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arXiv · astro-ph/9410037

Foreground Contributions to 0.2-2 Degree CMB Anisotropies

L. Toffolatti
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Abstract

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, $10^{\prime}\lsim θ\lsim 2^{\circ}$, 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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L. Toffolatti. 1994-10-12. Foreground Contributions to 0.2-2 Degree CMB Anisotropies. https://arxiv.org/abs/astro-ph/9410037

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