist: what more is there that these telescopes cannot see? One answer is the source-subtracted Cosmic Infrared Background (CIB). The CIB is comprised of the collective light from all sources remaining after known, resolved sources are accounted for. Ever-more-sensitive surveys will identify the brightest of these, allowing them to be removed, and - like peeling layers off an onion… CONTINUE READING

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