Explain each file. If you want to get an image go to quick_start.md, if you want to understand the steps go to Overview.md, if you are more advanced and want to start playing with the parameters to hone in your data combination go to DC_pars? General overview.md X Preparation.md (only once) Quick_start.md DC_pars.md – link to Template_pars.py and explain DC_run.md
These should be the steps that allow you to reproduce the figures in the paper:
- Ensure your CASA has astropy installed
- Ensure the analysisUtilities are installed for your CASA
- Run configure to be able to run the CASA based scripts
- Gather the data (see ../data/README_DC2019_data)
- Execfile DC_script.py to run through your selected data set
Details are given in Preparation You have to make these adjustments just once.
Details are in ../data/README_DC2019_data
This suggests that the data is present in ../data, physically or via a symlink.
At each start of a CASA instance you have to call the DC_locals.py once to set up your source and destination folders, e.g.
execfile("/home/teuben/dc2019/scripts4paper/DC_locals.py",globals())
DC_script.py is a wrapper that calls the DC_pars-file you defined in there and then the combination program DC_run.py.
Alternatively, you can call
execfile("/home/teuben/dc2019/scripts4paper/DC_pars_M100.py", globals())
execfile("/home/teuben/dc2019/scripts4paper/DC_run.py",globals())
An overview of the capabilities of DC_run.py is given in Overview and in more detail in DC_run. A quick start guide is given in Quick_start.
DC_run.py uses the python module datacomb.py for preparation and combination of the data and the python module IQA_script.py for the assessment of the combination products. Both modules can be used as a stand-alone.
This is a discussion how the DC2019 data should be circulated, and easily match a CASA tasks API for the different combination techniques discussed in the paper
Each method team should provide the way how the data teams should be calling that method:
- feather -
- tp2vis - experimenting with CASA 6
- sdint - upcoming in CASA 5.7
- faridani (?) - is also in QAC
- hybrid (?) - not really easily available, but a promising option
The data will be prepared in a form ready for the different methods API's:
- M100 (line)
- Lupus (line)
- Line data (from workshop) here: https://ftp.astro.umd.edu/pub/teuben/tp2vis/Lup3mms_12CO_tp_7m_12m_nchan10.tgz
- Images (preliminary combination): https://astrocloud.nrao.edu/s/Np7STzGMMY9fCWz
- Adele's script here: https://github.com/teuben/dc2019/blob/master/scripts/datacomb2019_outflowsWG.py
- HI (line)
- N346(line)
- skymodel (cont)
- Script for imaging the individual simulated datasets by Dirk Petry using the hogbom deconvolver https://github.com/teuben/dc2019/blob/master/scripts4paper/scriptForImaging.py
- ...
The final data will NOT be in github, we will use the UMD ftp server for this. Contact peter to provide a link so we can make it available to others. Currently this is https://ftp.astro.umd.edu/pub/teuben/DC2019/scripts4paper/ but that name may change.