ALMA North American Science Advisory Committee * L1521F: Dynamical interaction of star forming gas was found in a star forming region by observations wi...
NOTE: NONE OF THESE CHANGES ARE NEEDED ANY LONGER Until the script generator catches up to the CASA 4.2 release, here are changes you will have to make to your re...
computeAggregateBandwidth Return to directory of Todd's CASA extensions Computes the aggregate non overlapping bandwidth for a list of spws of a measurement set. ...
* To see if you are missing pointings: * look at the Field.xml file in the raw ASDM directory. There should be many fields listed. * OR: if you've alr...
Low SNR, Narrow bandwidth Data Reduction Some data have been collected with narrow/low bandwidth (FDM) spectral windows for all of the scans (science source, phas...
In CASA 4.2 and earlier, the weights column in a data set do not reflect the relative channel widths between SPWs. This turns out to be important for the imaging...
Band Width Switching Reduction Science observations that use very narrow band ("FDM") observations may be collected in an observing mode where some of the calibra...
Testing of May 2013 heuristics Note: If the link to the analyzemscal result is broken, this project has not been run through the new pipeline yet. * Older resu...
Testing of September 2013 heuristics Note: If the link to the analyzemscal result is broken, this project has not been run through the new pipeline yet. Please li...
Overview This wiki provides a procedure to repackage Cycle 1 data that has previously been delivered in the Cycle 0 style. Such data needs to be repackaged and in...
Scripts generated on 23 January 2014 and after should already be compatible with the scriptForPI.py. If you want to make a script generated before 23 January 201...
See this page for Dirk's instructions Steps to upload the fluxes so they can make it into the archive * After data reduction and the QA2 report are finished, a...