| Autor: |
Bernardis, P., Aquilini, E., Boscaleri, A., Petris, M., Gervasi, M., Martinis, L., Masi, S., Natale, V., Palumbo, P., Scaramuzzi, F. |
| Zdroj: |
Il Nuovo Cimento: C; 1993, Vol. 16 Issue 6, p721-726, 6p |
| Abstrakt: |
We describe a balloon-borne telescope, optimized for observations of the Cosmic Microwave Background (CMB) anisotropies in the mm wavelength region, at angular scales around 1. We stress the scientific motivations for these measurements and the problematics driving the experiment design. Using large throughput bolometers cooled at 0.3K we have a sensitivity high enough to detect CMB anisotropies at level Δ T/ T∼10 in few seconds of integration time. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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