The authors report the results of measurements of the cosmic background radiation temperature at wavelengths of 9.1 and 3.3 mm. The 9.1 mm result, T{sub CBR} = 2.87 {+-} 0.21 K, is in good agreement with previous results and those obtained at longer wavelengths during the same experiment. The 3.3 mm result, T{sub CBR} = 2.4 {+-} 1.0 K, is consistent with previous measurements, but has a large error due to uncertainty in the atmospheric correction
Observations carried out from an Alpine location (3500 m) using a Dicke-type radiometer with a broad...
Context. According to the Big Bang theory and as a consequence of adiabatic expansion of the Univers...
The absolute temperature of the cosmic microwave back- ground (CMB) has been measured at a frequency...
We have measured the temperature of the cosmic background radiation (CBR) at 3.3 mm wavelength in 19...
We have measured the temperature of the cosmic background radiation (CBR) at a frequency of 3.8 GHz ...
New measurements of the cosmic background radiation (CBR) intensity at 4.75 GHz (6.3 cm), made as a ...
We measured the temperature of the cosmic background radiation (CBR) at a frequency of 3.7 GHz (8.1 ...
We have measured the temperature of the cosmic microwave background radiation at wavelengths of 0.33...
We have measured the intensity of the cosmic microwave background (CMB) at a frequency of 7.5 GHz (w...
The intensity of the cosmic background radiation (CBR) has been measured at a wavelength of 3.0 cm a...
The spectrum of the cosmic background radiation (CBR) has been measured using a liquid helium cooled...
This paper presents an analysis of the results of recent temperature measurements of the cosmic micr...
This paper reviews the three major cosmic microwave background radiation (CMBR) spectrum measurement...
We have made measurements of the cosmic background radiation spectrum at 5 wavelengths (0.33, 0.9, 3...
An experimental measurement of the spectrum of the submillimeter cosmic background radiation is desc...
Observations carried out from an Alpine location (3500 m) using a Dicke-type radiometer with a broad...
Context. According to the Big Bang theory and as a consequence of adiabatic expansion of the Univers...
The absolute temperature of the cosmic microwave back- ground (CMB) has been measured at a frequency...
We have measured the temperature of the cosmic background radiation (CBR) at 3.3 mm wavelength in 19...
We have measured the temperature of the cosmic background radiation (CBR) at a frequency of 3.8 GHz ...
New measurements of the cosmic background radiation (CBR) intensity at 4.75 GHz (6.3 cm), made as a ...
We measured the temperature of the cosmic background radiation (CBR) at a frequency of 3.7 GHz (8.1 ...
We have measured the temperature of the cosmic microwave background radiation at wavelengths of 0.33...
We have measured the intensity of the cosmic microwave background (CMB) at a frequency of 7.5 GHz (w...
The intensity of the cosmic background radiation (CBR) has been measured at a wavelength of 3.0 cm a...
The spectrum of the cosmic background radiation (CBR) has been measured using a liquid helium cooled...
This paper presents an analysis of the results of recent temperature measurements of the cosmic micr...
This paper reviews the three major cosmic microwave background radiation (CMBR) spectrum measurement...
We have made measurements of the cosmic background radiation spectrum at 5 wavelengths (0.33, 0.9, 3...
An experimental measurement of the spectrum of the submillimeter cosmic background radiation is desc...
Observations carried out from an Alpine location (3500 m) using a Dicke-type radiometer with a broad...
Context. According to the Big Bang theory and as a consequence of adiabatic expansion of the Univers...
The absolute temperature of the cosmic microwave back- ground (CMB) has been measured at a frequency...