SMA Tutorials: Difference between revisions
From CASA Guides
Jump to navigationJump to search
No edit summary |
No edit summary |
||
| (One intermediate revision by the same user not shown) | |||
| Line 1: | Line 1: | ||
The following example starts with data that had been filled in MIRIAD and exported to FITS. The SMA group has | The following example starts with data that had been filled in MIRIAD and exported to FITS. The SMA group has | ||
recently written a filler to load SMA data directly into CASA, called [https://github.com/kenyoung/sma2casa sma2casa] which is publicly available. | recently written a filler to load SMA data directly into CASA, called [https://github.com/kenyoung/sma2casa sma2casa] which is publicly available on github. There is an announcement mailing list maintained by the author. | ||
* SMA Mosaic Observation of an Infrared Dark Cloud in CO(2-1) | * SMA Mosaic Observation of an Infrared Dark Cloud in CO(2-1) | ||
** Data reduction, Imaging, and Calibration:[[SMA CO Line Data 3.2]] | ** Data reduction, Imaging, and Calibration:[[SMA CO Line Data 3.2]] | ||
Latest revision as of 17:37, 7 April 2014
The following example starts with data that had been filled in MIRIAD and exported to FITS. The SMA group has recently written a filler to load SMA data directly into CASA, called sma2casa which is publicly available on github. There is an announcement mailing list maintained by the author.
- SMA Mosaic Observation of an Infrared Dark Cloud in CO(2-1)
- Data reduction, Imaging, and Calibration:SMA CO Line Data 3.2
