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1.
Measurement of the Cosmic Background Radiation Spectrum / Mandolesi,N (TESRE, Bologna) ; Cortiglioni, S (TESRE, Bologna) ; Morigi, G (TESRE, Bologna) ; Sironi, G (Milan U.) ; Bonelli,G (Milan U.) ; Danese, G (U. Padua, Dept. Phys. Astron.) ; de Zotti, L (U. Padua, Dept. Phys. Astron.) ; Partridge, R B (Haverford Coll.) ; Smoot, G F (UC, Berkeley, Space Sci. Dept. ; UC, Berkeley) ; De Amici, G (UC, Berkeley, Space Sci. Dept. ; UC, Berkeley) et al.
Measurements of the Cosmic Background Radiation (CBR) temperature have been performed at five wavelengths ranging from 0.33 to 12 cm. The results give a weighted average of 2.72 ~ 0.04 Kin agreement with the most recent data at higher frequencies and constrain possible Compton distorsions to less than 5%..
1986 - 4 p. - Published in : ESO Conf. Workshop Proc. (1986) , pp. 117-120 Fulltext: PDF;
In : 2nd ESO/CERN Symposium on Cosmology, Astronomy and Fundamental Physics, Garching, Germany, 17 - 21 Mar 1986, pp.117-120
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2.
Structure in the COBE differential microwave radiometer first-year maps / Smoot, G F ; Bennett, C L ; Kogut, A ; Wright, E L ; Aymon, J ; Boggess, N W ; Cheng, E S ; De Amici, G ; Gulkis, S ; Hauser, M G et al.
1992 - Published in : Astrophys. J. Lett.: 396 (1992) , no. 1.2, pp. L1-L5
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