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High Latitude Galactic Emission and the Search for Anisotropies in the CBR

Published online by Cambridge University Press:  08 February 2017

S. Masi
Affiliation:
Dipartimento di Fisica Università di Roma, Italy
P. Calisse
Affiliation:
Dipartimento di Fisica Università di Roma, Italy
P. de Bernardis
Affiliation:
Dipartimento di Fisica Università di Roma, Italy
M. De Petris
Affiliation:
Dipartimento di Fisica Università di Roma, Italy
M. Epifani
Affiliation:
Dipartimento di Fisica Università di Roma, Italy
M. Gervasi
Affiliation:
Dipartimento di Fisica Università di Roma, Italy
G. Guarini
Affiliation:
Dipartimento di Fisica Università di Roma, Italy
F. Melchiorri
Affiliation:
Dipartimento di Fisica Università di Roma, Italy
G. Moreno
Affiliation:
Dipartimento di Fisica Università di Roma, Italy
P. Temi
Affiliation:
Dipartimento di Fisica Università di Roma, Italy

Extract

The study of the anisotropies of the submillimeter relict radiation (RR) can provide important arguments to select among different theoretical scenarios (Panek and Rudak 1988). However, interstellar dust (ISD) emission is present in this spectral region and its patchy distribution can heavily contaminate anisotropy measurements. For example, the most sensitive measurement of CBR anisotropies has been reported so far in a broad band around 1 mm (Melchiorri et al. 1981): the detection of anisotropy is statistically very significant, but its cosmological origin is questionable.

Type
IV. Extragalactic Background Radiation and Cosmology
Copyright
Copyright © Kluwer 1990 

References

de Bernardis, P. et al 1988, Ap. J., 326, 941.CrossRefGoogle Scholar
Halpern, M. et al 1988, Ap. J., 332, 596.CrossRefGoogle Scholar
Matsumoto, T. et al. 1988, Ap. J., 329, 567.CrossRefGoogle Scholar
Melchiorri, F. et al. 1981, Ap. J. (Letters), 250, L1.CrossRefGoogle Scholar
Panek, M. and Rudak, B. 1988, MNRAS, 235, 1169.CrossRefGoogle Scholar

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