Add to ORKGThe Caltech Millimeter-Wave Interferometer has recently begun observations at a wavelength of 2.6 mm. We describe the instrument and some of the first results from it
The Caltech Submillimeter Observatory (CSO) operates at the summit of Mauna Kea, Hawaii, at an eleva...
xiii, 167 leaves : ill. ; 28 cm.The performance of existing and planned millimeter and submillimeter...
A new heterodyne interferometer for the atmospheric window from 9 to 12 microns was developed during...
The Caltech Millimeter-Wave Interferometer has recently begun observations at a wavelength of 2.6 mm...
A brief description of the history and technology of the Caltech Submillimeter Observatory (CSO) is ...
The system components, performance, and calibration of two element radio interferometer operating at...
The planets and their satellites were observed at high resolution at millimeter wavelengths with the...
The development of millimeter and submillimeter interferometers was basically motivated by the disc...
The present status and projected two year developments for the Owens Valley Millimeter Array are des...
The James Clerk Maxwell Telescope (JCMT) and the Caltech Submillimeter Observatory (CSO) are located...
This thesis describes my work on the project to connect the James Clerk Maxwell Telescope (JCMT) and...
69 leaves : ill. ; 28 cm.Bibliography: leaf 69.Online version unavailable; print version available f...
We present results from the engineering run of the BOLOCAM receiver at the Caltech Submillimeter Obs...
Phase fluctuations introduced by the atmosphere are the main limiting factor in attaining diffractio...
xii, 143 leaves : ill. ; 28 cm.The performance of astronomical interferometer arrays operating at (s...
The Caltech Submillimeter Observatory (CSO) operates at the summit of Mauna Kea, Hawaii, at an eleva...
xiii, 167 leaves : ill. ; 28 cm.The performance of existing and planned millimeter and submillimeter...
A new heterodyne interferometer for the atmospheric window from 9 to 12 microns was developed during...
The Caltech Millimeter-Wave Interferometer has recently begun observations at a wavelength of 2.6 mm...
A brief description of the history and technology of the Caltech Submillimeter Observatory (CSO) is ...
The system components, performance, and calibration of two element radio interferometer operating at...
The planets and their satellites were observed at high resolution at millimeter wavelengths with the...
The development of millimeter and submillimeter interferometers was basically motivated by the disc...
The present status and projected two year developments for the Owens Valley Millimeter Array are des...
The James Clerk Maxwell Telescope (JCMT) and the Caltech Submillimeter Observatory (CSO) are located...
This thesis describes my work on the project to connect the James Clerk Maxwell Telescope (JCMT) and...
69 leaves : ill. ; 28 cm.Bibliography: leaf 69.Online version unavailable; print version available f...
We present results from the engineering run of the BOLOCAM receiver at the Caltech Submillimeter Obs...
Phase fluctuations introduced by the atmosphere are the main limiting factor in attaining diffractio...
xii, 143 leaves : ill. ; 28 cm.The performance of astronomical interferometer arrays operating at (s...
The Caltech Submillimeter Observatory (CSO) operates at the summit of Mauna Kea, Hawaii, at an eleva...
xiii, 167 leaves : ill. ; 28 cm.The performance of existing and planned millimeter and submillimeter...
A new heterodyne interferometer for the atmospheric window from 9 to 12 microns was developed during...