Pilot study of Sgr B2 in preparation for WP2 of ACES. Below outlines the workflow for team decomposition of the Sgr B2 data.
- Fork the repository to your own branch
- Clone github repo using
git clone https://github.com/<yourusername>/WP2_pilot.git
- Download relevant data from globus including
HC3N_TP_7m_12m_feather.fits
andHC3N_TP_7m_12m_feather.mask2d.fits
- Move data cube and mask into local repo (.gitignore will prevent them from being uploaded to github post-decomposition)
- Assign issue to your name on github
- Create a local branch using
git checkout -b s1.XX.scousepy
whereXX
is the chunk number you are wanting to decompose - Update
run_scouse_chunks.py
with relevant assigned chunk numberXX
- Run
run_scouse_chunks.py
to completion - Note any problematic spectra as you go along (if there are any)
- Once completed commit your changes (remember to tag the issue in the commit
remarks using e.g. #1) and push to branch using
git push origin s1.XX.scousepy
- Create a pull request to
main
, again tagging the issue number in the comments - Update the issue comments with any problems encountered during fitting