DocumentCode
124909
Title
Detecting the peak of the cosmological 21 cm signal
Author
Mesinger, Andrei ; Ewall-Wice, A.
Author_Institution
Scuola Normale Superiore, Pisa, Italy
fYear
2014
fDate
8-11 Jan. 2014
Firstpage
1
Lastpage
1
Abstract
21 cm tomography promises to shed light on the formation of the first stars, galaxies, and black holes in the coming years. A number of radio interferometers are already taking data in an effort to detect the diffuse HI signal during the epoch of reionization using statistical measures such as the power spectrum.
Keywords
H I regions; black holes; cosmology; galaxies; interferometers; H I signal; black holes; cosmological signal; epoch-of-reionization; galaxies; power spectrum; radio interferometers; size 21 cm; tomography; Aerospace electronics; Arrays; Interferometers; Sensitivity; Space heating; Temperature measurement;
fLanguage
English
Publisher
ieee
Conference_Titel
Radio Science Meeting (USNC-URSI NRSM), 2014 United States National Committee of URSI National
Conference_Location
Boulder, CO
Print_ISBN
978-1-4799-3119-4
Type
conf
DOI
10.1109/USNC-URSI-NRSM.2014.6928126
Filename
6928126
Link To Document