Foreground Contributions to 0.2-2° CMB Anisotropies

Bibcode
1995ApL&C..32..125T
Toffolatti, L.; Danese, L.; Franceschini, A.; Mandolesi, N.; Smoot, G. F.; Bersanelli, M.; Vittorio, N.; Lasenby, A.; Partridge, R. B.; Davies, R.; Sironi, G.; Cesarsky, C.; Lachieze-Rey, M.; Martinez-Gonzalez, E.; Beckman, J.; Rebolo, R.; Sáez, D.; de Bernardis, P.; dall'Oglio, G.; Crane, P.; Janssen, M.; Puget, J. L.; Bussoletti, E.; Raffelt, G.; Encrenaz, P.; Natale, V.; Tofani, G.; Merluzzi, P.; Scaramella, R.; Efstathiou, G.
Referencia bibliográfica

Astrophysical Letters and Communications, Vol. 32, p.125

Fecha de publicación:
0
1995
Revista
Astrophysical Letters and Communications
Número de autores
30
Número de autores del IAC
1
Número de citas
13
Número de citas referidas
11
Descripción
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'< theta < 2 deg, since many current as well as future experiments have been designed to map CMB anisotropies at these angular scales. In fact, scales of > 10' are of crucial importance to test both the conditions in the early Universe and current theories of the gravitational collapse.
Tipo
Con árbitro
Radiación cósmica de fondo

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