Measurements of the cosmic background radiation through the 1.0-1.4-mm atmospheric window

G. Dall'Oglio, S. Fonti, B. Melchiorri, F. Melchiorri, V. Natale, P. Lombardini, P. Trivero, and S. Sivertsen
Phys. Rev. D 13, 1187 – Published 1 March 1976
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Abstract

Observations carried out from an Alpine location (3500 m) using a Dicke-type radiometer with a broad-band germanium bolometer have proved that the cosmic background radiation in the 900-1400-micron band can be measured from mountain altitudes with a precision comparable with that obtained in the 3.3-mm band. The inaccuracy in the measurements is attributed to calibration rather than to the atmospheric disturbances. The upper limit of 2.7°K observed is more stringent than that of previously reported balloon-borne and rocket-borne observations in the same band.

  • Received 30 October 1974

DOI:https://doi.org/10.1103/PhysRevD.13.1187

©1976 American Physical Society

Authors & Affiliations

G. Dall'Oglio, S. Fonti, B. Melchiorri, F. Melchiorri, and V. Natale

  • Laboratorio TeSRE-CNR, Infrared Section, Firenze, Italy

P. Lombardini and P. Trivero

  • Laboratorio di Cosmogeofisica, Torino, Italy

S. Sivertsen

  • Auroral Observatory, Tromsøe, Norway

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Issue

Vol. 13, Iss. 5 — 1 March 1976

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