Foreground Contributions to 0.2-2 Degree CMB Anisotropies

Details Foreground Contributions to 0.2-2 Degree CMB Anisotropies Foreground Contributions to 0.2-2 Degree CMB Anisotropies

1994-10-12

arxiv.org/abs/astro-ph/9410037v1

Astrophys.Lett.Commun. 32 (1995) 125

Astronomy and Astrophysics

Astrophysics

invited talk to be published in the Proc. of the Workshop "The cosmic microwave background", Capri (NA), 20-24 September 1993,

Scientific paper

We examine the extent to which galactic and extragalactic foregrounds can hamper the detection of primordial Cosmic Microwave Background (CMB) anisotropies. We limit our discussion to intermediate angular scales, $10^{\prime}\lsim \theta \lsim 2^{\circ}$, since many current as well as future experiments have been designed to map CMB anisotropies at these angular scales. In fact, scales of $\gsim 10^{\prime}$ are of crucial importance to test both the conditions in the early Universe and current theories of the gravitational collapse.

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