MG13 - Talk detail |
|
Participant |
Viero, Marco Viero | |||||||
|
Institution |
California Institute of Technology - 1200 E. California Blvd. - United States - CA - USA | |||||||
|
Session |
CB2 |
Accepted |
No |
Order |
4 |
Time |
||
|
Talk |
Oral abstract |
Title |
The Imprint of Correlated Dusty Star-Forming Galaxies on the Cosmic Infrared Background | |||||
| Co-authors | Lingyu Wang, Michael Zemcov, and the HeRMES Collaboration | |||||||
|
Abstract |
Imprinted on the Cosmic Infrared Background (CIB) is the clustering pattern of dusty star-forming galaxies spanning all of cosmic time. By measuring this pattern, we can trace the redshift-dependent relationship of star formation to dark matter, and uncover the environments in which star formation is most efficient. This measurement has been shown to have wide applications, from constraining phenomenological models of infrared galaxy populations, to characterizing correlations of the CMB with foreground emission. Here we present recent results of the CIB clustering measurement at 250, 350, and 500 μm (1200, 860, and 1200 GHz) from the Herschel Multi-tiered Extragalactic Survey (HeRMES), and discuss implications for galaxy formation models and CMB measurements. |
|||||||