This page will hold our notes from implementing first fringes on an OUS level ALMA restore, as tracked in JIRA:
SSA-4811 - Getting issue details... STATUS .
Test Data Set Details:
Project 2017.1.00886.L MOUS ID: uid://A001/X1284/X265f made up of four ASDM EBs: uid://A002/Xc7111c/X3979, uid://A002/Xc7111c/X409e, uid://A002/X7111c/X86a7, uid://A002/Xc72427/X2dfe All these were processed recently, so have the calibration products stored separately (note though the data are still proprietary, so should not be shown too widely).
PPR Examples:
Kana was kind enough to provide a few example PPRs that perform multi-eb processing:
- A combined calibration/imaging run for an OUS for 2 EBs from a single Session: calimage_2eb_1session_PPR_uid___A001_X12cc_X4b.xml
- A calibration-only run for an OUS containing 2 EBs which spanned 2 Sessions: calonly_2eb_2session_PPR_uid___A001_X1284_X267.xml
- An imaging-only run for an OUS containing 2 EBs which spanned 2 Sessions: imageonly_2eb_2session_PPR_uid___A001_X1284_X267.xml
I'm just starting in on understanding these, and comparing them with the PPRs for CIPL and Vlass quicklook imaging.
Software Details:
For our test data set, we want to be using CASA/pipeline version 5.1.1-5r40896. This is the ALMA-approved version of CASA for Cycle 5. See: https://almascience.nrao.edu/processing/science-pipeline
We'll need an introduction to the ACSSW tools beyond asdmExportLight. In particular the calibration access (CalDMexport?) & PPR building (pipelineMakeRequest, pipelineShowRequest) tools will be relevant.
We'll need to know where the current ACSSW suite is installed in CV. SSA may also need to update the version of ACSSW in /home/ssa/ACS, as we are currently using a version tagged for Cycle 3.