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On the Large-Scale Anisotropy of the Cosmic Background Radiation in the Far Infrared

Published online by Cambridge University Press:  04 August 2017

P. Boynton ,
C. Ceccarelli ,
P. de Bernardis ,
S. Masi ,
B. Melchiorri ,
F. Melchiorri ,
G. Moreno  and
V. Natale
P. Boynton
Affiliation:
Dept. of Physics, University of Washington, Seattle
C. Ceccarelli
Affiliation:
Istituto di Fisica Università di Roma
P. de Bernardis
Affiliation:
Istituto di Fisica Università di Roma
S. Masi
Affiliation:
Istituto di Fisica Università di Roma
B. Melchiorri
Affiliation:
Istituto di Fisica Università di Roma
F. Melchiorri
Affiliation:
Istituto di Fisica Università di Roma
G. Moreno
Affiliation:
Istituto di Fisica Università di Roma
V. Natale
Affiliation:
Istituto Onde Elettromagnetiche, C.N.R., Firenze

Abstract

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We report preliminary results relative to a balloon-borne search for the large-scale anisotropy carried out in 1980 by means of two far infrared photometers centered at 400 and 1100 microns. While these results are consistent with those obtained in an earlier flight, the second, shorter wavelength channel included in the 1980 work provides interesting insights into the influence of galactic dust on such far infrared observations.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 104: Early Evolution of the Universe and Its Present Structure , 1983 , pp. 139 - 141
Copyright
Copyright © Reidel 1983 

References

Ceccarelli, C., Dall'Oglio, G., Melchiorri, F., Pietranera, P. 1982, Ap. J., 260, 484.Google Scholar
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Melchiorri, F., Melchiorri, B., Ceccarelli, C., Pietranera, P. 1981, Ap. J. Lett., 250, L1.Google Scholar
Fabbri, R., Guidi, I., Natale, V. 1982, preprint.Google Scholar