techniques:interferometric相关论文
The National Solar Observatory is currently developing the Accurate Infrared Magnetic Field Measurements of the Sun(AIMS......
Deconvolution is used to eliminate imperfections in the point spread function,such as sidelobes caused by incomplete sam......
A sky model from CLEAN deconvolution is a particularly effective high dynamic range reconstruction in radio astronomy,wh......
In 21 cm intensity mapping,the spectral smoothness of the foreground is exploited to separate it from the much weaker 21......
SiO maser VLBA observations toward VX Sgr are performed at five epochs,and lots of maser spots are obtained.We make a st......
Deconvolution is used to eliminate imperfections in the point spread function,such as sidelobes caused by incomplete sam......
The Square Kilometre Array(SKA)would be the world’s largest radio telescope with eventually over a square kilometre of ......
In 21 cm intensity mapping,the spectral smoothness of the foreground is exploited to separate it from the much weaker 21......
A sky model from CLEAN deconvolution is a particularly effective high dynamic range reconstruction in radio astronomy,wh......
SiO maser VLBA observations toward VX Sgr are performed at five epochs, and lots of maser spots are obtained. We make a ......
The success of LISA Pathfinder in demonstrating the LISA drag-free requirement paved the way for using space interferome......
Radio interferometers are used to construct high resolution images of the sky at radio frequencies and are the key instr......
