A new receiver for the Onsala 20 m antenna with the possibility of being equipped with 3 mm and 4 mm bands has been built and the 3 mm channel has been commissioned during the Spring 2014. For single-dish operation, the receiver uses an innovative on-source/off-source optical switch. In combination with additional optical components and within the same optical layout, the switch provides two calibration loads (for the 3 mm and 4 mm channels), sideband rejection measurement, and tuning possibilities. The optical layout of the receiver employs all cold (4 K) offset elliptical mirrors for both channels, whereas the on-off switch employs flat mirrors only. The 3 mm channel employs a sideband separation (2SB) dual polarization receiver with orth...
Context. The Atacama Large Millimeter/submillimeter Array (ALMA) has been in operation since 2011, b...
Context. The Atacama Large Millimeter/submillimeter Array (ALMA) has been in operation since 2011, b...
Radio astronomy sources emit a very low signal of the order of 10. Therefore, in order to detect a ...
A new receiver for the Onsala 20 m antenna with the possibility of being equipped with 3 mm and 4 mm...
We present the design and the first light results for the new dual band receiver (4 mm and 3 mm band...
We present the design and the first light results for the new dual band receiver (4 mm and 3 mm band...
We describe the design of an integrated cryogenic receiver module based on an “active” waveguide Ort...
The work of this research is the design, analysis and verification of the optical performance of a 4...
This thesis outlines several different topics associated with the design and analysis of millimetre...
The work of this research is the design, analysis and verification of the optical performance of a 4...
The work of this research is the design, analysis and verification of the optical performance of a 4...
This thesis outlines several different topics associated with the design and analysis of millimetre...
This thesis outlines several different topics associated with the design and analysis of millimetre...
This thesis outlines several different topics associated with the design and analysis of millimetre ...
The work of this research is the design, analysis and verification of the optical performance of a 4...
Context. The Atacama Large Millimeter/submillimeter Array (ALMA) has been in operation since 2011, b...
Context. The Atacama Large Millimeter/submillimeter Array (ALMA) has been in operation since 2011, b...
Radio astronomy sources emit a very low signal of the order of 10. Therefore, in order to detect a ...
A new receiver for the Onsala 20 m antenna with the possibility of being equipped with 3 mm and 4 mm...
We present the design and the first light results for the new dual band receiver (4 mm and 3 mm band...
We present the design and the first light results for the new dual band receiver (4 mm and 3 mm band...
We describe the design of an integrated cryogenic receiver module based on an “active” waveguide Ort...
The work of this research is the design, analysis and verification of the optical performance of a 4...
This thesis outlines several different topics associated with the design and analysis of millimetre...
The work of this research is the design, analysis and verification of the optical performance of a 4...
The work of this research is the design, analysis and verification of the optical performance of a 4...
This thesis outlines several different topics associated with the design and analysis of millimetre...
This thesis outlines several different topics associated with the design and analysis of millimetre...
This thesis outlines several different topics associated with the design and analysis of millimetre ...
The work of this research is the design, analysis and verification of the optical performance of a 4...
Context. The Atacama Large Millimeter/submillimeter Array (ALMA) has been in operation since 2011, b...
Context. The Atacama Large Millimeter/submillimeter Array (ALMA) has been in operation since 2011, b...
Radio astronomy sources emit a very low signal of the order of 10. Therefore, in order to detect a ...